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12501480 | 1607.02567 | Running cosmological constant with observational tests | We investigate the running cosmological constant model with dark energy linearly proportional to the Hubble parameter, Λ = σH +Λ<SUB>0</SUB>, in which the ΛCDM limit is recovered by taking σ = 0. We derive the linear perturbation equations of gravity under the Friedmann-Lemaïtre-Robertson-Walker cosmology, and show the... | [
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... | 11.501476 | 1.152585 | 2016-07-01 | 11 | 2016PhLB..760..422G | [
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"Astrophysics - Cosmology and Nongalactic Astrophysics",
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] | 3 | [
"10.1016/j.physletb.2016.07.026",
"10.48550/arXiv.1607.02567"
] | [
"Geng, Chao-Qiang",
"Lee, Chung-Chi",
"Zhang, Kaituo"
] | [
"Chongqing University of Posts & Telecommunications, Chongqing, 400065, China",
"National Center for Theoretical Sciences, Hsinchu, 300, Taiwan",
"Anhui Normal University, Wuhu, Anhui, 24100, China"
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12458738 | 1607.00612 | Dark matter density spikes around primordial black holes | We show that density spikes begin to form from dark matter particles around primordial black holes immediately after their formation at the radiation-dominated cosmological stage. This stems from the fact that in the thermal velocity distribution of particles there are particles with low velocities that remain in finit... | [
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"gamma-ray astronomy",
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] | 9 | [
"10.1134/S1063773716060013",
"10.48550/arXiv.1607.00612"
] | [
"Eroshenko, Yu. N."
] | [
"Institute for Nuclear Research, Russian Academy of Sciences, Moscow, Russia"
] | [
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12614143 | 1607.08786 | Effective photon mass by Super and Lorentz symmetry breaking | In the context of Standard Model Extensions (SMEs), we analyse four general classes of Super Symmetry (SuSy) and Lorentz Symmetry (LoSy) breaking, leading to observable imprints at our energy scales. The photon dispersion relations show a non-Maxwellian behaviour for the CPT (Charge-Parity-Time reversal symmetry) odd a... | [
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0... | 8.539769 | 0.507883 | 2016-07-01 | 32 | 2017PhLB..764..203B | [
"odd CPT",
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"observable imprints",
"a non-Maxwellian behaviour",
"ground measurements",
"observation",
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"10.1016/j.physletb.2016.11.023",
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"Bonetti, Luca",
"dos Santos Filho, Luís R.",
"Helayël-Neto, José A.",
"Spallicci, Alessandro D. A. M."
] | [
"Université d'Orléans, Observatoire des Sciences de l'Univers en région Centre (OSUC), UMS 3116, 1A rue de la Férollerie, 45071 Orléans, France",
"Centro Brasileiro de Pesquisas Físicas (CBPF), Rua Xavier Sigaud 150, 22290-180 Urca, Rio de Janeiro, RJ, Brasil",
"Centro Brasileiro de Pesquisas Físicas (CBPF), Ru... | [
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900376 | 1607.08265 | A radio-pulsing white dwarf binary star | White dwarfs are compact stars, similar in size to Earth but approximately 200,000 times more massive. Isolated white dwarfs emit most of their power from ultraviolet to near-infrared wavelengths, but when in close orbits with less dense stars, white dwarfs can strip material from their companions and the resulting mas... | [
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... | 16.392759 | 13.133673 | 2016-07-01 | 135 | 2016Natur.537..374M | [
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"Astrophysics - Solar and Stellar Astrophysics",
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"10.1038/nature18620",
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"Marsh, T. R.",
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"Hümmerich, S.",
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"Schreiber, M. R.",
"Jonker, P. G.",
"van Roestel, J.",
"Kupfer, T.",
"Pala, A. F.",
"Dhillon, V. S.",... | [
"Department of Physics, Gibbet Hill Road, University of Warwick, Coventry CV4 7AL, UK;",
"Department of Physics, Gibbet Hill Road, University of Warwick, Coventry CV4 7AL, UK",
"Bundesdeutsche Arbeitsgemeinschaft für Veränderliche Sterne e.V. (BAV), Berlin, Germany; American Association of Variable Star Observe... | [
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2417607 | 1607.03494 | The Kepler Catalog of Stellar Flares | A homogeneous search for stellar flares has been performed using every available Kepler light curve. An iterative light curve de-trending approach was used to filter out both astrophysical and systematic variability to detect flares. The flare recovery completeness has also been computed throughout each light curve usi... | [
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"10.3847/0004-637X/829/1/23",
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"Davenport, James R. A."
] | [
"Department of Physics & Astronomy, Western Washington University, Bellingham, WA 98225, USA"
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12620005 | 1607.08862 | Cosmic rays in a galactic breeze | Motivated by the discovery of the nonthermal Fermi bubble features both below and above the Galactic plane, we investigate a scenario in which these bubbles are formed through galacto-centric outflow. Cosmic rays (CR) both diffusing and advecting within a galactic breeze outflow, interacting with the ambient gas presen... | [
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0.... | 7.488508 | 4.059526 | 2016-07-01 | 13 | 2017PhRvD..95b3001T | [
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"Astrophysics - High Energy Astrophysical Phenomena"
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"10.1103/PhysRevD.95.023001",
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"Taylor, Andrew M.",
"Giacinti, Gwenael"
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"Dublin Institute for Advanced Studies, 31 Fitzwilliam Place, Dublin 2, Ireland",
"Max-Planck-Institut für Kernphysik, Saupfercheckweg 1, D-69117 Heidelberg, Germany"
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12406391 | 1607.01943 | The warm absorber in the radio-loud quasar 4C +74.26 | Outflows of photoionized gas are commonly detected in the X-ray spectra of Seyfert 1 galaxies. However, the evidence for this phenomenon in broad line radio galaxies, which are analogous to Seyfert 1 galaxies in the radio-loud regime, has so far been scarce. Here, we present the analysis of the X-ray absorption in the ... | [
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] | [
"Di Gesu, L.",
"Costantini, E."
] | [
"SRON Netherlands Institute for Space Research, Sorbonnelaan 2, 3584 CA, Utrecht, The Netherlands; Department of Astronomy, University of Geneva, 16 Ch. d' Ecogia, 1290, Versoix, Switzerland",
"SRON Netherlands Institute for Space Research, Sorbonnelaan 2, 3584 CA, Utrecht, The Netherlands"
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12473067 | 1607.07879 | Finding binaries from phase modulation of pulsating stars with Kepler - IV. Detection limits and radial velocity verification | We explore the detection limits of the phase modulation (PM) method of finding binary systems among multiperiodic pulsating stars. The method is an attractive way of finding non-transiting planets in the habitable zones of intermediate-mass stars, whose rapid rotation inhibits detections via the radial velocity (RV) me... | [
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] | 8 | [
"10.1093/mnras/stw1622",
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"Murphy, Simon J.",
"Shibahashi, Hiromoto",
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] | [
"Sydney Institute for Astronomy (SIfA), School of Physics, The University of Sydney, NSW 2006, Australia; Stellar Astrophysics Centre, Department of Physics and Astronomy, Aarhus University, DK-8000 Aarhus C, Denmark; Department of Astronomy, The University of Tokyo, Tokyo 113-0033, Japan",
"Department of Astrono... | [
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12614315 | 1607.00032 | A combined view of sterile-neutrino constraints from CMB and neutrino oscillation measurements | We perform a comparative analysis of constraints on sterile neutrinos from the Planck experiment and from current and future neutrino oscillation experiments (MINOS, IceCube, SBN). For the first time, we express joint constraints on N<SUB>eff</SUB> and m<SUB>eff</SUB><SUP>sterile</SUP> from the CMB in the Δm<SUP>2</SUP... | [
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0.01... | 6.99586 | -1.46747 | 2016-07-01 | 20 | 2017PhLB..764..322B | [
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"Sterile neutrinos",
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] | 6 | [
"10.1016/j.physletb.2016.11.050",
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] | [
"Bridle, Sarah",
"Elvin-Poole, Jack",
"Evans, Justin",
"Fernandez, Susana",
"Guzowski, Pawel",
"Söldner-Rembold, Stefan"
] | [
"The University of Manchester, School of Physics and Astronomy, Manchester, M13 9PL, United Kingdom",
"The University of Manchester, School of Physics and Astronomy, Manchester, M13 9PL, United Kingdom",
"The University of Manchester, School of Physics and Astronomy, Manchester, M13 9PL, United Kingdom",
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12462050 | 1607.05329 | Systematic treatment of non-linear effects in Baryon Acoustic Oscillations | In this contribution we will discuss the non-linear effects in the baryon acoustic oscillations and present a systematic and controllable way to account for them within time-sliced perturbation theory. | [
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... | 12.056767 | 2.420104 | 2016-07-01 | 0 | 2016EPJWC.12503006I | [
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] | 4 | [
"10.1051/epjconf/201612503006",
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] | [
"Ivanov, Mikhail M."
] | [
"FSB/IPHYS/LPPC, École Polytechnique Fédérale de Lausanne, CH-1015, Lausanne, Switzerland; Institute for Nuclear Research of the Russian Academy of Sciences, 60th October Anniversary Prospect, 7a, 117312, Moscow, Russia; Department of Particle Physics and Cosmology, Physics Faculty, Moscow State University, Vorobje... | null | [
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12511163 | 1607.00817 | Precise measurements of inflationary features with 21 cm observations | Future observations of 21 cm emission using neutral hydrogen intensity mapping will enable us to probe the large scale structure of the Universe over very large survey volumes within a reasonable observation time. We demonstrate that the three-dimensional information contained in such surveys will be an extremely power... | [
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... | [
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] | 7 | [
"10.1103/PhysRevD.94.123518",
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] | [
"Xu, Yidong",
"Hamann, Jan",
"Chen, Xuelei"
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"Key Laboratory for Computational Astrophysics, National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, China",
"Sydney Institute for Astronomy, The University of Sydney, Sydney, New South Wales 2006, Australia",
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12435851 | 1607.05745 | Ultra-High Energy Astrophysical Neutrino Detection, and the Search for Lorentz Invariance Violations | A growing class of ultra-high energy neutrino (UHE-nu) observatories based on the Askaryan effect and Antarctic ice is able to search for Lorentz invariance violation (LIV). The ARA, ARIANNA, ANITA and EVA collaborations have the power to constrain the Standard Model Extension (SME) by measuring the flux and energy dis... | [
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0.0... | 5.914657 | -0.686966 | 2016-07-01 | 0 | 2016arXiv160705745H | [
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"Astrophysics - High Energy Astrophysical Phenomena",
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"10.48550/arXiv.1607.05745"
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"Hanson, J. C."
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1513670 | 1607.02353 | Spectropolarimetry of Superluminous Supernovae: Insight into Their Geometry | We present the first spectropolarimetric observations of a hydrogen-free superluminous supernova (SLSN) at z = 0.1136, namely SN 2015bn. The transient shows significant polarization at both of the observed epochs: one 24 days before maximum light in the rest-frame, and the other at 27 days after peak luminosity. Analys... | [
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"Astrophysics - High Energy Astrophysical Phenomena",
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"10.3847/0004-637X/831/1/79",
"10.48550/arXiv.1607.02353"
] | [
"Inserra, C.",
"Bulla, M.",
"Sim, S. A.",
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"Astrophysics Research Centre, School of Mathematics and Physics, Queens University Belfast, Belfast BT7 1NN, UK",
"Astrophysics Research Centre, School of Mathematics and Physics, Queens University Belfast, Belfast BT7 1NN, UK",
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2570297 | 1607.07740 | Detecting pulsars with interstellar scintillation in variance images | Pulsars are the only cosmic radio sources known to be sufficiently compact to show diffractive interstellar scintillations. Images of the variance of radio signals in both time and frequency can be used to detect pulsars in large-scale continuum surveys using the next generation of synthesis radio telescopes. This tech... | [
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"expensive pixel-by-pixel high time resolution searches",
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... | [
"methods: observational",
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"Astrophysics - Instrumentation and Methods for Astrophysics",
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] | 10 | [
"10.1093/mnras/stw1871",
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"Dai, S.",
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"Bell, M. E.",
"Coles, W. A.",
"Hobbs, G.",
"Ekers, R. D.",
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"CSIRO Astronomy and Space Science, Australia Telescope National Facility, PO Box 76, Epping, NSW 1710, Australia",
"CSIRO Astronomy and Space Science, Australia Telescope National Facility, PO Box 76, Epping, NSW 1710, Australia",
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12595183 | 1607.05059 | High-energy gamma-rays from Cyg X-1 | We have obtained a firm detection of Cyg X-1 during its hard and intermediate spectral states in the energy range of 40 MeV-60 GeV based on observations by the Fermi Large Area Telescope, confirming the independent results at ≥60 MeV of a previous work. The detection significance is ≃8σ in the 0.1-10 GeV range. In the ... | [
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... | 16.096653 | 9.135248 | 2016-07-01 | 51 | 2017MNRAS.471.3657Z | [
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... | [
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"Astrophysics - High Energy Astrophysical Phenomena"
] | 4 | [
"10.1093/mnras/stx1846",
"10.48550/arXiv.1607.05059"
] | [
"Zdziarski, Andrzej A.",
"Malyshev, Denys",
"Chernyakova, Maria",
"Pooley, Guy G."
] | [
"Nicolaus Copernicus Astronomical Center, Polish Academy of Sciences, Bartycka 18, PL-00-716 Warszawa, Poland",
"Institut für Astronomie und Astrophysik Tübingen, Universität Tübingen, Sand 1, D-72076 Tübingen, Germany",
"School of Physical Sciences, Dublin City University, Glasnevin, Dublin 9, Ireland; DIAS, F... | [
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12473004 | 1607.00951 | Accretion of pristine gas and dilution during the formation of multiple-population globular clusters | We study the interaction of the early spherical GC wind powered by Type II supernovae (SNe II) with the surrounding ambient medium consisting of the gaseous disc of a star-forming galaxy at redshift z ≳ 2. The bubble formed by the wind eventually breaks out of the disc, and most of the wind moves directly out of the ga... | [
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"hydrodynamics",
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] | 6 | [
"10.1093/mnras/stw1583",
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] | [
"D'Ercole, A.",
"D'Antona, F.",
"Vesperini, E."
] | [
"INAF, Osservatorio Astronomico di Bologna, via Ranzani 1, I-40127 Bologna, Italy",
"INAF, Osservatorio Astronomico di Roma, Via Frascati 33, I-00040 Monteporzio Catone (Roma), Italy",
"Department of Astronomy, Indiana University, Swain West, 727 E. 3rd Street, Bloomington, IN 47405 USA"
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12510952 | 1607.06093 | Galactic cosmic-ray propagation in the light of AMS-02: Analysis of protons, helium, and antiprotons | We present novel constraints on cosmic-ray propagation in the Galaxy using the recent precise measurements of proton and helium spectra from AMS-02, together with preliminary AMS-02 data on the antiproton over proton ratio. To explore efficiently the large (up to 11-dimensional) parameter space we employ the nested-sam... | [
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0.... | 6.854311 | 0.282234 | 2016-07-01 | 63 | 2016PhRvD..94l3019K | [
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"the solar modulation",
"the lo... | [
"Astrophysics - High Energy Astrophysical Phenomena",
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] | 14 | [
"10.1103/PhysRevD.94.123019",
"10.48550/arXiv.1607.06093"
] | [
"Korsmeier, Michael",
"Cuoco, Alessandro"
] | [
"Institute for Theoretical Particle Physics and Cosmology, RWTH Aachen University, 52056 Aachen, Germany",
"Institute for Theoretical Particle Physics and Cosmology, RWTH Aachen University, 52056 Aachen, Germany"
] | [
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12465028 | 1607.03952 | Scalar-tensor extension of the ΛCDM model | We construct a cosmological scalar-tensor-theory model in which the Brans-Dicke type scalar Φ enters the effective (Jordan-frame) Hubble rate as a simple modification of the Hubble rate of the ΛCDM model. This allows us to quantify differences between the background dynamics of scalar-tensor theories and general relati... | [
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-0.03586686402559280... | 10.375244 | 0.529473 | 2016-07-01 | 6 | 2016JCAP...11..034A | [
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"an effective fluid description",
"general relativity",
"old galaxies",
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"the effectiv... | [
"General Relativity and Quantum Cosmology",
"Astrophysics - Cosmology and Nongalactic Astrophysics",
"High Energy Physics - Theory"
] | 5 | [
"10.1088/1475-7516/2016/11/034",
"10.48550/arXiv.1607.03952"
] | [
"Algoner, W. C.",
"Velten, H. E. S.",
"Zimdahl, W."
] | [
"Departamento de Física, Universidade Federal do Espírito Santo, Av. Fernando Ferrari, 514, Campus de Goiabeiras, CEP 29075-910, Vitória, Espírito Santo, Brazil",
"Departamento de Física, Universidade Federal do Espírito Santo, Av. Fernando Ferrari, 514, Campus de Goiabeiras, CEP 29075-910, Vitória, Espírito Sant... | [
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5079399 | 1607.01020 | Far-reaching dust distribution in galaxy discs | In most studies of dust in galaxies, dust is only detected from its emission to approximately the optical radius of the galaxy. By combining the signal of 110 spiral galaxies observed as part of the Herschel Reference Survey, we are able to improve our sensitivity by an order of magnitude over that for a single object.... | [
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3996362 | 1607.06436 | Gain and Polarization Properties of a Large Radio Telescope from Calculation and Measurement: The John A. Galt Telescope | Measurement of the brightness temperature of extended radio emission demands knowledge of the gain (or aperture efficiency) of the telescope and measurement of the polarized component of the emission requires correction for the conversion of unpolarized emission from sky and ground to apparently polarized signal. Radia... | [
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12406343 | 1607.05954 | On the estimation of stellar parameters with uncertainty prediction from Generative Artificial Neural Networks: application to Gaia RVS simulated spectra | <BR /> Aims: We present an innovative artificial neural network (ANN) architecture, called Generative ANN (GANN), that computes the forward model, that is it learns the function that relates the unknown outputs (stellar atmospheric parameters, in this case) to the given inputs (spectra). Such a model can be integrated ... | [
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2409424 | 1607.02059 | HIRAX: a probe of dark energy and radio transients | The Hydrogen Intensity and Real-time Analysis eXperiment (HIRAX) is a new 400{800MHz radio interferometer under development for deployment in South Africa. HIRAX will comprise 1024 six meter parabolic dishes on a compact grid and will map most of the southern sky over the course of four years. HIRAX has two primary sci... | [
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... | 12.410657 | 3.229301 | 2016-07-01 | 211 | 2016SPIE.9906E..5XN | [
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"Karastergiou, A.",
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"McGill Univ. (Canada)",
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1208119 | 1607.06485 | Precision velocimetry planet hunting with PARAS: current performance and lessons to inform future extreme precision radial velocity instruments | The PRL Advanced Radial-velocity Abu-sky Search (PARAS) instrument is a fiber-fed stabilized high-resolution cross-dispersed echelle spectrograph, located on the 1.2 m telescope in Mt. Abu India. Designed for exoplanet detection, PARAS is capable of single-shot spectral coverage of 3800 - 9600 Å, and currently achievin... | [
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"10.1117/12.2232833",
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"Prasad, Neelam J. S. S. V.",
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"Pathan, F. M.",
"Anandarao, B. G."
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"The Pennsylvania State Univ. (United States)",
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"The Pennsylvania State Univ. (United States)",
"Physical Research Lab. (India)",
"Physical Research Lab. (India)",
"Physical Research Lab. (India)",
"Physical Research Lab. (India)",
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3941943 | 1607.06957 | Quasi-periodic Pulsations during the Impulsive and Decay phases of an X-class Flare | Quasi-periodic pulsations (QPPs) are often observed in X-ray emission from solar flares. To date, it is unclear what their physical origins are. Here, we present a multi-instrument investigation of the nature of QPP during the impulsive and decay phases of the X1.0 flare of 2013 October 28. We focus on the character of... | [
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"Hayes, L. A.",
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"Inglis, A. R.",
"Ryan, D. F."
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"School of Physics, Trinity College Dublin, Dublin 2, Ireland ; Solar Physics Laboratory, Heliophysics Science Division, NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA ; ADNET Systems, Inc., USA",
"School of Physics, Trinity College Dublin, Dublin 2, Ireland",
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12511058 | 1607.00737 | Study of WIMP annihilations into a pair of on-shell scalar mediators | In this article, we focus on new scalar ϕ mediated scalar/vectorial weakly interacting massive particles (WIMPs) with ϕ 's mass slightly below the WIMP mass. To explain the Galactic center 1-3 GeV gamma-ray excess, here we consider the case that a WIMP pair predominantly annihilates into an on-shell ϕ ϕ pair with ϕ mai... | [
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"High Energy Physics - Phenomenology",
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] | 5 | [
"10.1103/PhysRevD.94.095028",
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] | [
"Jia, Lian-Bao"
] | [
"School of Science, Southwest University of Science and Technology, Mianyang 621010, People's Republic of China"
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12471532 | 1607.08384 | Formation mechanisms of IMBH in globular clusters | We very briefly discuss proposed in the literature possible scenarios for intermediate mass black holes formation in globular clusters. We also discuss the results of the MOCCA simulations of about 2000 models (BigSurvey) regarding the distribution of events connected with electromagnetic and gravitational radiations, ... | [
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] | 4 | [
"10.48550/arXiv.1607.08384"
] | [
"Giersz, M.",
"Leigh, N.",
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] | [
"Nicolaus Copernicus Astronomical Centre, Polish Academy of Sciences, ul. Bartycka 18, 00-716 Warsaw, Poland,",
"Department of Astrophysics, American Museum of Natural History, Central Park West and 79th Street, New York, NY 10024",
"Leiden Observatory, Leiden University, PO Box 9513, NL-2300 RA Leiden, the Net... | [
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12585774 | 1607.03269 | General formalism for Fourier-based wave front sensing: application to the pyramid wave front sensors | We compare a set of wave front sensors (WFS) based on Fourier filtering technique. In particular, this study explores the "class of pyramidal WFS" defined as the 4-faces pyramid WFS, all its recent variations, and also some WFSs as the 3-faces pyramid WFS. First, we describe such a sensors class due to the optical para... | [
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"Fourier filtering technique",
"pyramidal WFS",
"WFS",
"performance specifications",
"sensitivity",
"faces",
"sensitivity and linearity range",
"incoming flux",
"wave front sensors",
"size",
"Fourier",
"influence",
"the modulation... | [
"Astrophysics - Instrumentation and Methods for Astrophysics"
] | 7 | [
"10.1117/1.JATIS.3.1.019001",
"10.48550/arXiv.1607.03269"
] | [
"Fauvarque, Olivier",
"Neichel, Benoit",
"Fusco, Thierry",
"Sauvage, Jean-Francois",
"Girault, Orion"
] | [
"Aix-Marseille Université, CNRS, Laboratoire d'Astrophysique de Marseille, UMR 7326, Marseille, France",
"Aix-Marseille Université, CNRS, Laboratoire d'Astrophysique de Marseille, UMR 7326, Marseille, France",
"ONERA-the French Aerospace Laboratory, Châtillon, France",
"ONERA-the French Aerospace Laboratory, ... | [
"2017arXiv170809044F",
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"2018JOSAA..35..594F",
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2523945 | 1607.06811 | Infrared High-resolution Integrated Light Spectral Analyses of M31 Globular Clusters from APOGEE | Chemical abundances are presented for 25 M31 globular clusters (GCs), based on moderately high resolution (R = 22,500) H-band integrated light (IL) spectra from the Apache Point Observatory Galactic Evolution Experiment (APOGEE). Infrared (IR) spectra offer lines from new elements, lines of different strengths, and lin... | [
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... | 9.236642 | 8.67336 | 2016-07-01 | 34 | 2016ApJ...829..116S | [
"optical abundances",
"optical Lick index abundances",
"Ti abundances",
"Chemical abundances",
"Integrated abundances",
"higher excitation potentials",
"OH molecular features",
"IR IL analyses",
"extragalactic GCs",
"lines",
"IR IL",
"atomic features",
"new elements",
"different strengths"... | [
"galaxies: abundances",
"galaxies: evolution",
"galaxies: individual: M31",
"galaxies: star clusters: general",
"globular clusters: general",
"Astrophysics - Astrophysics of Galaxies"
] | 8 | [
"10.3847/0004-637X/829/2/116",
"10.48550/arXiv.1607.06811"
] | [
"Sakari, Charli M.",
"Shetrone, Matthew D.",
"Schiavon, Ricardo P.",
"Bizyaev, Dmitry",
"Allende Prieto, Carlos",
"Beers, Timothy C.",
"Caldwell, Nelson",
"García-Hernández, D. A.",
"Lucatello, Sara",
"Majewski, Steven",
"O'Connell, Robert W.",
"Pan, Kaike",
"Strader, Jay"
] | [
"Department of Astronomy, University of Washington, Seattle WA 98195-1580, USA",
"McDonald Observatory, University of Texas at Austin, HC75 Box 1337-MCD, Fort Davis, TX 79734, USA",
"Gemini Observatory, 670 N. A'Ohoku Place, Hilo, HI 96720, USA ; Astrophysics Research Institute, Liverpool John Moores University... | [
"2017MNRAS.466.1010S",
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4188624 | 1607.02108 | Solar Coronal Jets: Observations, Theory, and Modeling | Coronal jets represent important manifestations of ubiquitous solar transients, which may be the source of significant mass and energy input to the upper solar atmosphere and the solar wind. While the energy involved in a jet-like event is smaller than that of "nominal" solar flares and coronal mass ejections (CMEs), j... | [
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0... | 12.823559 | 15.798986 | 2016-07-01 | 261 | 2016SSRv..201....1R | [
"ubiquitous solar transients",
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"the solar wind",
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"the solar activity",
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"Plasmas",
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"Sun: corona",
"Sun: magnetic fields",
"Sun: UV radiation",
"Sun: X-rays",
"Astrophysics - Solar and Stellar Astrophysics"
] | 28 | [
"10.1007/s11214-016-0260-5",
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] | [
"Raouafi, N. E.",
"Patsourakos, S.",
"Pariat, E.",
"Young, P. R.",
"Sterling, A. C.",
"Savcheva, A.",
"Shimojo, M.",
"Moreno-Insertis, F.",
"DeVore, C. R.",
"Archontis, V.",
"Török, T.",
"Mason, H.",
"Curdt, W.",
"Meyer, K.",
"Dalmasse, K.",
"Matsui, Y."
] | [
"The Johns Hopkins University Applied Physics Laboratory, Laurel, MD, USA",
"Department of Physics, University of Ioannina, Ioannina, Greece",
"LESIA, Observatoire de Paris, Meudon, France",
"College of Science, George Mason University, Fairfax, VA, USA; NASA/Goddard Space Flight Center, Greenbelt, MD, USA",
... | [
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12408793 | 1607.00380 | High-energy Neutrinos from Sources in Clusters of Galaxies | High-energy cosmic rays can be accelerated in clusters of galaxies, by mega-parsec scale shocks induced by the accretion of gas during the formation of large-scale structures, or by powerful sources harbored in clusters. Once accelerated, the highest energy particles leave the cluster via almost rectilinear trajectorie... | [
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... | 5.822984 | 0.014759 | 2016-07-01 | 31 | 2016ApJ...828...37F | [
"galaxy clusters",
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"high-energy cosmic rays",
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"cosmological time",
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"astroparticle physics",
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] | 2 | [
"10.3847/0004-637X/828/1/37",
"10.48550/arXiv.1607.00380"
] | [
"Fang, Ke",
"Olinto, Angela V."
] | [
"University of Maryland, Department of Astronomy, 1105 PSC, College Park, MD 20742, USA ; Joint Space-Science Institute, College Park, MD 20742, USA",
"Department of Astronomy & Astrophysics, Kavli Institute for Cosmological Physics, The University of Chicago, Chicago, Illinois 60637, USA"
] | [
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12464610 | 1607.07872 | Features from the non-attractor beginning of inflation | We study the effects of the non-attractor initial conditions for the canonical single-field inflation. The non-attractor stage can last only several e-folding numbers, and should be followed by hilltop inflation. This two-stage evolution leads to large scale suppression in the primordial power spectrum, which is favore... | [
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"the primordial power spectrum",
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"Astrophysics - Cosmology and Nongalactic Astrophysics",
"General Relativity and Quantum Cosmology",
"High Energy Physics - Phenomenology",
"High Energy Physics - Theory"
] | 4 | [
"10.1088/1475-7516/2016/10/017",
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] | [
"Cai, Yi-Fu",
"Gong, Jinn-Ouk",
"Wang, Dong-Gang",
"Wang, Ziwei"
] | [
"CAS Key Laboratory for Researches in Galaxies and Cosmology, University of Science and Technology of China, Chinese Academy of Sciences, Hefei, Anhui 230026, China",
"Asia Pacific Center for Theoretical Physics, Pohang 37673, Korea ; Department of Physics, Postech, Pohang 37673, Korea;",
"CAS Key Laboratory fo... | [
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1093459 | 1607.00725 | Location of γ-ray emission and magnetic field strengths in OJ 287 | Context. The γ-ray BL Lac object OJ 287 is known to exhibit inner-parsec "jet-wobbling", high degrees of variability at all wavelengths and quasi-stationary features, including an apparent (≈100°) position-angle change in projection on the sky plane. <BR /> Aims: Sub-50 micro-arcsecond resolution 86 GHz observations wi... | [
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0.... | 16.537378 | 5.591592 | 2016-07-01 | 71 | 2017A&A...597A..80H | [
"quasi-stationary features",
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"the downstream quasi-stationary feature",
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"a downstream stationary feature",
"projection",
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"BL Lacertae objects: individual: OJ 287",
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"galaxies: jets",
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] | 13 | [
"10.1051/0004-6361/201526727",
"10.48550/arXiv.1607.00725"
] | [
"Hodgson, J. A.",
"Krichbaum, T. P.",
"Marscher, A. P.",
"Jorstad, S. G.",
"Rani, B.",
"Marti-Vidal, I.",
"Bach, U.",
"Sanchez, S.",
"Bremer, M.",
"Lindqvist, M.",
"Uunila, M.",
"Kallunki, J.",
"Vicente, P.",
"Fuhrmann, L.",
"Angelakis, E.",
"Karamanavis, V.",
"Myserlis, I.",
"Nest... | [
"Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, 53121, Bonn, Germany; Korea Astronomy and Space Institute, 776 Daedeokdae-ro, Yuseong-gu, 34055, Daejeon, Korea",
"Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, 53121, Bonn, Germany",
"Institute for Astrophysical Research, Boston Universit... | [
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12578451 | 1607.07333 | Influence of a second satellite on the rotational dynamics of an oblate moon | The gravitational influence of a second satellite on the rotation of an oblate moon is numerically examined. A simplified model, assuming the axis of rotation perpendicular to the (Keplerian) orbit plane, is derived. The differences between the two models, i.e. in the absence and presence of the second satellite, are i... | [
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"oblate satellites",
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"The gravitational influence",
"the gravitational influence",
"a second satellite",
"the second satellite",
"the phase space",
"Keplerian",
"the oblate bo... | [
"Chaos",
"Planets and satellites",
"Rotation",
"Bifurcation diagrams",
"Astrophysics - Earth and Planetary Astrophysics",
"Nonlinear Sciences - Chaotic Dynamics",
"Physics - Space Physics"
] | 4 | [
"10.1007/s10569-016-9719-7",
"10.48550/arXiv.1607.07333"
] | [
"Tarnopolski, Mariusz"
] | [
"Astronomical Observatory of the Jagiellonian University, Kraków, Poland"
] | [
"2017A&A...606A..43T",
"2018IJBC...2830013K",
"2018exha.book.....P",
"2019CeMDA.131...33G",
"2020ApJ...899..103M",
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12472585 | 1607.07619 | MOCCA-SURVEY database I. Accreting white dwarf binary systems in globular clusters - I. Cataclysmic variables - present-day population | In this paper, which is the first in a series of papers associated with cataclysmic variables and related objects, we introduce the CATUABA code, a numerical machinery written for analysis of the MOCCA simulations, and show some first results by investigating the present-day population of cataclysmic variables in globu... | [
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-... | 5.481454 | 10.012635 | 2016-07-01 | 33 | 2016MNRAS.462.2950B | [
"cataclysmic variables",
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"globular clusters",
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"binary stellar evolution",
"no single cataclysmic variable",
"outbursts",
"strong dynamical interactions",
"place",
"Kroupa initial distributions",
"related objects",
"quiescence... | [
"methods: numerical",
"novae",
"cataclysmic variables",
"globular clusters: general",
"Astrophysics - Astrophysics of Galaxies"
] | 7 | [
"10.1093/mnras/stw1841",
"10.48550/arXiv.1607.07619"
] | [
"Belloni, Diogo",
"Giersz, Mirek",
"Askar, Abbas",
"Leigh, Nathan",
"Hypki, Arkadiusz"
] | [
"Nicolaus Copernicus Astronomical Centre, Polish Academy of Sciences, ul. Bartycka 18, PL-00-716 Warsaw, Poland; CAPES Foundation, Ministry of Education of Brazil, DF 70040-020 Brasilia, Brazil",
"Nicolaus Copernicus Astronomical Centre, Polish Academy of Sciences, ul. Bartycka 18, PL-00-716 Warsaw, Poland",
"N... | [
"2017MNRAS.464.2511H",
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1622440 | 1607.07934 | Satellite quenching time-scales in clusters from projected phase space measurements matched to simulated orbits | We measure the star formation quenching efficiency and time-scale in cluster environments. Our method uses N-body simulations to estimate the probability distribution of possible orbits for a sample of observed Sloan Digital Sky Survey galaxies in and around clusters based on their position and velocity offsets from th... | [
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-0.031... | 11.793753 | 6.391181 | 2016-07-01 | 89 | 2016MNRAS.463.3083O | [
"host cluster mass",
"cluster environments",
"previous group hosts",
"clusters",
"star formation",
"their host cluster",
"satellite galaxies",
"most ∼2 Gyr",
"Higher mass satellites",
"galaxy",
"a galaxys present-day host cluster",
"velocity",
"possible orbits",
"offsets",
"Gyr",
"the ... | [
"galaxies: clusters: general",
"galaxies: evolution",
"Astrophysics - Astrophysics of Galaxies"
] | 13 | [
"10.1093/mnras/stw2195",
"10.48550/arXiv.1607.07934"
] | [
"Oman, Kyle A.",
"Hudson, Michael J."
] | [
"Department of Physics and Astronomy, University of Victoria, Victoria, BC V8P 5C2, Canada; Department of Physics and Astronomy, University of Waterloo, Waterloo, ON N2L 3G1, Canada",
"Department of Physics and Astronomy, University of Waterloo, Waterloo, ON N2L 3G1, Canada; Perimeter Institute for Theoretical Ph... | [
"2016A&A...596A..11B",
"2017A&A...604A..54K",
"2017A&A...606A.108C",
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12473122 | 1607.04106 | Using baseline-dependent window functions for data compression and field-of-interest shaping in radio interferometry | In radio interferometry, observed visibilities are intrinsically sampled at some interval in time and frequency. Modern interferometers are capable of producing data at very high time and frequency resolution; practical limits on storage and computation costs require that some form of data compression be imposed. The t... | [
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] | 7 | [
"10.1093/mnras/stw1656",
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] | [
"Atemkeng, M. T.",
"Smirnov, O. M.",
"Tasse, C.",
"Foster, G.",
"Jonas, J."
] | [
"Department of Physics and Electronics, Rhodes University, PO Box 94, Grahamstown 6140, South Africa",
"Department of Physics and Electronics, Rhodes University, PO Box 94, Grahamstown 6140, South Africa; SKA South Africa, 3rd Floor, The Park, Park Road, Pinelands 7405, South Africa",
"Department of Physics and... | [
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12409587 | 1607.01453 | LAMOST Observations in the Kepler Field. Analysis of the Stellar Parameters Measured with LASP Based on Low-resolution Spectra | All 14 subfields of the Kepler field were observed at least once with the Large Sky Area Multi-Object Fiber Spectroscopic Telescope (lamost, Xinglong Observatory, China) during the 2012-2014 observation seasons. There are 88,628 reduced spectra with a signal-to-noise ratio in the g band (S/N<SUB> g </SUB>) ≥ 6 after th... | [
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"heliocentric radial velocity",
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] | 8 | [
"10.3847/0067-0049/225/2/28",
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] | [
"Ren, Anbing",
"Fu, Jianning",
"De Cat, Peter",
"Wu, Yue",
"Yang, Xiaohu",
"Shi, Jianrong",
"Luo, Ali",
"Zhang, Haotong",
"Dong, Subo",
"Zhang, Ruyuan",
"Zhang, Yong",
"Hou, Yonghui",
"Wang, Yuefei",
"Cao, Zihuang",
"Du, Bing"
] | [
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"Department of Astronomy, Beijing Normal University, No. 19 Xinjiekouwai Street, Haidian District, Beijing 100875, China",
"Royal observatory of Belgium, Ringlaan 3, B-1180 Brussel, Belgium... | [
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12464875 | 1607.03984 | Radial stability of anisotropic strange quark stars | The influence of the anisotropy in the equilibrium and stability of strange stars is investigated through the numerical solution of the hydrostatic equilibrium equation and the radial oscillation equation, both modified from their original version to include this effect. The strange matter inside the quark stars is des... | [
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0.... | 5.153157 | 2.059477 | 2016-07-01 | 80 | 2016JCAP...11..012A | [
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"10.1088/1475-7516/2016/11/012",
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"Arbañil, José D. V.",
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"ITA—Instituto Tecnológico de Aeronáutica—Departamento de Física, 12228-900, São José dos Campos, São Paulo, Brazil ; UPN—Universidad Privada del Norte—Departamento de Ciencias, Av. Alfredo Mendiola 6062 Urb. Los Olivos, Lima, Lima, Perú;",
"ITA—Instituto Tecnológico de Aeronáutica—Departamento de Física, 12228-9... | [
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12408858 | 1607.04040 | Enhanced Star Formation of Less Massive Galaxies in a Protocluster at z = 2.5 | We investigate a correlation between star formation rate (SFR) and stellar mass for Hα emission-line galaxies (HAEs) in one of the richest protoclusters ever known at z ∼ 2.5, the USS 1558-003 protocluster. This study is based on a 9.7 hr narrowband imaging data with MOIRCS on the Subaru telescope. We are able to const... | [
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"galaxies: clusters: general",
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] | 10 | [
"10.3847/2041-8205/826/2/L28",
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"Hayashi, Masao",
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"Koyama, Yusei",
"Tadaki, Ken-ichi",
"Suzuki, Tomoko L.",
"Yamamoto, Moegi"
] | [
"Optical and Infrared Astronomy Division, National Astronomical Observatory, Mitaka, Tokyo 181-8588, Japan",
"Optical and Infrared Astronomy Division, National Astronomical Observatory, Mitaka, Tokyo 181-8588, Japan; Department of Astronomical Science, SOKENDAI (The Graduate University for Advanced Studies), Mita... | [
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12436863 | 1607.06874 | Polarized Scattering and Biosignatures in Exoplanetary Atmospheres | Polarized scattering in planetary atmospheres is computed in the context of exoplanets. The problem of polarized radiative transfer is solved for a general case of absorption and scattering, while Rayleigh and Mie polarized scattering are considered as most relevant examples. We show that (1) relative contributions of ... | [
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... | 7.209954 | 14.877765 | 2016-07-01 | 4 | 2016arXiv160706874B | [
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... | [
"Astrophysics - Earth and Planetary Astrophysics",
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] | 5 | [
"10.48550/arXiv.1607.06874"
] | [
"Berdyugina, S. V."
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"-"
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12593828 | 1607.01386 | Precision prediction of the log power spectrum | At translinear scales, the log power spectrum captures significantly more cosmological information than the standard power spectrum. At high wavenumbers k, the Fisher information in the standard power spectrum P(k) fails to increase in proportion to k, in part due to correlations between large- and small-scale modes. A... | [
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... | 11.98091 | 2.714142 | 2016-07-01 | 15 | 2017MNRAS.464L..21R | [
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"surveys",
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] | 4 | [
"10.1093/mnrasl/slw178",
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] | [
"Repp, A.",
"Szapudi, I."
] | [
"Institute for Astronomy, 2680 Woodlawn Dr., Honolulu, Hawaii 96822, USA",
"Institute for Astronomy, 2680 Woodlawn Dr., Honolulu, Hawaii 96822, USA"
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12594710 | 1607.00043 | Perturbative approach to covariance matrix of the matter power spectrum | We evaluate the covariance matrix of the matter power spectrum using perturbation theory up to dominant terms at 1-loop order and compare it to numerical simulations. We decompose the covariance matrix into the disconnected (Gaussian) part, trispectrum from the modes outside the survey (supersample variance) and trispe... | [
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0.034... | 11.997189 | 2.752573 | 2016-07-01 | 56 | 2017MNRAS.466..780M | [
"large volumes",
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"The full covariance matrix",
"higher k",
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"perturbation theory",
"the wave vectors k",
"trispectrum",
"k΄",
"a given survey volume",
"... | [
"cosmology: theory",
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] | 12 | [
"10.1093/mnras/stw3196",
"10.48550/arXiv.1607.00043"
] | [
"Mohammed, Irshad",
"Seljak, Uroš",
"Vlah, Zvonimir"
] | [
"Fermilab Center for Particle Astrophysics, Fermi National Accelerator Laboratory, Batavia, IL 60510-0500, USA",
"Physics, Astronomy Department, University of California, Berkeley, CA 94720, USA; Lawrence Berkeley National Laboratory, Berkeley, CA 94720, USA",
"Stanford Institute for Theoretical Physics and Dep... | [
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12472971 | 1607.07725 | Orphan γ-ray flares from relativistic blobs encountering luminous stars | We propose that γ-rays in blazars can be produced during encounters of relativistic blobs of plasma with radiation field produced by luminous stars within (or close to) the jet. The blob is expected to contain relativistic electrons which Comptonize stellar radiation to the GeV-TeV energies. Produced γ-rays can initiat... | [
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... | 16.782362 | 5.103937 | 2016-07-01 | 14 | 2016MNRAS.463L..26B | [
"sub-TeV energy range",
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"stellar radiation",
"radiation field",
"luminous stars",
"rays",
"relativistic blobs",
"relativistic electrons",
"GeV",
"the extreme orphan γ-ray flare",
"the stellar radiation",
"the GeV-TeV energies",
"the flat-spectrum radio",
"the relativistic blob/lumin... | [
"radiation mechanisms: non-thermal",
"stars: massive",
"galaxies: active",
"galaxies: individual: PKS 1222+21",
"gamma-rays: general",
"Astrophysics - High Energy Astrophysical Phenomena"
] | 2 | [
"10.1093/mnrasl/slw149",
"10.48550/arXiv.1607.07725"
] | [
"Banasiński, P.",
"Bednarek, W.",
"Sitarek, J."
] | [
"Department of Astrophysics, The University of Łódź, ul. Pomorska 149/153, PL-90-236 Łódź, Poland",
"Department of Astrophysics, The University of Łódź, ul. Pomorska 149/153, PL-90-236 Łódź, Poland",
"Department of Astrophysics, The University of Łódź, ul. Pomorska 149/153, PL-90-236 Łódź, Poland"
] | [
"2017A&A...604A..57V",
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"2019A&A...622A.175V",
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12594003 | 1607.03937 | Dynamics of stellar spin driven by planets undergoing Lidov-Kozai migration: paths to spin-orbit misalignment | Many exoplanetary systems containing hot Jupiters (HJs) exhibit significant misalignment between the spin axes of the host stars and the orbital angular momentum axes of the planets ('spin-orbit misalignment'). High-eccentricity migration involving Lidov-Kozai oscillations of the planet's orbit induced by a distant per... | [
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... | 8.184191 | 14.199554 | 2016-07-01 | 25 | 2017MNRAS.465.3927S | [
"significant misalignment",
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"stellar rotation period",
"planets",
"stellar binaries",
"the stellar spin evolution",
"the stellar spin axis",
"Secular spin-orbit resonances",
"spin-orbit angles",
"the stellar spin precession freque... | [
"celestial mechanics",
"planets and satellites: dynamical evolution and stability",
"planetary systems",
"stars: rotation",
"Astrophysics - Earth and Planetary Astrophysics"
] | 1 | [
"10.1093/mnras/stw3018",
"10.48550/arXiv.1607.03937"
] | [
"Storch, Natalia I.",
"Lai, Dong",
"Anderson, Kassandra R."
] | [
"TAPIR, Walter Burke Institute for Theoretical Physics, Mailcode 350-17, Caltech, Pasadena, CA 91125, USA; Cornell Center for Astrophysics and Planetary Science, Department of Astronomy, Cornell University, Ithaca, NY 14853, USA",
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12518205 | 1607.01874 | JUDE: An Ultraviolet Imaging Telescope pipeline | The Ultraviolet Imaging Telescope (UVIT) was launched as part of the multi-wavelength Indian AstroSat mission on 28 September, 2015 into a low Earth orbit. A 6-month performance verification (PV) phase ended in March 2016, and the instrument is now in the general observing phase. UVIT operates in three channels: visibl... | [
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"Rahna, P. T.",
"Sutaria, F.",
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"Bubbly, S. G."
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"Indian Institute of Astrophysics, Bengaluru, India",
"Department of Physics, Christ University, Bengaluru, India",
"Indian Institute of Astrophysics, Bengaluru, India",
"M. P. Birla Institute of Fundamental Research, Bengaluru, India",
"Department of Physics, Christ University, Bengaluru, India",
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12473014 | 1607.06453 | Numerical simulation of vertical oscillations in an axisymmetric thick accretion flow around a black hole | We study time evolution of rotating, axisymmetric, two-dimensional inviscid accretion flows around black holes using a grid-based finite difference method. We do not use reflection symmetry on the equatorial plane in order to inspect if the disc along with the centrifugal barrier oscillated vertically. In the inviscid ... | [
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0.... | 7.818083 | 5.458817 | 2016-07-01 | 5 | 2016MNRAS.462.3502D | [
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] | [
"Deb, Arnab",
"Giri, Kinsuk",
"Chakrabarti, Sandip K."
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"S. N. Bose National Centre for Basic Sciences, Block-JD, Sector 3, Salt Lake, Kolkata 700098, India",
"National Institute of Technical Teachers Training and Research, Block-FC, Sector 3, Salt Lake, Kolkata 700106, India",
"S. N. Bose National Centre for Basic Sciences, Block-JD, Sector 3, Salt Lake, Kolkata 70... | [
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12406286 | 1607.01045 | Taking stock of superluminous supernovae and long gamma-ray burst host galaxy comparison using a complete sample of LGRBs | Long gamma-ray bursts (LGRBs) and superluminous supernovae (SLSNe) are both explosive transients with very massive progenitor stars. Clues about the nature of the progenitors can be found by investigating environments in which such transients occur. While studies of LGRB host galaxies have a long history, dedicated obs... | [
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"Japelj, J.",
"Vergani, S. D.",
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"GEPI, Observatoire de Paris, PSL Research University, CNRS, Univ. Paris Diderot, Sorbonne Paris Cité, Place Jules Janssen, 92195, Meudon, France; INAF-Osservatorio Astronomico di Brera, via E. Bianchi 46, 23807, Merate, Ital... | [
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12408841 | 1607.08487 | A Second-order Divergence-constrained Multidimensional Numerical Scheme for Relativistic Two-fluid Electrodynamics | A new multidimensional simulation code for relativistic two-fluid electrodynamics (RTFED) is described. The basic equations consist of the full set of Maxwell’s equations coupled with relativistic hydrodynamic equations for separate two charged fluids, representing the dynamics of either an electron-positron or an elec... | [
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"10.3847/0004-637X/831/1/100",
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"Amano, Takanobu"
] | [
"Department of Earth & Planetary Science, University of Tokyo, 113-0033, Japan"
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12593957 | 1607.01790 | H0LiCOW - V. New COSMOGRAIL time delays of HE 0435-1223: H<SUB>0</SUB> to 3.8 per cent precision from strong lensing in a flat ΛCDM model | We present a new measurement of the Hubble Constant H<SUB>0</SUB> and other cosmological parameters based on the joint analysis of three multiply imaged quasar systems with measured gravitational time delays. First, we measure the time delay of HE 0435-1223 from 13-yr light curves obtained as part of the COSMOGRAIL pro... | [
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"_",
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] | 29 | [
"10.1093/mnras/stw3006",
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"Bonvin, V.",
"Courbin, F.",
"Suyu, S. H.",
"Marshall, P. J.",
"Rusu, C. E.",
"Sluse, D.",
"Tewes, M.",
"Wong, K. C.",
"Collett, T.",
"Fassnacht, C. D.",
"Treu, T.",
"Auger, M. W.",
"Hilbert, S.",
"Koopmans, L. V. E.",
"Meylan, G.",
"Rumbaugh, N.",
"Sonnenfeld, A.",
"Spiniello, C."... | [
"Laboratory of Astrophysics, Institute of Physics, Ecole Polytechnique Fédérale de Lausanne (EPFL), Observatoire de Sauverny, CH-1290 Versoix, Switzerland",
"Laboratory of Astrophysics, Institute of Physics, Ecole Polytechnique Fédérale de Lausanne (EPFL), Observatoire de Sauverny, CH-1290 Versoix, Switzerland",
... | [
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12407000 | 1607.01267 | Star-forming Activity in the H II Regions Associated with the IRAS 17160-3707 Complex | We present a multiwavelength investigation of star formation activity toward the southern H II regions associated with IRAS 17160-3707, located at a distance of 6.2 kpc with a bolometric luminosity of 8.3 × 10<SUP>5</SUP> L <SUB>⊙</SUB>. The ionized gas distribution and dust clumps in the parental molecular cloud are e... | [
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-0.041222814470529556... | 10.749811 | 10.685938 | 2016-07-01 | 14 | 2016AJ....152..146N | [
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"H II regions",
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] | 6 | [
"10.3847/0004-6256/152/5/146",
"10.48550/arXiv.1607.01267"
] | [
"Nandakumar, G.",
"Veena, V. S.",
"Vig, S.",
"Tej, A.",
"Ghosh, S. K.",
"Ojha, D. K."
] | [
"Indian Institute of Space Science and Technology, Thiruvananthapuram 695 547, India",
"Indian Institute of Space Science and Technology, Thiruvananthapuram 695 547, India",
"Indian Institute of Space Science and Technology, Thiruvananthapuram 695 547, India",
"Indian Institute of Space Science and Technology... | [
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12408731 | 1607.04674 | Merger Hydrodynamics of the Luminous Cluster RX J1347.5-1145 | We present an analysis of the complex gas hydrodynamics in the X-ray-luminous galaxy cluster RX J1347.5-1145 caught in the act of merging with a subcluster to its southeast using a combined 186 ks Chandra exposure, 2.5 times greater than previous analyses. The primary cluster hosts a sloshing cold front spiral traced b... | [
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"previous analyses",
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"7\\buildrel{\\prime\\prime}\\over",
"the subcluster infall shock",
"Chandra ... | [
"galaxies: clusters: general",
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"galaxies: interactions",
"X-rays: galaxies: clusters",
"Astrophysics - Cosmology and Nongalactic Astrophysics",
"Astrophysics - Astrophysics of Galaxies"
] | 6 | [
"10.3847/0004-637X/830/1/39",
"10.48550/arXiv.1607.04674"
] | [
"Kreisch, C. D.",
"Machacek, M. E.",
"Jones, C.",
"Randall, S. W."
] | [
"Max Planck Institute for Astrophysics, Karl-Schwarzschild-Strasse 1, D-85748 Garching bei München, Germany; Department of Physics, Washington University in St. Louis, One Brookings Drive, St. Louis, MO 63130, USA;",
"Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138, USA",
"Har... | [
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12473116 | 1607.08170 | The stability of tidal equilibrium for hierarchical star-planet-moon systems | Motivated by the current search for exomoons, this paper considers the stability of tidal equilibrium for hierarchical three-body systems containing a star, a planet, and a moon. In this treatment, the energy and angular momentum budgets include contributions from the planetary orbit, lunar orbit, stellar spin, planeta... | [
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... | 8.021957 | 14.763345 | 2016-07-01 | 10 | 2016MNRAS.462.2527A | [
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... | [
"planets and satellites: dynamical evolution and stability",
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] | 8 | [
"10.1093/mnras/stw1883",
"10.48550/arXiv.1607.08170"
] | [
"Adams, Fred C.",
"Bloch, Anthony M."
] | [
"Physics Department, University of Michigan, Ann Arbor, MI 48109, USA; Astronomy Department, University of Michigan, Ann Arbor, MI 48109, USA",
"Math Department, University of Michigan, Ann Arbor, MI 48109, USA"
] | [
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12520904 | 1607.04218 | Self-consistent Modeling of Reionization in Cosmological Hydrodynamical Simulations | The ultraviolet background (UVB) emitted by quasars and galaxies governs the ionization and thermal state of the intergalactic medium (IGM), regulates the formation of high-redshift galaxies, and is thus a key quantity for modeling cosmic reionization. The vast majority of cosmological hydrodynamical simulations implem... | [
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] | [
"Oñorbe, Jose",
"Hennawi, Joseph F.",
"Lukić, Zarija"
] | [
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1910377 | 1607.03438 | A spectroscopic analysis of a sample of narrow-line Seyfert 1 galaxies selected from the Sloan Digital Sky Survey | We revisited the spectroscopic characteristics of narrow-line Seyfert 1 galaxies (NLS1s) by analysing a homogeneous sample of 296 NLS1s at redshift between 0.028 and 0.345, extracted from the Sloan Digital Sky Survey (SDSS-DR7) public archive. We confirm that NLS1s are mostly characterized by Balmer lines with Lorentzi... | [
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] | 18 | [
"10.1093/mnras/stw1689",
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] | [
"Cracco, V.",
"Ciroi, S.",
"Berton, M.",
"Di Mille, F.",
"Foschini, L.",
"La Mura, G.",
"Rafanelli, P."
] | [
"Department of Physics and Astronomy, Padova University, Vicolo dell'Osservatorio 3, I-35122 Padova, Italy",
"Department of Physics and Astronomy, Padova University, Vicolo dell'Osservatorio 3, I-35122 Padova, Italy",
"Department of Physics and Astronomy, Padova University, Vicolo dell'Osservatorio 3, I-35122 P... | [
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12409116 | 1607.08036 | Lighting the Dark Molecular Gas: H<SUB>2</SUB> as a Direct Tracer | Robust knowledge of molecular gas mass is critical for understanding star formation in galaxies. The {{{H}}}<SUB>2</SUB> molecule does not emit efficiently in the cold interstellar medium, hence the molecular gas content of galaxies is typically inferred using indirect tracers. At low metallicity and in other extreme e... | [
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"10.3847/0004-637X/830/1/18",
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] | [
"Togi, Aditya",
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] | [
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"Ritter Astrophysical Research Center, University of Toledo, 2825 West Bancroft Street, M. S. 113, Toledo, OH 43606, USA"
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1248190 | 1607.02322 | Particle dynamics in discs with turbulence generated by the vertical shear instability | Context. Among the candidates for generating turbulence in accretion discs in situations with low intrinsic ionization, the vertical shear instability (VSI) has become an interesting candidate, since it relies purely on a vertical gradient in the angular velocity. Existing numerical simulations have shown that α-values... | [
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] | 4 | [
"10.1051/0004-6361/201527716",
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] | [
"Stoll, Moritz H. R.",
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] | [
"Institut für Astronomie und Astrophysik, Universität Tübingen, Auf der Morgenstelle 10, 72076, Tübingen, Germany",
"Institut für Astronomie und Astrophysik, Universität Tübingen, Auf der Morgenstelle 10, 72076, Tübingen, Germany"
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12406476 | 1607.05734 | Close-in planetesimal formation by pile-up of drifting pebbles | Context. The consistency of planet formation models suffers from the disconnection between the regime of small and large bodies. This is primarily caused by so-called growth barriers: the direct growth of larger bodies is halted at centimetre-sized objects and particular conditions are required for the formation of lar... | [
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] | 15 | [
"10.1051/0004-6361/201628983",
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] | [
"Drążkowska, J.",
"Alibert, Y.",
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] | [
"Institute for Computational Science, University of Zurich, Winterthurerstrasse 190, 8057, Zurich, Switzerland",
"Physikalisches Institut & Center for Space and Habitability, University of Bern, Sidlerstrasse 5, 3012, Bern, Switzerland",
"Institute for Computational Science, University of Zurich, Winterthur... | [
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12473526 | 1607.05996 | Magnetic field amplification during the common envelope phase | During the common envelope (CE) phase, a giant star in a binary system overflows its Roche lobe and unstable mass transfer leads to a spiral-in of the companion, resulting in a close binary system or in a merger of the stellar cores. Dynamo processes during the CE phase have been proposed as a mechanism to generate mag... | [
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-0.0... | 5.377532 | 10.891885 | 2016-07-01 | 53 | 2016MNRAS.462L.121O | [
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] | 11 | [
"10.1093/mnrasl/slw144",
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] | [
"Ohlmann, Sebastian T.",
"Röpke, Friedrich K.",
"Pakmor, Rüdiger",
"Springel, Volker",
"Müller, Ewald"
] | [
"Heidelberger Institut für Theoretische Studien, Schloss-Wolfsbrunnenweg 35, D-69118 Heidelberg, Germany; Institut für Theoretische Physik und Astrophysik, Universität Würzburg, Emil-Fischer-Str. 31, D-97074 Würzburg, Germany",
"Heidelberger Institut für Theoretische Studien, Schloss-Wolfsbrunnenweg 35, D-69118 H... | [
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1073937 | 1607.07394 | Constraints on SME Coefficients from Lunar Laser Ranging, Very Long Baseline Interferometry, and Asteroid Orbital Dynamics | Lorentz symmetry violations can be parametrized by an effective field theory framework that contains both General Relativity and the Standard Model of particle physics, called the Standard-Model Extension or SME. We consider in this work only the pure gravitational sector of the minimal SME. We present new constraints ... | [
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-0.016... | 8.809752 | 1.414252 | 2016-07-01 | 2 | 2016arXiv160707394L | [
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"both G... | [
"High Energy Physics - Phenomenology",
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] | 4 | [
"10.48550/arXiv.1607.07394"
] | [
"Le Poncin-Lafitte, C.",
"Bourgoin, A.",
"Hees, A.",
"Bouquillon, S.",
"Lambert, S.",
"Francou, G.",
"Angonin, M. -C.",
"Bailey, Q. G.",
"Hestroffer, D.",
"David, P.",
"Meynadier, F.",
"Wolf, P."
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] |
3330704 | 1607.02787 | NIBLES: an H I census of stellar mass selected SDSS galaxies. I. The Nançay H I survey | To investigate galaxy properties as a function of their total stellar mass, we obtained 21 cm H I line observations at the 100-m class Nançay Radio Telescope of 2839 galaxies from the Sloan Digital Sky Survey (SDSS) in the Local Volume (900 < cz < 12 000 km s<SUP>-1</SUP>), dubbed the Nançay Interstellar Baryons ... | [
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... | 11.756528 | 7.625579 | 2016-07-01 | 34 | 2016A&A...595A.118V | [
"-23 mag",
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"lt",
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"z</SUB",
"absolute SDSS z-band magn... | [
"galaxies: general",
"galaxies: distances and redshifts",
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"galaxies: photometry",
"radio lines: galaxies",
"Astrophysics - Astrophysics of Galaxies"
] | 25 | [
"10.1051/0004-6361/201528048",
"10.48550/arXiv.1607.02787"
] | [
"van Driel, W.",
"Butcher, Z.",
"Schneider, S.",
"Lehnert, M. D.",
"Minchin, R.",
"Blyth, S. -L.",
"Chemin, L.",
"Hallet, N.",
"Joseph, T.",
"Kotze, P.",
"Kraan-Korteweg, R. C.",
"Olofsson, A. O. H.",
"Ramatsoku, M."
] | [
"GEPI, Observatoire de Paris, CNRS, Université Paris Diderot, 5 place Jules Janssen, 92190, Meudon, France ; Station de Radioastronomie de Nançay, Observatoire de Paris, CNRS/INSU USR 704, Université d'Orléans OSUC, route de Souesmes, 18330, Nançay, France",
"University of Massachusetts, Astronomy Program, 536 LG... | [
"2016A&A...596A..60B",
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"2020ApJ...903..... | [
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2414370 | 1607.03674 | High-velocity extended molecular outflow in the star-formation dominated luminous infrared galaxy ESO 320-G030 | We analyze new high spatial resolution (~60 pc) ALMA CO(2-1) observations of the isolated luminous infrared galaxy ESO 320-G030 (d = 48 Mpc) in combination with ancillary Hubble Space Telescope optical and near infrared (IR) imaging, as well as VLT/SINFONI near-IR integral field spectroscopy. We detect a high-velocity ... | [
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-0.030708029866218567,... | 13.965998 | 8.05909 | 2016-07-01 | 40 | 2016A&A...594A..81P | [
"Ṁ",
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"Hubble Space Telescope",
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"pc",
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"~3 Myr",
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"the observed molecular outflow",
"the outflowing cold molecular gas",
"size~2.5... | [
"galaxies: ISM",
"galaxies: kinematics and dynamics",
"galaxies: starburst",
"galaxies: nuclei",
"radio lines: galaxies",
"Astrophysics - Astrophysics of Galaxies"
] | 10 | [
"10.1051/0004-6361/201628875",
"10.48550/arXiv.1607.03674"
] | [
"Pereira-Santaella, M.",
"Colina, L.",
"García-Burillo, S.",
"Alonso-Herrero, A.",
"Arribas, S.",
"Cazzoli, S.",
"Emonts, B.",
"Piqueras López, J.",
"Planesas, P.",
"Storchi Bergmann, T.",
"Usero, A.",
"Villar-Martín, M."
] | [
"Centro de Astrobiología (CSIC/INTA), Ctra de Torrejón a Ajalvir, km 4, 28850, Torrejón de Ardoz, Madrid, Spain; ASTRO-UAM, UAM, Unidad Asociada CSIC, 28049, Madrid, Spain; Department of Physics, University of Oxford, Keble Road, Oxford, OX1 3RH, UK",
"Centro de Astrobiología (CSIC/INTA), Ctra de Torrejón a Ajalv... | [
"2016ApJ...832..142Z",
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3332979 | 1607.04262 | Discovery of a high state AM CVn binary in the Galactic Bulge Survey | We report on the discovery of a hydrogen-deficient compact binary (CXOGBS J175107.6-294037) belonging to the AM CVn class in the Galactic Bulge Survey. Deep archival X-ray observations constrain the X-ray positional uncertainty of the source to 0.57 arcsec, and allow us to uniquely identify the optical and UV counterpa... | [
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... | 5.293944 | 10.092311 | 2016-07-01 | 19 | 2016MNRAS.462L.106W | [
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] | 3 | [
"10.1093/mnrasl/slw141",
"10.48550/arXiv.1607.04262"
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"Wevers, T.",
"Torres, M. A. P.",
"Jonker, P. G.",
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"Nelemans, G.",
"Steeghs, D.",
"Maccarone, T. J.",
"Heinke, C.",
"Hynes, R. I.",
"Udalski, A.",
"Kostrzewa-Rutkowska, Z.",
"Groot, P. J.",
"Gazer, R.",
"Szymański, M. K.",
"Britt, C. T.",
"Wyrzykowski, Ł.",
"Poleski... | [
"Department of Astrophysics/IMAPP, Radboud University, PO Box 9010, NL-6500 GL Nijmegen, the Netherlands",
"Department of Astrophysics/IMAPP, Radboud University, PO Box 9010, NL-6500 GL Nijmegen, the Netherlands; SRON, Netherlands Institute for Space Research, Sorbonnelaan 2, NL-3584 CA Utrecht, the Netherlands",... | [
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1649322 | 1607.01392 | Outbursts in Two New Cool Pulsating DA White Dwarfs | The unprecedented extent of coverage provided by Kepler observations recently revealed outbursts in two hydrogen-atmosphere pulsating white dwarfs (DAVs) that cause hours-long increases in the overall mean flux of up to 14%. We have identified two new outbursting pulsating white dwarfs in K2, bringing the total number ... | [
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-0.... | 5.80732 | 11.171803 | 2016-07-01 | 26 | 2016ApJ...829...82B | [
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] | 12 | [
"10.3847/0004-637X/829/2/82",
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] | [
"Bell, Keaton J.",
"Hermes, J. J.",
"Montgomery, M. H.",
"Gentile Fusillo, N. P.",
"Raddi, R.",
"Gänsicke, B. T.",
"Winget, D. E.",
"Dennihy, E.",
"Gianninas, A.",
"Tremblay, P. -E.",
"Chote, P.",
"Winget, K. I."
] | [
"Department of Astronomy, University of Texas at Austin, Austin, TX-78712, USA ; McDonald Observatory, Fort Davis, TX-79734, USA;",
"Department of Physics and Astronomy, University of North Carolina, Chapel Hill, NC-27599, USA ;",
"Department of Astronomy, University of Texas at Austin, Austin, TX-78712, USA ; ... | [
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13975199 | 1607.06098 | Constraining the baryon-dark matter relative velocity with the large-scale three-point correlation function of the SDSS BOSS DR12 CMASS galaxies | We search for a galaxy clustering bias due to a modulation of galaxy number with the baryon-dark matter relative velocity resulting from recombination-era physics. We find no detected signal and place the constraint b<SUB>v</SUB> < 0.01 on the relative velocity bias for the CMASS galaxies. This bias is an important ... | [
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0.00916... | 12.322242 | 2.464336 | 2016-07-01 | 47 | 2018MNRAS.474.2109S | [
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"the baryon-dark matter relative velocity",
"the relative velocity",
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] | 7 | [
"10.1093/mnras/stx2723",
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"Slepian, Zachary",
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"Chuang, Chia-Hsun",
"Gil-Marín, Héctor",
"Ho, Shirley",
"Kitaura, Francisco-Shu",
"McEwen, Joseph E.",
"Percival, Will J.",
"Ross, Ashley J.",
"Rossi, Graziano",
"Seo, Hee-Jong",
"Slosar, Anže",
"... | [
"Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138, USA",
"Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138, USA",
"Center for Cosmology and Astroparticle Physics, Department of Physics, The Ohio State University, OH 43210, USA",
"Department o... | [
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12408761 | 1607.08616 | Empirically Constrained Predictions for Metal-line Emission from the Circumgalactic Medium | The circumgalactic medium (CGM) is one of the remaining least constrained components of galaxies and as such has significant potential for advancing galaxy formation theories. In this work, we vary the extragalactic ultraviolet background for a high-resolution cosmological simulation of a Milky-Way-like galaxy and exam... | [
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0.... | 13.353544 | 8.166255 | 2016-07-01 | 26 | 2016ApJ...827..148C | [
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"galaxies: evolution",
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"10.3847/0004-637X/827/2/148",
"10.48550/arXiv.1607.08616"
] | [
"Corlies, Lauren",
"Schiminovich, David"
] | [
"Department of Astronomy, Columbia University, New York, NY 10027, USA",
"Department of Astronomy, Columbia University, New York, NY 10027, USA"
] | [
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12472750 | 1607.01737 | Quasi-periodicities in the anomalous emission events in pulsars B1859+07 and B0919+06 | A quasi-periodicity has been identified in the strange emission shifts in pulsar B1859+07 and possibly B0919+06. These events, first investigated by Rankin, Rodriguez & Wright in 2006, originally appeared disordered or random, but further mapping as well as Fourier analysis has revealed that they occur on a fairly ... | [
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... | 6.007601 | 4.07551 | 2016-07-01 | 21 | 2016MNRAS.461.3740W | [
"pulsar B1859",
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"radiation mechanisms: non-thermal",
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"Astrophysics - High Energy Astrophysical Phenomena",
"Astrophysics - Solar and Stellar Astrophysics"
] | 8 | [
"10.1093/mnras/stw1589",
"10.48550/arXiv.1607.01737"
] | [
"Wahl, Haley M.",
"Orfeo, Daniel J.",
"Rankin, Joanna M.",
"Weisberg, Joel M."
] | [
"Physics Department, University of Vermont, Burlington, VT 05405, USA",
"Physics Department, University of Vermont, Burlington, VT 05405, USA",
"Physics Department, University of Vermont, Burlington, VT 05405, USA",
"Physics and Astronomy Department, Carleton College, Northfield, MN 55057, USA"
] | [
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2152772 | 1607.06117 | A Brown Dwarf Census from the SIMP Survey | We have conducted a near-infrared (NIR) proper motion survey, the Sondage Infrarouge de Mouvement Propre, in order to discover field ultracool dwarfs (UCD) in the solar neighborhood. The survey was conducted by imaging ∼28% of the sky with the Caméra PAnoramique Proche-InfraRouge both in the southern hemisphere at the ... | [
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... | 7.017281 | 12.392218 | 2016-07-01 | 37 | 2016ApJ...830..144R | [
"2MASS PSC",
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... | [
"brown dwarfs",
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] | 13 | [
"10.3847/0004-637X/830/2/144",
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] | [
"Robert, Jasmin",
"Gagné, Jonathan",
"Artigau, Étienne",
"Lafrenière, David",
"Nadeau, Daniel",
"Doyon, René",
"Malo, Lison",
"Albert, Loïc",
"Simard, Corinne",
"Bardalez Gagliuffi, Daniella C.",
"Burgasser, Adam J."
] | [
"Département de physique and Observatoire du Mont-Mégantic, Université de Montréal, Montréal, QC H3C 3J7, Canada ; Département de Physique, Université de Montréal, C.P. 6128 Succ. Centre-ville, Montréal, QC, H3C 3J7, Canada ;;",
"Département de physique and Observatoire du Mont-Mégantic, Université de Montréal, M... | [
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2932983 | 1607.05925 | Multiwavelength study of the low-luminosity outbursting young star HBC 722 | Context. HBC 722 (V2493 Cyg) is a young eruptive star in outburst since 2010. Spectroscopic evidence suggests that the source is an FU Orionis-type object, with an atypically low outburst luminosity. <BR /> Aims: Because it was well characterized in the pre-outburst phase, HBC 722 is one of the few FUors from which we ... | [
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"California Institute",
"Spitzer",
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"stars: formation",
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] | 7 | [
"10.1051/0004-6361/201528061",
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"Kóspál, Á.",
"Ábrahám, P.",
"Acosta-Pulido, J. A.",
"Dunham, M. M.",
"García-Álvarez, D.",
"Hogerheijde, M. R.",
"Kun, M.",
"Moór, A.",
"Farkas, A.",
"Hajdu, G.",
"Hodosán, G.",
"Kovács, T.",
"Kriskovics, L.",
"Marton, G.",
"Molnár, L.",
"Pál, A.",
"Sárneczky, K.",
"Sódor, Á.",
... | [
"Konkoly Observatory, Research Centre for Astronomy and Earth Sciences, Hungarian Academy of Sciences, PO Box 67, 1525, Budapest, Hungary",
"Konkoly Observatory, Research Centre for Astronomy and Earth Sciences, Hungarian Academy of Sciences, PO Box 67, 1525, Budapest, Hungary",
"Instituto de Astrofísica de Can... | [
"2017A&A...597L..10K",
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12406078 | 1607.02996 | The effects of magnetic-field geometry on longitudinal oscillations of solar prominences: Cross-sectional area variation for thin tubes | Context. Solar prominences are subject to both field-aligned (longitudinal) and transverse oscillatory motions, as evidenced by an increasing number of observations. Large-amplitude longitudinal motions provide valuable information on the geometry of the filament-channel magnetic structure that supports the cool promin... | [
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0.01... | 12.57048 | 15.813916 | 2016-07-01 | 9 | 2016A&A...593A..64L | [
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"the field lines",... | [
"Sun: corona",
"Sun: filaments",
"prominences",
"Sun: oscillations",
"Sun: magnetic fields",
"Astrophysics - Solar and Stellar Astrophysics"
] | 3 | [
"10.1051/0004-6361/201628845",
"10.48550/arXiv.1607.02996"
] | [
"Luna, M.",
"Díaz, A. J.",
"Oliver, R.",
"Terradas, J.",
"Karpen, J."
] | [
"Instituto de Astrofísica de Canarias, 38205 La Laguna, Tenerife, Spain; Universidad de La Laguna, Dept. Astrofísica, 38206 La Laguna, Tenerife, Spain",
"Departament Física, Universitat de les Illes Balears, 07122 Palma de Mallorca, Spain",
"Departament Física, Universitat de les Illes Balears, 07122 Palma de M... | [
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12472551 | 1607.06466 | The supermassive black hole and double nucleus of the core elliptical NGC 5419 | We obtained adaptive-optics assisted SINFONI observations of the central regions of the giant elliptical galaxy NGC 5419 with a spatial resolution of 0.2 arcsec (≈55 pc). NGC 5419 has a large depleted stellar core with a radius of 1.58 arcsec (430 pc). HST and SINFONI images show a point source located at the galaxy's ... | [
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"galaxies: individual: NGC 5419",
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] | 3 | [
"10.1093/mnras/stw1802",
"10.48550/arXiv.1607.06466"
] | [
"Mazzalay, Ximena",
"Thomas, Jens",
"Saglia, Roberto P.",
"Wegner, Gary A.",
"Bender, Ralf",
"Erwin, Peter",
"Fabricius, Maximilian H.",
"Rusli, Stephanie P."
] | [
"Max-Planck-Institut für extraterrestrische Physik, Postfach 1312, D-85741 Garching, Germany",
"Max-Planck-Institut für extraterrestrische Physik, Postfach 1312, D-85741 Garching, Germany; Universitätssternwarte, Scheinerstrasse 1, D-81679 München, Germany",
"Max-Planck-Institut für extraterrestrische Physik, P... | [
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12460150 | 1607.03133 | Testing the black hole ‘no-hair’ hypothesis | Black holes (BHs) in general relativity (GR) are very simple objects. This property, that goes under the name of ‘no-hair’, has been refined in the last few decades and admits several versions. The simplicity of BHs makes them ideal testbeds of fundamental physics and of GR itself. Here we discuss the no-hair property ... | [
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... | 8.885659 | 2.573003 | 2016-07-01 | 186 | 2016CQGra..33q4001C | [
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"the name",
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"General Relativity and Quantum Cosmology",
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"High Energy Physics - Theory",
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] | 27 | [
"10.1088/0264-9381/33/17/174001",
"10.48550/arXiv.1607.03133"
] | [
"Cardoso, Vitor",
"Gualtieri, Leonardo"
] | [
"CENTRA, Departamento de Física, Instituto Superior Técnico, Universidade de Lisboa, Avenida Rovisco Pais 1, 1049 Lisboa, Portugal ; Perimeter Institute for Theoretical Physics, 31 Caroline Street North Waterloo, Ontario N2L 2Y5, Canada ; Theoretical Physics Department, CERN, CH-1211 Genève 23, Switzerland ;;",
"... | [
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12408842 | 1607.00306 | Multi-wavelength Study of Transition Region Penumbral Subarcsecond Bright Dots Using IRIS and NST | Using high-resolution transition region (TR) observations taken by the Interface Region Imaging Spectrograph (IRIS) mission, Tian et al. revealed numerous short-lived subarcsecond bright dots (BDs) above sunspots (mostly located in the penumbrae), which indicate yet unexplained small-scale energy releases. Moreover, wh... | [
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"the TR penumbral BDs",
"al.",
"sunspots",
"BDs",
"small-scale impulsive magnetic reconnection",
"the Big Bear Solar Observatory",
"darker fibrils",
"coronal heigh... | [
"Sun: activity",
"Sun: chromosphere",
"Sun: magnetic fields",
"Sun: photosphere",
"Sun: transition region",
"sunspots",
"Astrophysics - Solar and Stellar Astrophysics"
] | 5 | [
"10.3847/0004-637X/829/2/103",
"10.48550/arXiv.1607.00306"
] | [
"Deng, Na",
"Yurchyshyn, Vasyl",
"Tian, Hui",
"Kleint, Lucia",
"Liu, Chang",
"Xu, Yan",
"Wang, Haimin"
] | [
"Space Weather Research Laboratory, New Jersey Institute of Technology, University Heights, Newark, NJ 07102-1982, USA ; Big Bear Solar Observatory, New Jersey Institute of Technology, 40386 North Shore Lane, Big Bear City, CA 92314-9672, USA;",
"Big Bear Solar Observatory, New Jersey Institute of Technology, 403... | [
"2016ApJ...829L..30H",
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2301789 | 1607.07710 | VLA and ALMA Imaging of Intense Galaxy-wide Star Formation in z ∼ 2 Galaxies | We present ≃0.″4 resolution extinction-independent distributions of star formation and dust in 11 star-forming galaxies (SFGs) at z = 1.3-3.0. These galaxies are selected from sensitive blank-field surveys of the 2‧ × 2‧ Hubble Ultra-Deep Field at λ = 5 cm and 1.3 mm using the Karl G. Jansky Very Large Array and Atacam... | [
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"star formation",
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"star formation rates",
"vigorous mass assembly",
"Atacama Large Millimeter",
"SFGs",
"more compact SFGs",
"Array",
"Atacama Large Millimeter/submillimeter Array",
"stellar masses",
"SUB>⊙</SUB",
"galaxy-wide star formation",
"z",
"massive... | [
"galaxies: active",
"galaxies: evolution",
"galaxies: high-redshift",
"galaxies: star formation",
"Astrophysics - Astrophysics of Galaxies",
"Astrophysics - Cosmology and Nongalactic Astrophysics"
] | 9 | [
"10.3847/0004-637X/833/1/12",
"10.48550/arXiv.1607.07710"
] | [
"Rujopakarn, W.",
"Dunlop, J. S.",
"Rieke, G. H.",
"Ivison, R. J.",
"Cibinel, A.",
"Nyland, K.",
"Jagannathan, P.",
"Silverman, J. D.",
"Alexander, D. M.",
"Biggs, A. D.",
"Bhatnagar, S.",
"Ballantyne, D. R.",
"Dickinson, M.",
"Elbaz, D.",
"Geach, J. E.",
"Hayward, C. C.",
"Kirkpatri... | [
"Kavli Institute for the Physics and Mathematics of the universe (WPI), The University of Tokyo Institutes for Advanced Study, The University of Tokyo, Kashiwa, Chiba 277-8583, Japan ; Department of Physics, Faculty of Science, Chulalongkorn University, 254 Phayathai Road, Pathumwan, Bangkok 10330, Thailand;",
"I... | [
"2016ApJ...828L..21K",
"2016ApJ...833...68A",
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"2017ApJ...849..... | [
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12464727 | 1607.05715 | On dynamical systems approaches and methods in f(R) cosmology | We discuss dynamical systems approaches and methods applied to flat Robertson-Walker models in f(R)-gravity. We argue that a complete description of the solution space of a model requires a global state space analysis that motivates globally covering state space adapted variables. This is shown explicitly by an illustr... | [
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"state space adapted variables",
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"dynamical systems formulations",
"new regular dynamical systems",
"previous dynamical systems approaches",
"Jordan",
"the Einstein frame",
"the Einstein frames",
"the Jordan frame",
"mono... | [
"General Relativity and Quantum Cosmology",
"Astrophysics - Cosmology and Nongalactic Astrophysics",
"Mathematical Physics",
"Mathematics - Dynamical Systems"
] | 9 | [
"10.1088/1475-7516/2016/08/064",
"10.48550/arXiv.1607.05715"
] | [
"Alho, Artur",
"Carloni, Sante",
"Uggla, Claes"
] | [
"Center for Mathematical Analysis, Geometry and Dynamical Systems, Instituto Superior Técnico, Universidade de Lisboa, Av. Rovisco Pais, 1049-001 Lisboa, Portugal",
"Centro Multidisciplinar de Astrofisica – CENTRA, Instituto Superior Técnico, Universidade de Lisboa, Av. Rovisco Pais, 1049-001 Lisboa, Portugal",
... | [
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1469802 | 1607.02629 | Ensemble X-ray variability of active galactic nuclei. II. Excess variance and updated structure function | Context. Most investigations of the X-ray variability of active galactic nuclei (AGN) have been concentrated on the detailed analyses of individual, nearby sources. A relatively small number of studies have treated the ensemble behaviour of the more general AGN population in wider regions of the luminosity-redshift pla... | [
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0... | 16.173054 | 7.052226 | 2016-07-01 | 52 | 2016A&A...593A..55V | [
"Ensemble X-ray variability",
"X-ray luminosities",
"different X-ray bands",
"Multi-Epoch XMM Serendipitous AGN Sample",
"variability",
"SF studies",
"SF",
"the X-ray variability",
"AGN",
"nearby sources",
"appropriate corrections",
"the X-ray luminosity",
"redshift",
"the ensemble variabi... | [
"catalogs",
"galaxies: active",
"quasars: general",
"X-rays: galaxies",
"Astrophysics - Astrophysics of Galaxies",
"Astrophysics - High Energy Astrophysical Phenomena"
] | 12 | [
"10.1051/0004-6361/201629057",
"10.48550/arXiv.1607.02629"
] | [
"Vagnetti, F.",
"Middei, R.",
"Antonucci, M.",
"Paolillo, M.",
"Serafinelli, R."
] | [
"Dipartimento di FisicaUniversità di Roma \"Tor Vergata\", via della Ricerca Scientifica 1, 00133, Roma, Italy",
"Dipartimento di FisicaUniversità di Roma \"Tor Vergata\", via della Ricerca Scientifica 1, 00133, Roma, Italy; Dipartimento di Matematica e Fisica, Università Roma Tre, via della Vasca Navale 84, 0014... | [
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1491627 | 1607.08568 | An `analytic dynamical magnetosphere' formalism for X-ray and optical emission from slowly rotating magnetic massive stars | Slowly rotating magnetic massive stars develop `dynamical magnetospheres' (DMs), characterized by trapping of stellar wind outflow in closed magnetic loops, shock heating from collision of the upflow from opposite loop footpoints, and subsequent gravitational infall of radiatively cooled material. In 2D and 3D magnetoh... | [
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... | 8.867357 | 11.75889 | 2016-07-01 | 60 | 2016MNRAS.462.3830O | [
"hot post-shock gas",
"stellar wind outflow",
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"closed magnetic loops",
"subsequent gravitational infall",
"opposite loop footpoints",
"magnetic massive stars",
"observational diagnostics",
"the hot post-shock gas",
"observational signatures",
... | [
"magnetic fields",
"MHD",
"stars: early-type",
"stars: mass loss",
"stars: winds",
"outflows",
"X-rays: stars",
"Astrophysics - Solar and Stellar Astrophysics"
] | 4 | [
"10.1093/mnras/stw1894",
"10.48550/arXiv.1607.08568"
] | [
"Owocki, Stanley P.",
"ud-Doula, Asif",
"Sundqvist, Jon O.",
"Petit, Veronique",
"Cohen, David H.",
"Townsend, Richard H. D."
] | [
"Department of Physics and Astronomy, Bartol Research Institute, University of Delaware, Newark, DE 19716, USA",
"Penn State Worthington Scranton, Dunmore, PA 18512, USA",
"Centro de Astrobiología, CSIC-INTA, Ctra. Torrejón a Ajalvir km.4, E-28850 Madrid, Spain; Instituut voor Sterrenkunde, KU Leuven, Celestijn... | [
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"2018CoSka..48..... | [
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12594336 | 1607.05186 | Dynamical formation of black hole low-mass X-ray binaries in the field: an alternative to the common envelope | Very wide binaries (>500 au) are subject to numerous encounters with fly-by stars in the Galactic field and can be perturbed into highly eccentric orbits (e ∼ 0.99). For such systems, the tidal interactions at close pericentre passages can lead to orbit circularization and, possibly, to mass transfer, consequently p... | [
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0.0... | 6.648624 | 6.220695 | 2016-07-01 | 12 | 2017MNRAS.469.3088K | [
"mass transfer",
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"X-ray binaries",
"random stellar encounters",
"dormant BH LMXBs",
"numerous encounters",
"BH",
"BHs",
"several km s",
"circularization",
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"known sources",
"∼20",
"low-mass stars",
"e",
"low-mass donors",
"close pericentre passages... | [
"celestial mechanics",
"binaries: close",
"stars: black holes",
"X-rays: binaries",
"Astrophysics - High Energy Astrophysical Phenomena",
"Astrophysics - Solar and Stellar Astrophysics"
] | 11 | [
"10.1093/mnras/stx842",
"10.48550/arXiv.1607.05186"
] | [
"Klencki, Jakub",
"Wiktorowicz, Grzegorz",
"Gładysz, Wojciech",
"Belczynski, Krzysztof"
] | [
"Astronomical Observatory, University of Warsaw, Al. Ujazdowskie 4, 00-478 Warsaw, Poland",
"Astronomical Observatory, University of Warsaw, Al. Ujazdowskie 4, 00-478 Warsaw, Poland",
"Astronomical Observatory, University of Warsaw, Al. Ujazdowskie 4, 00-478 Warsaw, Poland",
"Astronomical Observatory, Univers... | [
"2018A&A...619A..53T",
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12406321 | 1607.06841 | Time-series Doppler imaging of the red giant HD 208472. Active longitudes and differential rotation | Context. HD 208472 is among the most active RS CVn binaries with cool starspots. Decade-long photometry has shown that the spots seem to change their longitudinal appearance with a period of about six years, coherent with brightness variations. <BR /> Aims: Our aim is to spatially resolve the stellar surface of <ASTROB... | [
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] | 8 | [
"10.1051/0004-6361/201628545",
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] | [
"Özdarcan, O.",
"Carroll, T. A.",
"Künstler, A.",
"Strassmeier, K. G.",
"Evren, S.",
"Weber, M.",
"Granzer, T."
] | [
"Leibniz Institute for Astrophysics Potsdam (AIP), An der Sternwarte 16, 14482, Potsdam, Germany; Ege University, Faculty of Science, Astronomy and Space Sciences Department, 35100 Bornova, İzmir, Turkey",
"Leibniz Institute for Astrophysics Potsdam (AIP), An der Sternwarte 16, 14482, Potsdam, Germany",
"Leibni... | [
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12593805 | 1607.08895 | The power and production efficiency of blazar jets | We use published data on the power and production efficiency of jets in blazars with double radio lobes in order to compare results obtained using different methods. In order to eliminate selection effects, we use cross-matched sub-samples containing only luminous blazars. We compare the three main existing methods, na... | [
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0.01... | 16.337254 | 5.22619 | 2016-07-01 | 39 | 2017MNRAS.465.3506P | [
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] | 6 | [
"10.1093/mnras/stw2960",
"10.48550/arXiv.1607.08895"
] | [
"Pjanka, Patryk",
"Zdziarski, Andrzej A.",
"Sikora, Marek"
] | [
"Department of Astrophysical Sciences, Princeton University, 4 Ivy Lane, Princeton, NJ 08544, USA",
"Nicolaus Copernicus Astronomical Center, Polish Academy of Sciences, Bartycka 18, PL-00-716 Warsaw, Poland",
"Nicolaus Copernicus Astronomical Center, Polish Academy of Sciences, Bartycka 18, PL-00-716 Warsaw, P... | [
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12406880 | 1607.04133 | A Hypothesis for the Color Bimodality of Jupiter Trojans | One of the most enigmatic and hitherto unexplained properties of Jupiter Trojans is their bimodal color distribution. This bimodality is indicative of two sub-populations within the Trojans, which have distinct size distributions. In this paper, we present a simple, plausible hypothesis for the origin and evolution of ... | [
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... | 8.012424 | 16.31444 | 2016-07-01 | 60 | 2016AJ....152...90W | [
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] | 6 | [
"10.3847/0004-6256/152/4/90",
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] | [
"Wong, Ian",
"Brown, Michael E."
] | [
"Division of Geological and Planetary Sciences, California Institute of Technology, Pasadena, CA 91125, USA",
"Division of Geological and Planetary Sciences, California Institute of Technology, Pasadena, CA 91125, USA"
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12473104 | 1607.04305 | The complex star cluster system of NGC 1316 (Fornax A) | This paper presents Gemini-gri' high-quality photometry for cluster candidates in the field of NGC 1316 (Fornax A) as part of a study that also includes GMOS spectroscopy. A preliminary discussion of the photometric data indicates the presence of four stellar cluster populations with distinctive features in terms of ag... | [
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] | 8 | [
"10.1093/mnras/stw1627",
"10.48550/arXiv.1607.04305"
] | [
"Sesto, Leandro A.",
"Faifer, Favio R.",
"Forte, Juan C."
] | [
"Facultad de Cs. Astronómicas y Geofísicas, Univ. Nac. de La Plata, Paseo del bosque S/N, B1900FWA LA Plata, Argentina; Instituto de Astrofísica de La Plata, Paseo del bosque S/N, B1900FWA LA Plata, Argentina; Consejo Nacional de Investigaciones Científicas y Técnicas (CONICET), Rivadavia 1917, C1033AAJ Ciudad Autó... | [
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12405904 | 1607.02379 | 3D WKB solution for fast magnetoacoustic wave behaviour around an X-line | Context. We study the propagation of a fast magnetoacoustic wave in a 3D magnetic field created from two magnetic dipoles. The magnetic topology contains an X-line. <BR /> Aims: We aim to contribute to the overall understanding of MHD wave propagation within inhomogeneous media, specifically around X-lines. <BR /> Meth... | [
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... | 12.513522 | 14.55368 | 2016-07-01 | 1 | 2016A&A...591A.103M | [
"wave behaviour",
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"magnetic fields",
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] | 6 | [
"10.1051/0004-6361/201527789",
"10.48550/arXiv.1607.02379"
] | [
"McLaughlin, J. A.",
"Botha, G. J. J.",
"Régnier, S.",
"Spoors, D. L."
] | [
"Department of Mathematics and Information Sciences, Northumbria University, Newcastle upon Tyne, NE1 8ST, UK",
"Department of Mathematics and Information Sciences, Northumbria University, Newcastle upon Tyne, NE1 8ST, UK",
"Department of Mathematics and Information Sciences, Northumbria University, Newcastle u... | [
"2017ApJ...837...94T"
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12509811 | 1607.02186 | Structure of stable binary neutron star merger remnants: A case study | In this work, we study the merger of two neutron stars with a gravitational mass of 1.4 M<SUB>⊙</SUB> each, employing the Shen-Horowitz-Teige equation of state. This equation of state is a corner case, allowing the formation of a stable neutron star with the given total baryonic mass of 3.03 M<SUB>⊙</SUB>. We investiga... | [
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0.00... | 6.398161 | 2.339051 | 2016-07-01 | 84 | 2016PhRvD..94d4060K | [
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"Astrophysics - High Energy Astrophysical Phenomena",
"General Relativity and Quantum Cosmology"
] | 10 | [
"10.1103/PhysRevD.94.044060",
"10.48550/arXiv.1607.02186"
] | [
"Kastaun, W.",
"Ciolfi, R.",
"Giacomazzo, B."
] | [
"Physics Department, University of Trento, via Sommarive 14, I-38123 Trento, Italy and INFN-TIFPA, Trento Institute for Fundamental Physics and Applications, via Sommarive 14, I-38123 Trento, Italy",
"Physics Department, University of Trento, via Sommarive 14, I-38123 Trento, Italy and INFN-TIFPA, Trento Institut... | [
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12521800 | 1607.00018 | Shining Light on Quantum Gravity with Pulsar-Black hole Binaries | Pulsars are some of the most accurate clocks found in nature, while black holes offer a unique arena for the study of quantum gravity. As such, pulsar-black hole (PSR-BH) binaries provide ideal astrophysical systems for detecting the effects of quantum gravity. With the success of aLIGO and the advent of instruments li... | [
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... | [
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] | 5 | [
"10.3847/1538-4357/aa610e",
"10.48550/arXiv.1607.00018"
] | [
"Estes, John",
"Kavic, Michael",
"Lippert, Matthew",
"Simonetti, John H."
] | [
"Department of Physics, Long Island University, Brooklyn, NY 11201, USA",
"Department of Physics, Long Island University, Brooklyn, NY 11201, USA",
"Department of Physics, Long Island University, Brooklyn, NY 11201, USA",
"Department of Physics, Virginia Tech, Blacksburg, VA, USA"
] | [
"2017IJMPD..2643004E",
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12406323 | 1607.08623 | Constraining dust extinction properties via the VVV survey | Near-infrared color-excess and extinction ratios are essential for establishing the cosmic distance scale and probing the Galaxy, particularly when analyzing targets attenuated by significant dust. A robust determination of those ratios followed from leveraging new infrared observations from the VVV survey, wherein num... | [
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"dust",
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] | 2 | [
"10.1051/0004-6361/201628763",
"10.48550/arXiv.1607.08623"
] | [
"Majaess, D.",
"Turner, D.",
"Dékány, I.",
"Minniti, D.",
"Gieren, W."
] | [
"Mount Saint Vincent University, Halifax, NS B3M 2J6, Canada ; Department of Astronomy & Physics, Saint Mary's University, Halifax, NS, B3H 3C3, Canada",
"Department of Astronomy & Physics, Saint Mary's University, Halifax, NS, B3H 3C3, Canada",
"Astronomisches Rechen-Institut, Zentrum für Astronomie de... | [
"2016ApJ...830L..14M",
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12437107 | 1607.08765 | Directional detection of Dark Matter with the MIcro-tpc MAtrix of Chambers | Particles weakly interacting with ordinary matter, with an associated mass of the order of an atomic nucleus (WIMPs), are plausible candidates for Dark Matter. The direct detection of an elastic collision of a target nuclei induced by one of these WIMPs has to be discriminated from the signal produced by the neutrons, ... | [
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-0... | 7.388408 | -2.768025 | 2016-07-01 | 4 | 2016arXiv160708765C | [
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] | 5 | [
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12472939 | 1607.08848 | Effect of a magnetic field on massive-star winds - I. Mass-loss and velocity for a dipole field | We generalize the Rigid-Field Hydrodynamic equations to accommodate arbitrary magnetic field topologies, resulting in a new Arbitrary Rigid-Field Hydrodynamic (ARFHD) formalism. We undertake a critical point calculation of the steady-state ARFHD equations with a CAK-type radiative acceleration and determine the effects... | [
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"Bard, Christopher",
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12516950 | 1607.06064 | Readout of two-kilopixel transition-edge sensor arrays for Advanced ACTPol | Advanced ACTPol is an instrument upgrade for the six-meter Atacama Cosmology Telescope (ACT) designed to measure the cosmic microwave background (CMB) temperature and polarization with arcminute-scale angular resolution. To achieve its science goals, Advanced ACTPol utilizes a larger readout multiplexing factor than an... | [
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12520464 | 1607.00312 | Hamburger Sternwarte plate archives: Historic long-term variability study of active galaxies based on digitized photographic plates | At the Hamburger Sternwarte, an effort was started in 2010 with the aim of digitizing its more than 45,000 photographic plates and films stored in its plate archives. At the time of writing, more than 31,000 plates have already been made available on the Internet for researchers, historians, and the interested public. ... | [
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12436113 | 1607.04707 | Properties of strongly magnetized ultradense matter and their imprints on magnetar pulsations | We investigate the effect of strong magnetic fields on the adiabatic radial oscillations of hadronic stars. We describe magnetized hadronic matter within the framework of the relativistic nonlinear Walecka model and integrate the equations of relativistic radial oscillations to determine the fundamental pulsation mode.... | [
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12623290 | 1607.01314 | Gravitational Waves from Oscillons after Inflation | We investigate the production of gravitational waves during preheating after inflation in the common case of field potentials that are asymmetric around the minimum. In particular, we study the impact of oscillons, comparatively long lived and spatially localized regions where a scalar field (e.g., the inflaton) oscill... | [
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"10.1103/PhysRevLett.118.011303",
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"Antusch, Stefan",
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"Deparment of Physics, University of Basel, Klingelbergstr. 82, CH-4056 Basel, Switzerland; Max-Planck-Institut für Physik (Werner-Heisenberg-Institut), Föhringer Ring 6, D-80805 München, Germany",
"Deparment of Physics, University of Basel, Klingelbergstr. 82, CH-4056 Basel, Switzerland",
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1497653 | 1607.06228 | Properties of the outer regions of spiral disks: abundances, colors and ages | We summarize the results obtained from our suite of chemical evolution models for spiral disks, computed for different total masses and star formation efficiencies. Once the gas, stars and star formation radial distributions are reproduced, we analyze the Oxygen abundances radial profiles for gas and stars, in addition... | [
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"Mollá, Mercedes",
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"Departamento de Investigación Básica, CIEMAT, 28040, Madrid. Spain",
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"E.A. Milne Centre for Astrophysics, Dept. of Physics & Mathematics, University of Hull, Hull, HU6 7RX, United Kingdom",
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12594074 | 1607.03127 | The stellar mass-halo mass relation of isolated field dwarfs: a critical test of ΛCDM at the edge of galaxy formation | We fit the rotation curves of isolated dwarf galaxies to directly measure the stellar mass-halo mass relation (M<SUB>⋆</SUB>-M<SUB>200</SUB>) over the mass range 5 × 10<SUP>5</SUP> ≲ M<SUB>⋆</SUB>/M<SUB>⊙</SUB> ≲ 10<SUP>8</SUP>. By accounting for cusp-core transformations due to stellar feedback, we find a monotonic re... | [
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"Read, J. I.",
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"Department of Physics, University of Surrey, Guildford, GU2 7XH, Surrey, UK",
"Dipartimento di Fisica e Astronomia, Università di Bologna, Viale Berti Pichat 6/2, I-40127, Bologna, Italy; INAF - Osservatorio Astronomico di Bologna, via Ranzani 1, I-40127, Bologna, Italy",
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12621568 | 1607.03916 | Chiral gravitational waves from chiral fermions | We report on a new mechanism that leads to the generation of primordial chiral gravitational waves, and hence, the violation of the parity symmetry in the Universe. We show that nonperturbative production of fermions with a definite helicity is accompanied by the generation of chiral gravitational waves. This is a gene... | [
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0... | 10.341102 | -1.193801 | 2016-07-01 | 13 | 2017PhRvD..96b3501A | [
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] | 7 | [
"10.1103/PhysRevD.96.023501",
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] | [
"Anber, Mohamed M.",
"Sabancilar, Eray"
] | [
"Lewis & Clark College, Portland, Oregon 97219, USA; Institute of Physics, Ecole Polytechnique Fédérale de Lausanne CH-1015 Lausanne Switzerland",
"Institute of Physics, Ecole Polytechnique Fédérale de Lausanne CH-1015 Lausanne Switzerland; Bielefeld University, D-33615 Bielefeld, Germany"
] | [
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12473126 | 1607.04641 | A M ≳ 3 shock in `El Gordo' cluster and the origin of the radio relic | We present an X-ray and radio study of the famous `El Gordo', a massive and distant (z = 0.87) galaxy cluster. In the deep (340 ks) Chandra observation, the cluster appears with an elongated and cometary morphology, a sign of its current merging state. The GMRT radio observations at 610 MHz confirm the presence of a ra... | [
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"X-rays: galaxies: clusters",
"galaxies: clusters: individual: ACT-CL J0102-4915",
"radio continuum: general",
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"Astrophysics - Cosmology and Nongalactic Astrophysics"
] | 14 | [
"10.1093/mnras/stw2089",
"10.48550/arXiv.1607.04641"
] | [
"Botteon, A.",
"Gastaldello, F.",
"Brunetti, G.",
"Kale, R."
] | [
"Dipartimento di Fisica e Astronomia, Università di Bologna, via C. Ranzani 1, I-40127 Bologna, Italy; INAF - IRA, via P. Gobetti 101, I-40129 Bologna, Italy",
"INAF - IASF Milano, via E. Bassini 15, I-20133 Milano, Italy",
"INAF - IRA, via P. Gobetti 101, I-40129 Bologna, Italy",
"National Centre for Radio A... | [
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12473130 | 1607.01587 | Linear stability analysis of magnetized jets: the rotating case | We perform a linear stability analysis of magnetized rotating cylindrical jet flows in the approximation of zero thermal pressure. We focus our analysis on the effect of rotation on the current driven mode and on the unstable modes introduced by rotation. We find that rotation has a stabilizing effect on the current dr... | [
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... | 15.66865 | 5.128445 | 2016-07-01 | 19 | 2016MNRAS.462.3031B | [
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"a... | [
"instabilities",
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] | 6 | [
"10.1093/mnras/stw1650",
"10.48550/arXiv.1607.01587"
] | [
"Bodo, G.",
"Mamatsashvili, G.",
"Rossi, P.",
"Mignone, A."
] | [
"INAF/Osservatorio Astrofisico di Torino, Strada Osservatorio 20, I-10025 Pino Torinese, Italy",
"Helmholtz-Zentrum Dresden-Rossendorf, PO Box 510119, D-01314 Dresden, Germany; Department of Physics, Faculty of Exact and Natural Sciences, Tbilisi State University, Il. Chavchavadze ave 3, Tbilisi 0179, Georgia; Ab... | [
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12473489 | 1607.03061 | Ammonia excitation imaging of shocked gas towards the W28 gamma-ray source HESS J1801-233 | We present 12 mm Mopra observations of the dense (>10<SUP>3</SUP> cm<SUP>-3</SUP>) molecular gas towards the north-east of the W28 supernova remnant (SNR). This cloud is spatially well matched to the TeV gamma-ray source HESS J1801-233 and is known to be an SNR-molecular cloud interaction region. Shock-disruption is... | [
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"a hot, dense mole... | [
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] | 7 | [
"10.1093/mnras/stw1687",
"10.48550/arXiv.1607.03061"
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"Maxted, Nigel I.",
"de Wilt, Phoebe",
"Rowell, Gavin P.",
"Nicholas, Brent P.",
"Burton, Michael. G.",
"Walsh, Andrew",
"Fukui, Yasuo",
"Kawamura, Akiko"
] | [
"School of Physics, University of New South Wales, Sydney 2052, Australia",
"School of Physical Sciences, Adelaide University, Adelaide 5005, Australia",
"School of Physical Sciences, Adelaide University, Adelaide 5005, Australia",
"School of Physical Sciences, Adelaide University, Adelaide 5005, Australia",
... | [
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12435444 | 1607.03347 | Hidden Photon Compton and Bremsstrahlung in White Dwarf Anomalous Cooling and Luminosity Functions | We computed the contribution of the Compton and Bremsstrahlung processes with a hidden light $U(1)_D$ neutral boson $\gamma_D$ to the white dwarf G117-B15A anomalous cooling rate, as well as the white dwarf luminosity functions (WDLF). We demonstrated that for a light mass of hidden photon ($m_{\gamma_D} \ll$ a few keV... | [
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-0.... | 8.393627 | -1.162431 | 2016-07-01 | 5 | 2016arXiv160703347C | [
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"the recent Sloan Digital Sky Survey",
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"the oldest computed stars",
"an anoma... | [
"High Energy Physics - Phenomenology",
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] | 3 | [
"10.48550/arXiv.1607.03347"
] | [
"Chang, Chia-Feng"
] | [
"-"
] | [
"2017IJMPA..3250138H",
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12516896 | 1607.08749 | Simultaneous water vapor and dry air optical path length measurements and compensation with the large binocular telescope interferometer | The Large Binocular Telescope Interferometer uses a near-infrared camera to measure the optical path length variations between the two AO-corrected apertures and provide high-angular resolution observations for all its science channels (1.5-13 microns). There is however a wavelength dependent component to the atmospher... | [
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-... | 13.993945 | 10.493579 | 2016-07-01 | 6 | 2016SPIE.9907E..1GD | [
"optical path length errors",
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"the optical path length fluctuations",
"the optical path length variations",
"the path length fluctuations",
"high-precision infrared interferometric observations",
"high-angular resolution observations",
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"dry air and water... | [
"Astrophysics - Instrumentation and Methods for Astrophysics"
] | 4 | [
"10.1117/12.2233884",
"10.48550/arXiv.1607.08749"
] | [
"Defrère, D.",
"Hinz, P.",
"Downey, E.",
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"Ertel, S.",
"Hill, J. M.",
"Hoffmann, W. F.",
"Mennesson, B.",
"Millan-Gabet, R.",
"Montoya, M.",
"Pott, J. -U.",
"Skemer, A.",
"Spalding, E.",
"Stone, J.",
"Vaz, A."
] | [
"Univ. of Arizona (United States)",
"Univ. of Arizona (United States)",
"Univ. of Arizona (United States)",
"Univ. of Stuttgart (Germany)",
"NASA Goddard Space Flight Ctr. (United States)",
"Univ. of Arizona (United States)",
"Univ. of Arizona (United States)",
"Univ. of Arizona (United States)",
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] |
2074416 | 1607.04567 | Optical characterization of the BICEP3 CMB polarimeter at the South Pole | BICEP3 is a small-aperture refracting cosmic microwave background (CMB) telescope designed to make sensitive polarization maps in pursuit of a potential B-mode signal from inflationary gravitational waves. It is the latest in the Bicep/Keck Array series of CMB experiments located at the South Pole, which has provided t... | [
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... | 10.625125 | 2.722964 | 2016-07-01 | 15 | 2016SPIE.9914E..30K | [
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"CMB",
"differential pointing",
"inflation",
"polarization",
"calibra... | [
"Astrophysics - Instrumentation and Methods for Astrophysics",
"Astrophysics - Cosmology and Nongalactic Astrophysics"
] | 6 | [
"10.1117/12.2231747",
"10.48550/arXiv.1607.04567"
] | [
"Karkare, K. S.",
"Ade, P. A. R.",
"Ahmed, Z.",
"Alexander, K. D.",
"Amiri, M.",
"Barkats, D.",
"Benton, S. J.",
"Bischoff, C. A.",
"Bock, J. J.",
"Boenish, H.",
"Bowens-Rubin, R.",
"Buder, I.",
"Bullock, E.",
"Buza, V.",
"Connors, J.",
"Filippini, J. P.",
"Fliescher, S. T.",
"Gray... | [
"Harvard-Smithsonian Ctr. for Astrophysics (United States)",
"Cardiff Univ. (United Kingdom)",
"Stanford Univ. (United States)",
"Harvard-Smithsonian Ctr. for Astrophysics (United States)",
"The Univ. of British Columbia (Canada)",
"Harvard-Smithsonian Ctr. for Astrophysics (United States)",
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