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19952026
most citedAstropy: A Community Python Package for Astronomy

14.6k citations

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417 papers · 1 filter

astro-ph.CO2013★ 102 cited

A Molecular Line Scan in the Hubble Deep Field North: Constraints on the CO Luminosity Function and the Cosmic H2 Density

F. Walter, R. Decarli, M. Sargent +19

We present direct constraints on the CO luminosity function at high redshift and the resulting cosmic evolution of the molecular gas density, (z), based on a blind mole…

astro-ph.GA2013★ 67 cited

A molecular line scan in the Hubble Deep Field North

R. Decarli, F. Walter, C. Carilli +20

We present a molecular line scan in the Hubble Deep Field North (HDF-N) that covers the entire 3mm window (79-115 GHz) using the IRAM Plateau de Bure Interferometer. Our CO redshif…

astro-ph.SR2013★ 12 cited

HOPS 136: An Edge-On Orion Protostar Near the End of Envelope Infall

William J. Fischer, S. Thomas Megeath, John J. Tobin +10

Edge-on protostars are valuable for understanding the disk and envelope properties of embedded young stellar objects, since the disk, envelope, and envelope cavities are all distin…

astro-ph.HE2013★ 3 cited

Formation and collimation of relativistic MHD jets - simulations and radio maps

Christian Fendt, Oliver Porth, Somayeh Sheikhnezami

We present results of magnetohydrodynamic (MHD) simulations of jet formation and propagation, discussing a variety of astrophysical setups. In the first approach we consider simula…

astro-ph.GA2013★ 61 cited

Formation of silicon oxide grains at low temperature

S. A. Krasnokutski, G. Rouille, C. Jager +3

The formation of grains in the interstellar medium, i.e., at low temperature, has been proposed as a possibility to solve the lifetime problem of cosmic dust. This process lacks a…

astro-ph.SR2013★ 139 cited

Brown Dwarf Photospheres are Patchy: A Hubble Space Telescope Near-infrared Spectroscopic Survey Finds Frequent Low-level Variability

Esther Buenzli, Daniel Apai, Jacqueline Radigan +2

Condensate clouds strongly impact the spectra of brown dwarfs and exoplanets. Recent discoveries of variable L/T transition dwarfs argued for patchy clouds in at least some ultraco…

astro-ph.CO2013★ 296 cited

Discovery of three z>6.5 quasars in the VISTA Kilo-degree Infrared Galaxy (VIKING) survey

B. P. Venemans, J. R. Findlay, W. J. Sutherland +6

Studying quasars at the highest redshifts can constrain models of galaxy and black hole formation, and it also probes the intergalactic medium in the early universe. Optical survey…

astro-ph.GA2013★ 198 cited

Detection of a Noble Gas Molecular Ion, {36}ArH^+, in the Crab Nebula

M. J. Barlow, B. M. Swinyard, P. J. Owen +9

Noble gas molecules have not hitherto been detected in space. From spectra obtained with the Herschel Space Observatory, we report the detection of emission in the 617.5 GHz and 12…

astro-ph.GA2013★ 53 cited

Virgo Cluster and field dwarf ellipticals in 3D - II. Internal dynamics points to tidal harassment?

Agnieszka Ryś, Glenn van de Ven, Jesús Falcón-Barroso

We present the dynamical analysis of a sample of 12 dwarf elliptical (dE) galaxies for which we have obtained SAURON large-scale two-dimensional spectroscopic data. We construct Je…

astro-ph.GA2013★ 216 cited

The dusty torus in the Circinus galaxy: a dense disk and the torus funnel

K. R. W. Tristram, L. Burtscher, W. Jaffe +5

(Abridged) With infrared interferometry it is possible to resolve the nuclear dust distributions that are commonly associated with the dusty torus in active galactic nuclei (AGN).…

astro-ph.EP2013★ 128 cited

Kepler-91b: a planet at the end of its life. Planet and giant host star properties via light-curve variations

J. Lillo-Box, D. Barrado, A. Moya +8

The evolution of planetary systems is intimately linked to the evolution of their host star. Our understanding of the whole planetary evolution process is based on the large planet…

astro-ph.SR2013★ 21 cited

A Herschel view of IC 1396 A: Unveiling the different sequences of star formation

Aurora Sicilia-Aguilar, Veronica Roccatagliata, Konstantin Getman +5

The IC1396A globule in the young cluster Tr37, hosting many young stars and protostars, is assumed to be a site of triggered star formation. We mapped IC1396A with Herschel/PACS at…

astro-ph.GA2013★ 661 cited

Gas-to-Dust mass ratios in local galaxies over a 2 dex metallicity range

A. Rémy-Ruyer, S. C. Madden, F. Galliano +17

This paper analyses the behaviour of the gas-to-dust mass ratio (G/D) of local Universe galaxies over a large metallicity range. We combine three samples: the Dwarf Galaxy Survey,…

astro-ph.GA2013★ 23 cited

3D Galactic dust extinction mapping with multi-band photometry

R. J. Hanson, C. A. L. Bailer-Jones

We present a method to simultaneously infer the interstellar extinction parameters and , stellar effective temperature , and distance modulus in a Bayes…

astro-ph.CO2013★ 246 cited

An Atlas of Galaxy Spectral Energy Distributions from the Ultraviolet to the Mid-Infrared

Michael J. I. Brown, John Moustakas, J. -D. T. Smith +6

We present an atlas of 129 spectral energy distributions for nearby galaxies, with wavelength coverage spanning from the UV to the mid-infrared. Our atlas spans a broad range of ga…

astro-ph.CO2013★ 69 cited

AGN X-ray variability in the XMM-COSMOS survey

G. Lanzuisi, G. Ponti, M. Salvato +18

We took advantage of the observations carried out by XMM in the COSMOS field during 3.5 years, to study the long term variability of a large sample of AGN (638 sources), in a wide…

astro-ph.EP2013★ 140 cited

Stellar Diameters and Temperatures V. Eleven Newly Characterized Exoplanet Host Stars

Kaspar von Braun, Tabetha S. Boyajian, Gerard T. van Belle +17

We use near-infrared interferometric data coupled with trigonometric parallax values and spectral energy distribution fitting to directly determine stellar radii, effective tempera…

astro-ph.IM2013

Up to 700k GPU cores, Kepler, and the Exascale future for simulations of star clusters around black holes

P. Berczik, R. Spurzem, L. Wang +9

We present direct astrophysical N-body simulations with up to a few million bodies using our parallel MPI/CUDA code on large GPU clusters in China, Ukraine and Germany, with differ…

astro-ph.GA2013★ 35 cited

The Green Bank Telescope Maps the Dense, Star-Forming Gas in the Nearby Starburst Galaxy M82

Amanda A. Kepley, Adam K. Leroy, David Frayer +3

Observations of the Milky Way and nearby galaxies show that dense molecular gas correlates with recent star formation, suggesting that the formation of this gas phase may help regu…

astro-ph.GA2013★ 10 cited

Characterizing Quasars in the Mid-infrared: High Signal-to-Noise Spectral Templates

Allison R. Hill, S. C. Gallagher, R. P. Deo +2

Mid-infrared (MIR) quasar spectra exhibit a suite of emission features including high ionization coronal lines from the narrow line region illuminated by the ionizing continuum, br…

astro-ph.GA2013★ 13 cited

Cannibalization and Rebirth in the NGC5387 System. I. The Stellar Stream & Star Forming Region

Rachael L. Beaton, David Martinez-Delgado, Elena D'Onghia +6

We have identified a low surface brightness stellar stream from visual inspection of SDSS imaging for the edge-on, spiral galaxy NGC5387. A blue overdensity was also identified in…

astro-ph.EP2013★ 117 cited

Impact of atmospheric refraction: How deeply can we probe exo-Earth's atmospheres during primary eclipse observations?

Y. Betremieux, L. Kaltenegger

Most models used to predict or fit exoplanet transmission spectra do not include all the effects of atmospheric refraction. Namely, the angular size of the star with respect to the…

astro-ph.EP2013★ 55 cited

Physical properties and transmission spectrum of the WASP-80 planetary system from multi-colour photometry

L. Mancini, J. Southworth, S. Ciceri +29

WASP-80 is one of only two systems known to contain a hot Jupiter which transits its M-dwarf host star. We present eight light curves of one transit event, obtained simultaneously…

astro-ph.GA2013★ 230 cited

The ATLASGAL survey: a catalog of dust condensations in the Galactic plane

T. Csengeri, J. S. Urquhart, F. Schuller +10

The formation processes and the evolutionary stages of high-mass stars are poorly understood compared to low-mass stars. Large-scale surveys are needed to provide an unbiased censu…