output
19952026
most citedAstropy: A Community Python Package for Astronomy

14.6k citations

Showing 2004Show all

126 papers · 1 filter

astro-ph2004★ 58 cited

The Orion Nebula in the mid-IR

M. Robberto, S. V. W. Beckwith, N. Panagia +6

We present two wide-field (5'x5'), diffraction limited, broad-band 10 and 20 micron images of the Orion Nebula, plus six 7-13 micron narrow-band images of BN/KL taken at the 3.8m U…

astro-ph2004★ 1 cited

Weak lensing measurements of dark matter halos of galaxies from COMBO-17

M. Kleinheinrich, P. Schneider, H. -W. Rix +8

We present a measurement of mass estimates for dark matter halos around galaxies from the COMBO-17 survey using weak gravitational lensing. COMBO-17 is particularly useful for this…

astro-ph2004★ 70 cited

Effects of dynamical evolution on the distribution of substructures

J. Penarrubia, A. J. Benson

We develop a semi-analytical model that determines the evolution of the mass, position and internal structure of dark matter substructures orbiting in dark matter haloes. We apply…

astro-ph2004★ 77 cited

Discovery of Two Gravitationally Lensed Quasars with Image Separations of 3 Arcseconds from the Sloan Digital Sky Survey

Masamune Oguri, Naohisa Inada, Joseph F. Hennawi +15

We report the discovery of two doubly-imaged quasars, SDSS J100128.61+502756.9 and SDSS J120629.65+433217.6, at redshifts of 1.838 and 1.789 and with image separations of 2.86'' an…

astro-ph2004★ 64 cited

Adaptive Optics Imaging of the AU Microscopii Circumstellar Disk: Evidence for Dynamical Evolution

Stanimir Metchev, Joshua A. Eisner, Lynne A. Hillenbrand +1

We present an H-band image of the light scattered from circumstellar dust around the nearby (10 pc) young M star AU Microscopii (AU Mic, GJ 803, HD 197481), obtained with the Keck…

astro-ph2004★ 97 cited

No cold dust within the supernova remnant Cassiopeia A

O. Krause, S. M. Birkmann, G. H. Rieke +4

A large amount (about three solar masses) of cold (18 K) dust in the prototypical type II supernova remnant Cassiopeia A was recently reported. It was concluded that dust productio…

astro-ph2004★ 20 cited

The Wide Field Imager Lyman-Alpha Search (WFILAS) for Galaxies at Redshift ~5.7: I. A Spatially Compact Lyman-alpha Emitting Galaxy at Redshift 5.721

Eduard Westra, D. Heath Jones, Chris E. Lidman +6

We report the spectroscopic confirmation of a compact \lya emitting galaxy at . A FORS2 spectrum of the source shows a strong asymmetric line with a flux of 5$\times10^{-1…

astro-ph2004★ 133 cited

The Evolution of Early-type Red Galaxies with the GEMS Survey: Luminosity-size and Stellar Mass-size Relations Since z=1

Daniel H. McIntosh, Eric F. Bell, Hans-Walter Rix +14

We combine HST/ACS imaging from the GEMS survey with redshifts and rest-frame quantities from COMBO-17 to study the evolution of morphologically early-type galaxies with red colors…

astro-ph2004

A recent rebuilding of most spirals ?

F. Hammer, H. Flores, X. Z. Zheng +1

Re-examination of the properties of distant galaxies leads to the evidence that most present-day spirals have built up half of their stellar masses during the last 8 Gyr, mostly du…

astro-ph2004★ 277 cited

Hot Jupiters and Hot Spots: The Short- and Long-term Chromospheric Activity on Stars with Giant Planets

E. Shkolnik, G. A. H. Walker, D. A. Bohlender +2

We monitored the chromospheric activity in the Ca II H & K lines of 13 solar-type stars (including the Sun); 8 of them over three years at the CFHT and 5 in a single run at the VLT…

astro-ph2004★ 76 cited

Millimeter observations and modeling of the AB Aurigae system

D. Semenov, Ya. Pavlyuchenkov, K. Schreyer +3

(Abriged) We present the results of millimeter observations and a suitable chemical and radiative transfer model of the AB Aur (HD 31293) circumstellar disk and surrounding envelop…

astro-ph2004

Evolution of the infrared luminosity density and star formation history up to z~1: preliminary results from MIPS

E. Le Floc'h, C. Papovich, H. Dole +6

Using deep observations of the Chandra Deep Field South obtained with MIPS at 24mic, we present our preliminary estimates on the evolution of the infrared (IR) luminosity density o…

astro-ph2004

Halo Mass Function: Low-mass Stars in Deep Fields

Wolfgang Brandner

Deep fields are unique probes of the Galactic halo. With a limiting magnitude of, e.g., I = 30 mag, all stars down to the hydrogen-burning limit are detected out to distances of 10…

astro-ph2004★ 246 cited

Did most present-day spirals form during the last 8 Gyrs? A formation history with violent episodes revealed by panchromatic observations

F. Hammer, H. Flores, D. Elbaz +3

(abridged) Studies of distant galaxies have shown that ellipticals and large spirals were already in place 8 Gyr ago, leading to a very modest recent star formation in intermediate…

astro-ph2004★ 14 cited

ISO observations of 3 - 200 micron emission by three dust populations in an isolated local translucent cloud

M. G. Rawlings, M. Juvela, K. Mattila +2

We present ISOPHOT spectrophotometry of three positions within the isolated high latitude cirrus cloud G 300.2 - 16.8, spanning from the near- to far-infrared. The positions exhibi…

astro-ph2004★ 17 cited

The Initial Mass Function toward the low-mass end in the Large Magellanic Cloud with HST/WFPC2 Observations

D. Gouliermis, W. Brandner, Th. Henning

We present V and I equivalent HST/WFPC2 photometry of two areas in the Large Magellanic Cloud: The southern part of the stellar association LH 52, located on the western edge of th…

astro-ph2004★ 116 cited

Cosmological weak lensing with the HST GEMS survey

Catherine Heymans, Michael L. Brown, Marco Barden +16

We present our cosmic shear analysis of GEMS, one of the largest wide-field surveys ever undertaken by the Hubble Space Telescope. Imaged with the Advanced Camera for Surveys (ACS)…

astro-ph2004★ 113 cited

Evolution of Cold Circumstellar Dust Around Solar-Type Stars

John M. Carpenter, Sebastian Wolf, Katharina Schreyer +2

We present submillimeter (CSO 350um) and millimeter (SEST 1.2 mm, OVRO 3 mm) photometry for 125 solar-type stars from the FEPS Spitzer Legacy program that have masses between ~0.5…

astro-ph2004★ 67 cited

Large scale inhomogeneity and local dynamical friction

A. Just, J. Penarrubia

We investigate the effect of a density gradient on Chandrasekhar's dynamical friction formula based on the method of 2-body encounters in the local approximation. We apply these ge…

astro-ph2004★ 44 cited

3D Continuum radiative transfer in complex dust configurations around young stellar objects and active nuclei II. 3D Structure of the dense molecular cloud core Rho Oph D

J. Steinacker, A. Bacmann, Th. Henning +2

Constraints on the density and thermal 3D structure of the dense molecular cloud core Rho Oph D are derived from a detailed 3D radiative transfer modeling. Two ISOCAM images at 7 a…

astro-ph2004★ 73 cited

The radio-ultraviolet spectral energy distribution of the jet in 3C273

S. Jester, H. -J. Roeser, K. Meisenheimer +1

We present deep VLA and HST observations of the large-scale jet in 3C 273 matched to 0.3" resolution. The observed spectra show a significant flattening in the infrared-ultraviolet…

astro-ph2004★ 191 cited

A comprehensive model for the Monoceros tidal stream

J. Penarrubia, D. Martinez-Delgado, H. W. Rix +7

We have compiled an extensive dataset on potential parts of the Monoceros tidal stream and performed an exhaustive survey of dwarf galaxy semi-analytic orbits in order to constrain…

astro-ph2004★ 3 cited

Microarcsecond astrometry with Gaia: the solar system, the Galaxy and beyond

C. A. L. Bailer-Jones

Gaia is an all sky, high precision astrometric and photometric satellite of the European Space Agency (ESA) due for launch in 2010-2011. Its primary mission is to study the composi…

astro-ph2004★ 38 cited

The European Large Area ISO Survey VIII: 90-micron final analysis and source counts

Ph. Heraudeau, S. Oliver, C. del Burgo +17

We present a re--analysis of the European Large Area ISO Survey (ELAIS) 90mum observations carried out with ISOPHOT, an instrument on board the ESA's Infrared Space Observatory (IS…