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A Population of Massive, Luminous Galaxies Hosting Heavily Dust-obscured Gamma-Ray Bursts: Implications for the Use of GRBs as Tracers of Cosmic Star Formation
DOI: 10.1088/0004-637X/778/2/128 Bibcode: 2013ApJ...778..128P

Cenko, S. B.; Bloom, J. S.; Filippenko, A. V. +13 more

We present observations and analysis of the host galaxies of 23 heavily dust-obscured gamma-ray bursts (GRBs) observed by the Swift satellite during the years 2005-2009, representing all GRBs with an unambiguous host-frame extinction of AV > 1 mag from this period. Deep observations with Keck, Gemini, Very Large Telescope, Hubble Spa…

2013 The Astrophysical Journal
eHST 192
Stellar Velocity Dispersion Measurements in High-luminosity Quasar Hosts and Implications for the AGN Black Hole Mass Scale
DOI: 10.1088/0004-637X/773/2/90 Bibcode: 2013ApJ...773...90G

Ferrarese, L.; Martini, P.; Peterson, B. M. +7 more

We present new stellar velocity dispersion measurements for four luminous quasars with the Near-Infrared Integral Field Spectrometer instrument and the ALTAIR laser guide star adaptive optics system on the Gemini North 8 m telescope. Stellar velocity dispersion measurements and measurements of the supermassive black hole (BH) masses in luminous qu…

2013 The Astrophysical Journal
eHST 191
Gravitational Lens Models Based on Submillimeter Array Imaging of Herschel-selected Strongly Lensed Sub-millimeter Galaxies at z > 1.5
DOI: 10.1088/0004-637X/779/1/25 Bibcode: 2013ApJ...779...25B

Maiolino, R.; Pérez-Fournon, I.; Ivison, R. J. +46 more

Strong gravitational lenses are now being routinely discovered in wide-field surveys at (sub-)millimeter wavelengths. We present Submillimeter Array (SMA) high-spatial resolution imaging and Gemini-South and Multiple Mirror Telescope optical spectroscopy of strong lens candidates discovered in the two widest extragalactic surveys conducted by the …

2013 The Astrophysical Journal
Herschel eHST 190
The Changing Lyα Optical Depth in the Range 6 < z < 9 from the MOSFIRE Spectroscopy of Y-dropouts
DOI: 10.1088/2041-8205/775/1/L29 Bibcode: 2013ApJ...775L..29T

Stiavelli, Massimo; Schmidt, Kasper B.; Treu, Tommaso +2 more

We present the MOSFIRE spectroscopy of 13 candidate z ~ 8 galaxies selected as Y-dropouts as part of the Brightest of Reionization Galaxies pure parallel survey. We detect no significant Lyα emission (our median 1σ rest-frame equivalent width sensitivity is in the range 2-16 Å). Using the Bayesian framework derived in a previous paper, we perform …

2013 The Astrophysical Journal
eHST 188
The sizes, masses and specific star formation rates of massive galaxies at 1.3 < z < 1.5: strong evidence in favour of evolution via minor mergers
DOI: 10.1093/mnras/sts092 Bibcode: 2013MNRAS.428.1088M

McLure, R. J.; Dunlop, J. S.; Jarvis, M. J. +12 more

We report the results of a comprehensive study of the relationship between galaxy size, stellar mass and specific star formation rate (sSFR) at redshifts 1.3 < z < 1.5. Based on a mass-complete (M ≥ 6 × 1010 M), spectroscopic sample from the UK Infrared Deep Sky Survey (UKIDSS) Ultradeep Survey, with accura…

2013 Monthly Notices of the Royal Astronomical Society
eHST 185
An Intensely Star-forming Galaxy at z ~ 7 with Low Dust and Metal Content Revealed by Deep ALMA and HST Observations
DOI: 10.1088/0004-637X/778/2/102 Bibcode: 2013ApJ...778..102O

Ono, Yoshiaki; Ouchi, Masami; Kurono, Yasutaka +10 more

We report deep ALMA observations complemented by associated Hubble Space Telescope (HST) imaging for a luminous (m UV = 25) galaxy, "Himiko," at a redshift of z = 6.595. The galaxy is remarkable for its high star formation rate, 100 M yr-1, which has been securely estimated from our deep HST and Spitzer photometr…

2013 The Astrophysical Journal
eHST 185
A Young Protoplanet Candidate Embedded in the Circumstellar Disk of HD 100546
DOI: 10.1088/2041-8205/766/1/L1 Bibcode: 2013ApJ...766L...1Q

Amara, Adam; Meyer, Michael R.; Girard, Julien H. +3 more

We present high-contrast observations of the circumstellar environment of the Herbig Ae/Be star HD 100546. The final 3.8 µm image reveals an emission source at a projected separation of 0.''48 ± 0.''04 (corresponding to ~47 ± 4 AU) at a position angle of 8.°9 ± 0.°9. The emission appears slightly extended with a point source component with a…

2013 The Astrophysical Journal
ISO eHST 183
The UV continua and inferred stellar populations of galaxies at z ≃ 7-9 revealed by the Hubble Ultra-Deep Field 2012 campaign
DOI: 10.1093/mnras/stt702 Bibcode: 2013MNRAS.432.3520D

Bowler, R. A. A.; McLure, R. J.; Dunlop, J. S. +16 more

We use the new ultra-deep, near-infrared imaging of the Hubble Ultra-Deep Field (HUDF) provided by our UDF12 Hubble Space Telescope (HST) Wide Field Camera 3/IR campaign to explore the rest-frame ultraviolet (UV) properties of galaxies at redshifts z > 6.5. We present the first unbiased measurement of the average UV power-law index, <β>, …

2013 Monthly Notices of the Royal Astronomical Society
eHST 182
Direct Evidence for a Fast Coronal Mass Ejection Driven by the Prior Formation and Subsequent Destabilization of a Magnetic Flux Rope
DOI: 10.1088/0004-637X/764/2/125 Bibcode: 2013ApJ...764..125P

Patsourakos, S.; Stenborg, G.; Vourlidas, A.

Magnetic flux ropes play a central role in the physics of coronal mass ejections (CMEs). Although a flux-rope topology is inferred for the majority of coronagraphic observations of CMEs, a heated debate rages on whether the flux ropes pre-exist or whether they are formed on-the-fly during the eruption. Here, we present a detailed analysis of extre…

2013 The Astrophysical Journal
SOHO 182
The Stellar Initial Mass Function of Ultra-faint Dwarf Galaxies: Evidence for IMF Variations with Galactic Environment
DOI: 10.1088/0004-637X/771/1/29 Bibcode: 2013ApJ...771...29G

Ferguson, Henry C.; Brown, Thomas M.; Geha, Marla +8 more

We present constraints on the stellar initial mass function (IMF) in two ultra-faint dwarf (UFD) galaxies, Hercules and Leo IV, based on deep Hubble Space Telescope Advanced Camera for Surveys imaging. The Hercules and Leo IV galaxies are extremely low luminosity (MV = -6.2, -5.5), metal-poor (lang[Fe/H]rang = -2.4, -2.5) systems that h…

2013 The Astrophysical Journal
eHST 181