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The Hubble Space Telescope Cluster Supernova Survey. II. The Type Ia Supernova Rate in High-redshift Galaxy Clusters
DOI: 10.1088/0004-637X/745/1/32 Bibcode: 2012ApJ...745...32B

Gladders, M. D.; Panagia, N.; Huang, X. +41 more

We report a measurement of the Type Ia supernova (SN Ia) rate in galaxy clusters at 0.9 < z < 1.46 from the Hubble Space Telescope Cluster Supernova Survey. This is the first cluster SN Ia rate measurement with detected z > 0.9 SNe. Finding 8 ± 1 cluster SNe Ia, we determine an SN Ia rate of 0.50+0.23 -0.19 (stat)

2012 The Astrophysical Journal
eHST 52
Resolving the Galaxies within a Giant Lyα Nebula: Witnessing the Formation of a Galaxy Group?
DOI: 10.1088/0004-637X/752/2/86 Bibcode: 2012ApJ...752...86P

Dey, Arjun; Jannuzi, Buell T.; Soifer, B. T. +8 more

Detailed analysis of the substructure of Lyα nebulae can put important constraints on the physical mechanisms at work and the properties of galaxies forming within them. Using high-resolution Hubble Space Telescope (HST) imaging of a Lyα nebula at z ≈ 2.656, we have taken a census of the compact galaxies in the vicinity, used optical/near-infrared…

2012 The Astrophysical Journal
eHST 52
Morphological Evolution of a Three-dimensional Coronal Mass Ejection Cloud Reconstructed from Three Viewpoints
DOI: 10.1088/0004-637X/751/1/18 Bibcode: 2012ApJ...751...18F

Feng, L.; Inhester, B.; Wei, Y. +3 more

The propagation properties of coronal mass ejections (CMEs) are crucial to predict its geomagnetic effect. A newly developed three-dimensional (3D) mask fitting reconstruction method using coronagraph images from three viewpoints has been described and applied to the CME ejected on 2010 August 7. The CME's 3D localization, real shape, and morpholo…

2012 The Astrophysical Journal
SOHO VenusExpress 52
On the Role of the Accretion Disk in Black Hole Disk-Jet Connections
DOI: 10.1088/0004-637X/757/1/11 Bibcode: 2012ApJ...757...11M

Fabian, A. C.; Miller, J. M.; Nowak, M. A. +5 more

Models of jet production in black hole systems suggest that the properties of the accretion disk—such as its mass accretion rate, inner radius, and emergent magnetic field—should drive and modulate the production of relativistic jets. Stellar-mass black holes in the "low/hard" state are an excellent laboratory in which to study disk-jet connection…

2012 The Astrophysical Journal
Suzaku 51
Early-type Galaxies at z ~ 1.3. IV. Scaling Relations in Different Environments
DOI: 10.1088/0004-637X/745/2/130 Bibcode: 2012ApJ...745..130R

Demarco, R.; Tanaka, M.; Rosati, P. +15 more

We present the Kormendy and mass-size relations (MSR) for early-type galaxies (ETGs) as a function of environment at z ~ 1.3. Our sample includes 76 visually classified ETGs with masses 1010 < M/M < 1011.5, selected in the Lynx supercluster and in the Great Observatories Origins Deep Survey/Chandra Deep Fie…

2012 The Astrophysical Journal
eHST 51
A Herschel Survey of Cold Dust in Disks around Brown Dwarfs and Low-mass Stars
DOI: 10.1088/0004-637X/755/1/67 Bibcode: 2012ApJ...755...67H

Pascucci, Ilaria; Henning, Thomas; Ménard, François +6 more

We report the complete photometric results from our Herschel study which is the first comprehensive program to search for far-infrared emission from cold dust around young brown dwarfs (BDs). We surveyed 50 fields containing 51 known or suspected BDs and very low mass stars that have evidence of circumstellar disks based on Spitzer photometry and/…

2012 The Astrophysical Journal
Herschel 51
Luminous and High Stellar Mass Candidate Galaxies at z ≈ 8 Discovered in the Cosmic Assembly Near-Infrared Deep Extragalactic Legacy Survey
DOI: 10.1088/0004-637X/761/2/177 Bibcode: 2012ApJ...761..177Y

Papovich, Casey; Finkelstein, Steven L.; Dickinson, Mark +26 more

One key goal of the Hubble Space Telescope Cosmic Assembly Near-Infrared Deep Extragalactic Legacy Survey is to track galaxy evolution back to z ≈ 8. Its two-tiered "wide and deep" strategy bridges significant gaps in existing near-infrared surveys. Here we report on z ≈ 8 galaxy candidates selected as F105W-band dropouts in one of its deep fields…

2012 The Astrophysical Journal
eHST 51
The Unusual Temporal and Spectral Evolution of SN2011ht. II. Peculiar Type IIn or Impostor?
DOI: 10.1088/0004-637X/760/1/93 Bibcode: 2012ApJ...760...93H

Humphreys, Roberta M.; Davidson, Kris; Pogge, R. W. +4 more

SN2011ht has been described both as a true supernova (SN) and as an impostor. In this paper, we conclude that it does not match some basic expectations for a core-collapse event. We discuss SN2011ht's spectral evolution from a hot dense wind to a cool dense wind, followed by the post-plateau appearance of a faster low density wind during a rapid d…

2012 The Astrophysical Journal
eHST 51
Luminous Satellites. II. Spatial Distribution, Luminosity Function, and Cosmic Evolution
DOI: 10.1088/0004-637X/752/2/99 Bibcode: 2012ApJ...752...99N

Treu, T.; Auger, M. W.; Fassnacht, C. D. +3 more

We infer the normalization and the radial and angular distributions of the number density of satellites of massive galaxies (log10[M*h/M ] > 10.5) between redshifts 0.1 and 0.8 as a function of host stellar mass, redshift, morphology, and satellite luminosity. Exploiting the depth and resolution of the COSMOS H…

2012 The Astrophysical Journal
eHST 51
The Relationship between the Sudden Change of the Lorentz Force and the Magnitude of Associated Flares
DOI: 10.1088/2041-8205/757/1/L5 Bibcode: 2012ApJ...757L...5W

Liu, Chang; Wang, Haimin; Wang, Shuo

The rapid and irreversible change of photospheric magnetic fields associated with flares has been confirmed by many recent studies. These studies showed that the photospheric magnetic fields respond to coronal field restructuring and turn to a more horizontal state near the magnetic polarity inversion line (PIL) after eruptions. Recent theoretical…

2012 The Astrophysical Journal
SOHO 51