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Re-evaluating WASP-12b: Strong Emission at 2.315 µm, Deeper Occultations, and an Isothermal Atmosphere
DOI: 10.1088/0004-637X/760/2/140 Bibcode: 2012ApJ...760..140C

Barman, Travis; Crossfield, Ian J. M.; Kodama, Tadayuki +2 more

We revisit the atmospheric properties of the extremely hot Jupiter WASP-12b in light of several new developments. First, we present new narrowband (2.315 µm) secondary eclipse photometry, which exhibits a planet/star flux ratio of 0.45% ± 0.06%, corresponding to a brightness temperature of 3640 ± 230 K; second, recent Spitzer/Infrared Array …

2012 The Astrophysical Journal
eHST 98
Understanding SDO/AIA Observations of the 2010 June 13 EUV Wave Event: Direct Insight from a Global Thermodynamic MHD Simulation
DOI: 10.1088/0004-637X/750/2/134 Bibcode: 2012ApJ...750..134D

Lugaz, Noé; Downs, Cooper; Roussev, Ilia I. +2 more

In this work, we present a comprehensive observation and modeling analysis of the 2010 June 13 extreme-ultraviolet (EUV) wave observed by the Atmospheric Imaging Assembly (AIA) aboard the Solar Dynamics Observatory (SDO). Due to extreme advances in cadence, resolution, and bandpass coverage in the EUV regime, the AIA instrument offers an unprecede…

2012 The Astrophysical Journal
SOHO 97
Inferences on the Distribution of Lyα Emission of z ~ 7 and z ~ 8 Galaxies
DOI: 10.1088/0004-637X/747/1/27 Bibcode: 2012ApJ...747...27T

Stiavelli, Massimo; Treu, Tommaso; Trenti, Michele +2 more

Spectroscopic confirmation of galaxies at z ~ 7 and above has been extremely difficult, owing to a drop in intensity of Lyα emission in comparison with samples at z ~ 6. This crucial finding could potentially signal the ending of cosmic reionization. However, it is based on small data sets, often incomplete and heterogeneous in nature. We introduc…

2012 The Astrophysical Journal
eHST 96
The Impact of Evolving Infrared Spectral Energy Distributions of Galaxies on Star Formation Rate Estimates
DOI: 10.1088/0004-637X/745/2/182 Bibcode: 2012ApJ...745..182N

Berta, S.; Magnelli, B.; Nordon, R. +27 more

We combine Herschel-Photodetector Array Camera and Spectrometer (PACS) data from the PACS Evolutionary Probe (PEP) program with Spitzer 24 µm and 16 µm photometry and ultra deep Infrared Spectrograph (IRS) mid-infrared spectra to measure the mid- to far-infrared spectral energy distribution (SED) of 0.7 < z < 2.5 normal star-form…

2012 The Astrophysical Journal
Herschel 95
The Molecular Gas Content of z = 3 Lyman Break Galaxies: Evidence of a Non-evolving Gas Fraction in Main-sequence Galaxies at z > 2
DOI: 10.1088/2041-8205/758/1/L9 Bibcode: 2012ApJ...758L...9M

Aussel, H.; Daddi, E.; Elbaz, D. +10 more

We present observations of the CO[J = 3 → 2] emission toward two massive and infrared luminous Lyman break galaxies (LBGs) at z = 3.21 and z = 2.92, using the IRAM Plateau de Bure Interferometer, placing first constraints on the molecular gas masses (M gas) of non-lensed LBGs. Their overall properties are consistent with those of typica…

2012 The Astrophysical Journal
Herschel eHST 94
The 60 Month All-sky Burst Alert Telescope Survey of Active Galactic Nucleus and the Anisotropy of nearby AGNs
DOI: 10.1088/0004-637X/749/1/21 Bibcode: 2012ApJ...749...21A

Greiner, J.; Alexander, D. M.; Ajello, M. +3 more

Surveys above 10 keV represent one of the best resources to provide an unbiased census of the population of active galactic nuclei (AGNs). We present the results of 60 months of observation of the hard X-ray sky with Swift/Burst Alert Telescope (BAT). In this time frame, BAT-detected (in the 15-55 keV band) 720 sources in an all-sky survey of whic…

2012 The Astrophysical Journal
INTEGRAL 93
LoCuSS: The Sunyaev-Zel'dovich Effect and Weak-lensing Mass Scaling Relation
DOI: 10.1088/0004-637X/754/2/119 Bibcode: 2012ApJ...754..119M

Smith, Graham P.; Gralla, Megan; Mroczkowski, Tony +22 more

We present the first weak-lensing-based scaling relation between galaxy cluster mass, M WL, and integrated Compton parameter Y sph. Observations of 18 galaxy clusters at z ~= 0.2 were obtained with the Subaru 8.2 m telescope and the Sunyaev-Zel'dovich Array. The M WL-Y sph scaling relations, measured at …

2012 The Astrophysical Journal
eHST 93
A Hubble Space Telescope Survey of H2 Emission in the Circumstellar Environments of Young Stars
DOI: 10.1088/0004-637X/756/2/171 Bibcode: 2012ApJ...756..171F

Herczeg, Gregory J.; Brown, Alexander; France, Kevin +8 more

The formation timescale and final architecture of exoplanetary systems are closely related to the properties of the molecular disks from which they form. Observations of the spatial distribution and lifetime of the molecular gas at planet-forming radii (a < 10 AU) are important for understanding the formation and evolution of exoplanetary syste…

2012 The Astrophysical Journal
eHST 93
The Red Supergiant Progenitor of Supernova 2012aw (PTF12bvh) in Messier 95
DOI: 10.1088/0004-637X/756/2/131 Bibcode: 2012ApJ...756..131V

Van Dyk, Schuyler D.; Filippenko, Alexei V.; Cenko, S. Bradley +9 more

We report on the direct detection and characterization of the probable red supergiant (RSG) progenitor of the intermediate-luminosity Type II-Plateau (II-P) supernova (SN) 2012aw in the nearby (10.0 Mpc) spiral galaxy Messier 95 (M95; NGC 3351). We have identified the star in both Hubble Space Telescope images of the host galaxy, obtained 17-18 yr…

2012 The Astrophysical Journal
eHST 92
A Disk-wind Model for the Near-infrared Excess Emission in Protostars
DOI: 10.1088/0004-637X/758/2/100 Bibcode: 2012ApJ...758..100B

Bans, Alissa; Königl, Arieh

Protostellar systems, ranging from low-luminosity classical T Tauri and Herbig Ae stars to high-luminosity Herbig Be stars, exhibit a near-infrared (NIR) excess in their spectra that is dominated by a bump in the monochromatic luminosity with a peak near 3 µm. The bump can be approximated by a thermal emission component of temperature ~1500 …

2012 The Astrophysical Journal
ISO 92