Search Publications

Galaxy Structure and Mode of Star Formation in the SFR-Mass Plane from z ~ 2.5 to z ~ 0.1
DOI: 10.1088/0004-637X/742/2/96 Bibcode: 2011ApJ...742...96W

Barro, Guillermo; Hathi, Nimish P.; Kocevski, Dale D. +23 more

We analyze the dependence of galaxy structure (size and Sérsic index) and mode of star formation (ΣSFR and SFRIR/SFRUV) on the position of galaxies in the star formation rate (SFR) versus mass diagram. Our sample comprises roughly 640,000 galaxies at z ~ 0.1, 130,000 galaxies at z ~ 1, and 36,000 galaxies at z ~ 2.…

2011 The Astrophysical Journal
Herschel eHST 659
Coronal Mass Ejections: Models and Their Observational Basis
DOI: 10.12942/lrsp-2011-1 Bibcode: 2011LRSP....8....1C

Chen, P. F.

Coronal mass ejections (CMEs) are the largest-scale eruptive phenomenon in the solar system, expanding from active region-sized nonpotential magnetic structure to a much larger size. The bulk of plasma with a mass of ∼ 1011,1013 kg is hauled up all the way out to the interplanetary space with a typical velocity of several hun…

2011 Living Reviews in Solar Physics
SOHO 643
Characterizing interstellar filaments with Herschel in IC 5146
DOI: 10.1051/0004-6361/201116596 Bibcode: 2011A&A...529L...6A

Hill, T.; André, Ph.; Arzoumanian, D. +21 more

We provide a first look at the results of the Herschel Gould Belt survey toward the IC 5146 molecular cloud and present a preliminary analysis of the filamentary structure in this region. The column density map, derived from our 70-500 µm Herschel data, reveals a complex network of filaments and confirms that these filaments are the main bir…

2011 Astronomy and Astrophysics
Herschel 635
The Second Catalog of Active Galactic Nuclei Detected by the Fermi Large Area Telescope
DOI: 10.1088/0004-637X/743/2/171 Bibcode: 2011ApJ...743..171A

Ozaki, M.; Troja, E.; Caraveo, P. A. +174 more

The second catalog of active galactic nuclei (AGNs) detected by the Fermi Large Area Telescope (LAT) in two years of scientific operation is presented. The second LAT AGN catalog (2LAC) includes 1017 γ-ray sources located at high Galactic latitudes (|b| > 10°) that are detected with a test statistic (TS) greater than 25 and associated statistic…

2011 The Astrophysical Journal
Planck 623
Subsurface water and clay mineral formation during the early history of Mars
DOI: 10.1038/nature10582 Bibcode: 2011Natur.479...53E

Murchie, Scott L.; Ehlmann, Bethany L.; Mustard, John F. +4 more

Clay minerals, recently discovered to be widespread in Mars's Noachian terrains, indicate long-duration interaction between water and rock over 3.7 billion years ago. Analysis of how they formed should indicate what environmental conditions prevailed on early Mars. If clays formed near the surface by weathering, as is common on Earth, their presen…

2011 Nature
MEx 610
The Sins Survey of z ~ 2 Galaxy Kinematics: Properties of the Giant Star-forming Clumps
DOI: 10.1088/0004-637X/733/2/101 Bibcode: 2011ApJ...733..101G

Lutz, D.; Förster Schreiber, N. M.; Genzel, R. +24 more

We have studied the properties of giant star-forming clumps in five z ~ 2 star-forming disks with deep SINFONI AO spectroscopy at the ESO VLT. The clumps reside in disk regions where the Toomre Q-parameter is below unity, consistent with their being bound and having formed from gravitational instability. Broad Hα/[N II] line wings demonstrate that…

2011 The Astrophysical Journal
eHST 602
Ultraviolet Luminosity Functions from 132 z ~ 7 and z ~ 8 Lyman-break Galaxies in the Ultra-deep HUDF09 and Wide-area Early Release Science WFC3/IR Observations
DOI: 10.1088/0004-637X/737/2/90 Bibcode: 2011ApJ...737...90B

Trenti, M.; Oesch, P. A.; Carollo, C. M. +8 more

We identify 73 z ~ 7 and 59 z ~ 8 candidate galaxies in the reionization epoch, and use this large 26-29.4 AB mag sample of galaxies to derive very deep luminosity functions to < - 18 AB mag and the star formation rate (SFR) density at z ~ 7 and z ~ 8 (just 800 Myr and 650 Myr after recombination, respectively). The galaxy sample is derived usi…

2011 The Astrophysical Journal
eHST 580
The Chandra Deep Field-South Survey: 4 Ms Source Catalogs
DOI: 10.1088/0067-0049/195/1/10 Bibcode: 2011ApJS..195...10X

Smail, I.; Lehmer, B. D.; Hornschemeier, A. E. +22 more

We present source catalogs for the 4 Ms Chandra Deep Field-South (CDF-S), which is the deepest Chandra survey to date and covers an area of 464.5 arcmin2. We provide a main Chandra source catalog, which contains 740 X-ray sources that are detected with WAVDETECT at a false-positive probability threshold of 10-5 in at least on…

2011 The Astrophysical Journal Supplement Series
eHST 530
A new, lower value of total solar irradiance: Evidence and climate significance
DOI: 10.1029/2010GL045777 Bibcode: 2011GeoRL..38.1706K

Lean, Judith L.; Kopp, Greg

The most accurate value of total solar irradiance during the 2008 solar minimum period is 1360.8 ± 0.5 W m-2 according to measurements from the Total Irradiance Monitor (TIM) on NASA's Solar Radiation and Climate Experiment (SORCE) and a series of new radiometric laboratory tests. This value is significantly lower than the canonical val…

2011 Geophysical Research Letters
SOHO 529
Relativistic jet activity from the tidal disruption of a star by a massive black hole
DOI: 10.1038/nature10374 Bibcode: 2011Natur.476..421B

Troja, E.; Im, M.; Sakamoto, T. +55 more

Supermassive black holes have powerful gravitational fields with strong gradients that can destroy stars that get too close, producing a bright flare in ultraviolet and X-ray spectral regions from stellar debris that forms an accretion disk around the black hole. The aftermath of this process may have been seen several times over the past two deca…

2011 Nature
XMM-Newton 510