Search Publications

Galaxy Stellar Mass Functions from ZFOURGE/CANDELS: An Excess of Low-mass Galaxies since z = 2 and the Rapid Buildup of Quiescent Galaxies
DOI: 10.1088/0004-637X/783/2/85 Bibcode: 2014ApJ...783...85T

Papovich, Casey; Kelson, Daniel D.; Kacprzak, Glenn G. +16 more

Using observations from the FourStar Galaxy Evolution Survey (ZFOURGE), we obtain the deepest measurements to date of the galaxy stellar mass function (SMF) at 0.2 < z < 3. ZFOURGE provides well-constrained photometric redshifts made possible through deep medium-bandwidth imaging at 1-2 µm. We combine this with Hubble Space Telescope i…

2014 The Astrophysical Journal
eHST 410
Measuring Black Hole Spin Using X-Ray Reflection Spectroscopy
DOI: 10.1007/s11214-013-0006-6 Bibcode: 2014SSRv..183..277R

Reynolds, Christopher S.

I review the current status of X-ray reflection (a.k.a. broad iron line) based black hole spin measurements. This is a powerful technique that allows us to measure robust black hole spins across the mass range, from the stellar-mass black holes in X-ray binaries to the supermassive black holes in active galactic nuclei. After describing the basic …

2014 Space Science Reviews
Suzaku 410
The 1% Concordance Hubble Constant
DOI: 10.1088/0004-637X/794/2/135 Bibcode: 2014ApJ...794..135B

Larson, D.; Weiland, J. L.; Hinshaw, G. +1 more

The determination of the Hubble constant has been a central goal in observational astrophysics for nearly a hundred years. Extraordinary progress has occurred in recent years on two fronts: the cosmic distance ladder measurements at low redshift and cosmic microwave background (CMB) measurements at high redshift. The CMB is used to predict the cur…

2014 The Astrophysical Journal
Planck 404
Planck 2013 results. XVII. Gravitational lensing by large-scale structure
DOI: 10.1051/0004-6361/201321543 Bibcode: 2014A&A...571A..17P

Kneissl, R.; Miville-Deschênes, M. -A.; Bernard, J. -P. +238 more

On the arcminute angular scales probed by Planck, the cosmic microwave background (CMB) anisotropies are gently perturbed by gravitational lensing. Here we present a detailed study of this effect, detecting lensing independently in the 100, 143, and 217 GHz frequency bands with an overall significance of greater than 25σ. We use thetemperature-gra…

2014 Astronomy and Astrophysics
Planck 402
Molecular line emission in NGC 1068 imaged with ALMA. I. An AGN-driven outflow in the dense molecular gas
DOI: 10.1051/0004-6361/201423843 Bibcode: 2014A&A...567A.125G

Tacconi, L. J.; Hunt, L. K.; Colina, L. +23 more


Aims: We investigate the fueling and the feedback of star formation and nuclear activity in NGC 1068, a nearby (D = 14 Mpc) Seyfert 2 barred galaxy, by analyzing the distribution and kinematics of the molecular gas in the disk. We aim to understand if and how gas accretion can self-regulate.
Methods: We have used the A…

2014 Astronomy and Astrophysics
eHST 395
The frequency of planetary debris around young white dwarfs
DOI: 10.1051/0004-6361/201423691 Bibcode: 2014A&A...566A..34K

Gänsicke, B. T.; Koester, D.; Farihi, J.

Context. Heavy metals in the atmospheres of white dwarfs are thought in many cases to be accreted from a circumstellar debris disk, which was formed by the tidal disruption of a rocky planetary body within the Roche radius of the star. The abundance analysis of photospheric elements and conclusions about the chemical composition of the accreted ma…

2014 Astronomy and Astrophysics
eHST 383
Transient Water Vapor at Europa's South Pole
DOI: 10.1126/science.1247051 Bibcode: 2014Sci...343..171R

Nimmo, Francis; Saur, Joachim; Roth, Lorenz +4 more

In November and December 2012, the Hubble Space Telescope (HST) imaged Europa's ultraviolet emissions in the search for vapor plume activity. We report statistically significant coincident surpluses of hydrogen Lyman-α and oxygen OI 130.4-nanometer emissions above the southern hemisphere in December 2012. These emissions were persistently found in…

2014 Science
eHST 374
The applicability of far-infrared fine-structure lines as star formation rate tracers over wide ranges of metallicities and galaxy types
DOI: 10.1051/0004-6361/201322489 Bibcode: 2014A&A...568A..62D

Lebouteiller, Vianney; De Looze, Ilse; Baes, Maarten +19 more


Aims: We analyze the applicability of far-infrared fine-structure lines [Cii] 158 µm, [Oi] 63 µm, and [Oiii] 88 µm to reliably trace the star formation rate (SFR) in a sample of low-metallicity dwarf galaxies from the Herschel Dwarf Galaxy Survey and, furthermore, extend the analysis to a broad sample of galaxies of various …

2014 Astronomy and Astrophysics
Herschel ISO 370
Andromeda's Dust
DOI: 10.1088/0004-637X/780/2/172 Bibcode: 2014ApJ...780..172D

Schinnerer, Eva; Rix, Hans-Walter; Draine, B. T. +10 more

Spitzer Space Telescope and Herschel Space Observatory imaging of M31 is used, with a physical dust model, to construct maps of dust surface density, dust-to-gas ratio, starlight heating intensity, and polycyclic aromatic hydrocarbon (PAH) abundance, out to R ≈ 25 kpc. The global dust mass is M d = 5.4 × 107 M , t…

2014 The Astrophysical Journal
Herschel 358
Planck 2013 results. XXV. Searches for cosmic strings and other topological defects
DOI: 10.1051/0004-6361/201321621 Bibcode: 2014A&A...571A..25P

Miville-Deschênes, M. -A.; Bernard, J. -P.; Planck Collaboration +225 more

Planck data have been used to provide stringent new constraints on cosmic strings and other defects. We describe forecasts of the CMB power spectrum induced by cosmic strings, calculating these from network models and simulations using line-of-sight Boltzmann solvers. We have studied Nambu-Goto cosmic strings, as well as field theory strings for w…

2014 Astronomy and Astrophysics
Planck 352