Search Publications

A mass of less than 15 solar masses for the black hole in an ultraluminous X-ray source
DOI: 10.1038/nature13730 Bibcode: 2014Natur.514..198M

Motch, C.; Soria, R.; Pakull, M. W. +2 more

Most ultraluminous X-ray sources have a typical set of properties not seen in Galactic stellar-mass black holes. They have luminosities of more than 3 × 1039 ergs per second, unusually soft X-ray components (with a typical temperature of less than about 0.3 kiloelectronvolts) and a characteristic downturn in their spectra above about 5 …

2014 Nature
XMM-Newton eHST 211
SOUSA: the Swift Optical/Ultraviolet Supernova Archive
DOI: 10.1007/s10509-014-2059-8 Bibcode: 2014Ap&SS.354...89B

Kuin, Paul; Brown, Peter J.; Holland, Stephen +2 more

The Ultra-Violet Optical Telescope on the Swift spacecraft has observed hundreds of supernovae, covering all major types and most subtypes. Here we introduce the Swift Optical/Ultraviolet Supernova Archive (SOUSA), which will contain all of the supernova images and photometry. We describe the observation and reduction procedures and how they impac…

2014 Astrophysics and Space Science
eHST 211
Mass and magnification maps for the Hubble Space Telescope Frontier Fields clusters: implications for high-redshift studies
DOI: 10.1093/mnras/stu1395 Bibcode: 2014MNRAS.444..268R

Richard, Johan; Kneib, Jean-Paul; Egami, Eiichi +9 more

Extending over three Hubble Space Telescope (HST) cycles, the Hubble Frontier Fields (HFF) initiative constitutes the largest commitment ever of HST time to the exploration of the distant Universe via gravitational lensing by massive galaxy clusters. Here, we present models of the mass distribution in the six HFF cluster lenses, derived from a joi…

2014 Monthly Notices of the Royal Astronomical Society
eHST 206
Robust weak-lensing mass calibration of Planck galaxy clusters
DOI: 10.1093/mnras/stu1423 Bibcode: 2014MNRAS.443.1973V

Kelly, Patrick L.; Allen, Steven W.; Ebeling, Harald +9 more

In light of the tension in cosmological constraints reported by the Planck team between their Sunyaev-Zel'dovich-selected cluster counts and Cosmic Microwave Background (CMB) temperature anisotropies, we compare the Planck cluster mass estimates with robust, weak-lensing mass measurements from the Weighing the Giants (WtG) project. For the 22 clus…

2014 Monthly Notices of the Royal Astronomical Society
Planck 206
The Panchromatic Hubble Andromeda Treasury. X. Ultraviolet to Infrared Photometry of 117 Million Equidistant Stars
DOI: 10.1088/0067-0049/215/1/9 Bibcode: 2014ApJS..215....9W

Bell, Eric F.; Monachesi, Antonela; Dolphin, Andrew E. +16 more

We have measured stellar photometry with the Hubble Space Telescope Wide Field Camera 3 (WFC3) and Advanced Camera for Surveys in near ultraviolet (F275W, F336W), optical (F475W, F814W), and near infrared (F110W, F160W) bands for 117 million resolved stars in M31. As part of the Panchromatic Hubble Andromeda Treasury survey, we measured photometry…

2014 The Astrophysical Journal Supplement Series
eHST 206
A Census of Star-forming Galaxies in the Z ~ 9-10 Universe based on HST+Spitzer Observations over 19 Clash Clusters: Three Candidate Z ~ 9-10 Galaxies and Improved Constraints on the Star Formation Rate Density at Z ~ 9.2
DOI: 10.1088/0004-637X/795/2/126 Bibcode: 2014ApJ...795..126B

Kelson, D. D.; Infante, L.; Zheng, W. +34 more

We utilize a two-color Lyman-break selection criterion to search for z ~ 9-10 galaxies over the first 19 clusters in the CLASH program. A systematic search yields three z ~ 9-10 candidates. While we have already reported the most robust of these candidates, MACS1149-JD, two additional z ~ 9 candidates are also found and have H 160-band …

2014 The Astrophysical Journal
eHST 205
Ultraviolet emission lines in young low-mass galaxies at z ≃ 2: physical properties and implications for studies at z > 7
DOI: 10.1093/mnras/stu1618 Bibcode: 2014MNRAS.445.3200S

Charlot, Stéphane; Richard, Johan; Siana, Brian +8 more

We present deep spectroscopy of 17 very low mass (M ≃ 2.0 × 106-1.4 × 109 M) and low luminosity (MUV ≃ -13.7 to -19.9) gravitationally lensed galaxies in the redshift range z ≃ 1.5-3.0. Deep rest-frame ultraviolet spectra reveal large equivalent width emission from numerous emission lines (N…

2014 Monthly Notices of the Royal Astronomical Society
eHST 204
A 2.5 per cent measurement of the growth rate from small-scale redshift space clustering of SDSS-III CMASS galaxies
DOI: 10.1093/mnras/stu1391 Bibcode: 2014MNRAS.444..476R

Leauthaud, Alexie; Seo, Hee-Jong; Tinker, Jeremy L. +2 more

We perform the first fit to the anisotropic clustering of Sloan Digital Sky Survey III CMASS data release 10 galaxies on scales of ∼0.8-32 h-1 Mpc. A standard halo occupation distribution model evaluated near the best-fitting Planck Λ cold dark matter (ΛCDM) cosmology provides a good fit to the observed anisotropic clustering, and impli…

2014 Monthly Notices of the Royal Astronomical Society
Planck 203
The Second Fermi GBM Gamma-Ray Burst Catalog: The First Four Years
DOI: 10.1088/0067-0049/211/1/13 Bibcode: 2014ApJS..211...13V

Collazzi, Andrew C.; Goldstein, Adam; Preece, Robert D. +30 more

This is the second of a series of catalogs of gamma-ray bursts (GRBs) observed with the Fermi Gamma-ray Burst Monitor (GBM). It extends the first two-year catalog by two more years, resulting in an overall list of 953 GBM triggered GRBs. The intention of the GBM GRB catalog is to provide information to the community on the most important observabl…

2014 The Astrophysical Journal Supplement Series
INTEGRAL 202
Physical Properties of Emission-line Galaxies at z ~ 2 from Near-infrared Spectroscopy with Magellan FIRE
DOI: 10.1088/0004-637X/785/2/153 Bibcode: 2014ApJ...785..153M

Hathi, Nimish P.; Martin, Crystal L.; Bunker, Andrew J. +16 more

We present results from near-infrared spectroscopy of 26 emission-line galaxies at z ~ 2.2 and z ~ 1.5 obtained with the Folded-port InfraRed Echellette (FIRE) spectrometer on the 6.5 m Magellan Baade telescope. The sample was selected from the WFC3 Infrared Spectroscopic Parallels survey, which uses the near-infrared grism of the Hubble Space Tel…

2014 The Astrophysical Journal
eHST 198