Search Publications

GOODS-Herschel: Star Formation, Dust Attenuation, and the FIR-radio Correlation on the Main Sequence of Star-forming Galaxies up to z ≃4
DOI: 10.1088/0004-637X/807/2/141 Bibcode: 2015ApJ...807..141P

Aussel, H.; Daddi, E.; Elbaz, D. +25 more

We use deep panchromatic data sets in the GOODS-N field, from GALEX to the deepest Herschel far-infrared (FIR) and VLA radio continuum imaging, to explore the evolution of star-formation activity and dust attenuation properties of star-forming galaxies to z ≃ 4, using mass-complete samples. Our main results can be summarized as follows: (i) the sl…

2015 The Astrophysical Journal
Herschel 204
Blowin' in the Wind: Both "Negative" and "Positive" Feedback in an Obscured High-z Quasar
DOI: 10.1088/0004-637X/799/1/82 Bibcode: 2015ApJ...799...82C

Maiolino, R.; Silverman, J. D.; Merloni, A. +13 more

Quasar feedback in the form of powerful outflows is invoked as a key mechanism to quench star formation in galaxies, preventing massive galaxies to overgrow and producing the red colors of ellipticals. On the other hand, some models are also requiring "positive" active galactic nucleus feedback, inducing star formation in the host galaxy through e…

2015 The Astrophysical Journal
eHST 203
[C II] 158 µm Emission as a Star Formation Tracer
DOI: 10.1088/0004-637X/800/1/1 Bibcode: 2015ApJ...800....1H

Helou, G.; Boquien, M.; Roussel, H. +23 more

The [C II] 157.74 µm transition is the dominant coolant of the neutral interstellar gas, and has great potential as a star formation rate (SFR) tracer. Using the Herschel KINGFISH sample of 46 nearby galaxies, we investigate the relation of [C II] surface brightness and luminosity with SFR. We conclude that [C II] can be used for measurement…

2015 The Astrophysical Journal
Herschel 203
Tau-REx I: A Next Generation Retrieval Code for Exoplanetary Atmospheres
DOI: 10.1088/0004-637X/802/2/107 Bibcode: 2015ApJ...802..107W

Waldmann, I. P.; Rocchetto, M.; Tinetti, G. +3 more

Spectroscopy of exoplanetary atmospheres has become a well established method for the characterization of extrasolar planets. We here present a novel inverse retrieval code for exoplanetary atmospheres. T-REx(Tau Retrieval for Exoplanets) is a line-by-line radiative transfer fully Bayesian retrieval framework. T-REx includes the following features…

2015 The Astrophysical Journal
eHST 199
Are Ultra-faint Galaxies at z = 6-8 Responsible for Cosmic Reionization? Combined Constraints from the Hubble Frontier Fields Clusters and Parallels
DOI: 10.1088/0004-637X/814/1/69 Bibcode: 2015ApJ...814...69A

Richard, Johan; Schaerer, Daniel; Kneib, Jean-Paul +8 more

We use deep Hubble Space Telescope imaging of the Frontier Fields to accurately measure the galaxy rest-frame ultraviolet luminosity function (UV LF) in the redshift range z ∼ 6-8. We combine observations in three lensing clusters, A2744, MACS 0416, and MACS 0717, and their associated parallel fields to select high-redshift dropout candidates. We …

2015 The Astrophysical Journal
eHST 186
The Hubble Space Telescope UV Legacy Survey of Galactic Globular Clusters. III. A Quintuple Stellar Population in NGC 2808
DOI: 10.1088/0004-637X/808/1/51 Bibcode: 2015ApJ...808...51M

Anderson, J.; Milone, A. P.; Marino, A. F. +9 more

In this study we present the first results from multi-wavelength Hubble Space Telescope (HST) observations of the Galactic globular cluster (GC) NGC 2808 as an extension of the Hubble Space Telescope UV Legacy Survey of Galactic GCs (GO-13297 and previous proprietary and HST archive data). Our analysis allowed us to disclose a multiple-stellar-pop…

2015 The Astrophysical Journal
eHST 185
The Light Curve of the Macronova Associated with the Long-Short Burst GRB 060614
DOI: 10.1088/2041-8205/811/2/L22 Bibcode: 2015ApJ...811L..22J

Li, Xiang; Jin, Zhi-Ping; Covino, Stefano +3 more

The Swift-detected GRB 060614 was a unique burst that straddles an imaginary divide between long- and short-duration gamma-ray bursts (GRBs), and its physical origin has been heavily debated over the years. Recently, a distinct, very soft F814W-band excess at t∼ 13.6 days after the burst was identified in a joint-analysis of VLT and Hubble Space T…

2015 The Astrophysical Journal
eHST 185
Hubble Frontier Fields First Complete Cluster Data: Faint Galaxies at z ~ 5-10 for UV Luminosity Functions and Cosmic Reionization
DOI: 10.1088/0004-637X/799/1/12 Bibcode: 2015ApJ...799...12I

Ono, Yoshiaki; Ouchi, Masami; Shimasaku, Kazuhiro +3 more

We present comprehensive analyses of faint dropout galaxies up to z ~ 10 with the first full-depth data set of the A2744 lensing cluster and parallel fields observed by the Hubble Frontier Fields (HFF) program. We identify 54 dropouts at z ~ 5-10 in the HFF fields and enlarge the size of the z ~ 9 galaxy sample obtained to date. Although the numbe…

2015 The Astrophysical Journal
eHST 178
Major Mergers Host the Most-luminous Red Quasars at z ~ 2: A Hubble Space Telescope WFC3/IR Study
DOI: 10.1088/0004-637X/806/2/218 Bibcode: 2015ApJ...806..218G

Schawinski, Kevin; Urry, C. M.; Glikman, Eilat +3 more

We used the Hubble Space Telescope (HST) Wide Field Camera 3 (WFC3) near-infrared camera to image the host galaxies of a sample of 11 luminous, dust-reddened quasars at z∼ 2—the peak epoch of black hole growth and star formation in the universe—to test the merger-driven picture for the coevolution of galaxies and their nuclear black holes. The red…

2015 The Astrophysical Journal
eHST 170
High-precision Photometric Redshifts from Spitzer/IRAC: Extreme [3.6] - [4.5] Colors Identify Galaxies in the Redshift Range z ∼ 6.6 - 6.9
DOI: 10.1088/0004-637X/801/2/122 Bibcode: 2015ApJ...801..122S

Holwerda, Benne; Franx, Marijn; Labbé, Ivo +7 more

One of the most challenging aspects of studying galaxies in the z≳ 7 universe is the infrequent confirmation of their redshifts through spectroscopy, a phenomenon thought to occur from the increasing opacity of the intergalactic medium to Lyα photons at z\gt 6.5. The resulting redshift uncertainties inhibit the efficient search for [C ii] in z∼ 7 …

2015 The Astrophysical Journal
eHST 168