Search Publications

The 2014 ALMA Long Baseline Campaign: First Results from High Angular Resolution Observations toward the HL Tau Region
DOI: 10.1088/2041-8205/808/1/L3 Bibcode: 2015ApJ...808L...3A

Kneissl, R.; Andreani, P.; Hill, T. +82 more

We present Atacama Large Millimeter/submillimeter Array (ALMA) observations from the 2014 Long Baseline Campaign in dust continuum and spectral line emission from the HL Tau region. The continuum images at wavelengths of 2.9, 1.3, and 0.87 mm have unprecedented angular resolutions of 0.″ 075 (10 AU) to 0.″ 025 (3.5 AU), revealing an astonishing le…

2015 The Astrophysical Journal
eHST 1285
UV Luminosity Functions at Redshifts z ∼ 4 to z ∼ 10: 10,000 Galaxies from HST Legacy Fields
DOI: 10.1088/0004-637X/803/1/34 Bibcode: 2015ApJ...803...34B

Trenti, M.; Oesch, P. A.; Bouwens, R. J. +11 more

The remarkable Hubble Space Telescope (HST) data sets from the CANDELS, HUDF09, HUDF12, ERS, and BoRG/HIPPIES programs have allowed us to map the evolution of the rest-frame UV luminosity function (LF) from z∼ 10 to z∼ 4. We develop new color criteria that more optimally utilize the full wavelength coverage from the optical, near-IR, and mid-IR ob…

2015 The Astrophysical Journal
eHST 1197
The Evolution of the Galaxy Rest-frame Ultraviolet Luminosity Function over the First Two Billion Years
DOI: 10.1088/0004-637X/810/1/71 Bibcode: 2015ApJ...810...71F

Papovich, Casey; Finkelstein, Steven L.; Castellano, Marco +26 more

We present a robust measurement and analysis of the rest-frame ultraviolet (UV) luminosity functions at z = 4-8. We use deep Hubble Space Telescope imaging over the Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey/GOODS fields, the Hubble Ultra Deep Field, and the Hubble Frontier Field deep parallel observations near the Abell 2744 a…

2015 The Astrophysical Journal
eHST 667
How to Constrain Your M Dwarf: Measuring Effective Temperature, Bolometric Luminosity, Mass, and Radius
DOI: 10.1088/0004-637X/804/1/64 Bibcode: 2015ApJ...804...64M

Gaidos, Eric; Mann, Andrew W.; von Braun, Kaspar +2 more

Precise and accurate parameters for late-type (late K and M) dwarf stars are important for characterization of any orbiting planets, but such determinations have been hampered by these stars’ complex spectra and dissimilarity to the Sun. We exploit an empirically calibrated method to estimate spectroscopic effective temperature (Teff) a…

2015 The Astrophysical Journal
eHST 578
The KMOS3D Survey: Design, First Results, and the Evolution of Galaxy Kinematics from 0.7 <= z <= 2.7
DOI: 10.1088/0004-637X/799/2/209 Bibcode: 2015ApJ...799..209W

Wuyts, E.; Lutz, D.; Wuyts, S. +24 more

We present the KMOS3D survey, a new integral field survey of over 600 galaxies at 0.7 < z < 2.7 using KMOS at the Very Large Telescope. The KMOS3D survey utilizes synergies with multi-wavelength ground- and space-based surveys to trace the evolution of spatially resolved kinematics and star formation from a homogeneous …

2015 The Astrophysical Journal
eHST 499
Forty-seven Milky Way-sized, Extremely Diffuse Galaxies in the Coma Cluster
DOI: 10.1088/2041-8205/798/2/L45 Bibcode: 2015ApJ...798L..45V

van Dokkum, Pieter G.; Conroy, Charlie; Abraham, Roberto +3 more

We report the discovery of 47 low surface brightness objects in deep images of a 3° × 3° field centered on the Coma cluster, obtained with the Dragonfly Telephoto Array. The objects have central surface brightness µ(g, 0) ranging from 24-26 mag arcsec-2 and effective radii r eff = 3''-10'', as measured from archival Can…

2015 The Astrophysical Journal
eHST 493
The MOSDEF Survey: Measurements of Balmer Decrements and the Dust Attenuation Curve at Redshifts z ~ 1.4-2.6
DOI: 10.1088/0004-637X/806/2/259 Bibcode: 2015ApJ...806..259R

Siana, Brian; Shapley, Alice E.; Reddy, Naveen A. +7 more

We present results on the dust attenuation curve of z ∼ 2 galaxies using early observations from the MOSFIRE Deep Evolution Field survey. Our sample consists of 224 star-forming galaxies with zspec = 1.36-2.59 and high signal-to-noise ratio measurements of Hα and Hβ obtained with Keck/MOSFIRE. We construct composite spectral energy dist…

2015 The Astrophysical Journal
eHST 356
Fundamental Parameters and Spectral Energy Distributions of Young and Field Age Objects with Masses Spanning the Stellar to Planetary Regime
DOI: 10.1088/0004-637X/810/2/158 Bibcode: 2015ApJ...810..158F

Faherty, Jacqueline; Cruz, Kelle L.; Rice, Emily L. +3 more

We combine optical, near-infrared, and mid-infrared spectra and photometry to construct expanded spectral energy distributions for 145 field age (>500 Myr) and 53 young (lower age estimate <500 Myr) ultracool dwarfs (M6-T9). This range of spectral types includes very low mass stars, brown dwarfs, and planetary mass objects, providing fundame…

2015 The Astrophysical Journal
eHST 307
The Systematic Properties of the Warm Phase of Starburst-Driven Galactic Winds
DOI: 10.1088/0004-637X/809/2/147 Bibcode: 2015ApJ...809..147H

Heckman, Timothy M.; Leitherer, Claus; Borthakur, Sanchayeeta +2 more

Using ultraviolet absorption lines, we analyze the systematic properties of the warm ionized phase of starburst-driven winds in a sample of 39 low-redshift objects that spans broad ranges in starburst and galaxy properties. Total column densities for the outflows are ∼1021 cm-2. The outflow velocity (vout) correlat…

2015 The Astrophysical Journal
eHST 302
Forming Compact Massive Galaxies
DOI: 10.1088/0004-637X/813/1/23 Bibcode: 2015ApJ...813...23V

van Dokkum, Pieter G.; Franx, Marijn; Illingworth, Garth D. +13 more

In this paper we study a key phase in the formation of massive galaxies: the transition of star-forming galaxies into massive (Mstars ∼ 1011M), compact (re ∼ 1 kpc) quiescent galaxies, which takes place from z ∼ 3 to z ∼ 1.5. We use HST grism redshifts and extensive photometry in all five 3D-HST/CANDELS…

2015 The Astrophysical Journal
eHST 291