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20052026
most cited3D-HST+CANDELS: The Evolution of the Galaxy Size-Mass Distribution since

1.4k citations · 15.9k across the 120 of their papers we have counts for

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Showing 2012Show all

6 papers · 1 filter

astro-ph.CO2012★ 30 cited

Large-Scale Star Formation-Driven Outflows at 1<z<2 in the 3D-HST Survey

Britt F. Lundgren, Gabriel Brammer, Pieter van Dokkum +18

We present evidence of large-scale outflows from three low-mass (log(M/M_sun)~9.75) star-forming (SFR >4 M_sun/yr) galaxies observed at z=1.24, z=1.35 and z=1.75 in the 3D-HST Surv…

astro-ph.CO2012★ 75 cited

Nebular Attenuation in Hα-selected Star-forming Galaxies at z=0.8 from the NewHα Survey

Ivelina Momcheva, Janice C. Lee, Chun Ly +5

We present measurements of the dust attenuation of Hα-selected emission-line galaxies at z=0.8 from the NewHα narrowband survey. The analysis is based on deep follow-up spectroscop…

astro-ph.CO2012★ 80 cited

3D-HST Grism Spectroscopy of a Gravitationally Lensed, Low-metallicity Starburst Galaxy at z=1.847

Gabriel B. Brammer, Ruben Sanchez-Janssen, Ivo Labbe +17

We present Hubble Space Telescope (HST) imaging and spectroscopy of the gravitational lens SL2SJ02176-0513, a cusp arc at z=1.847. The UV continuum of the lensed galaxy is very blu…

astro-ph.CO2012★ 116 cited

Halpha Equivalent Widths from the 3D-HST survey: evolution with redshift and dependence on stellar mass

Mattia Fumagalli, Shannon G. Patel, Marijn Franx +12

We investigate the evolution of the Halpha equivalent width, EW(Halpha), with redshift and its dependence on stellar mass, taking advantage of the first data from the 3D-HST survey…

astro-ph.CO2012★ 699 cited

3D-HST: A wide-field grism spectroscopic survey with the Hubble Space Telescope

Gabriel Brammer, Pieter van Dokkum, Marijn Franx +27

We present 3D-HST, a near-infrared spectroscopic Treasury program with the Hubble Space Telescope for studying the processes that shape galaxies in the distant Universe. 3D-HST pro…

astro-ph.CO2012★ 59 cited

A Tale of Dwarfs and Giants: Using a z=1.62 Cluster to Understand How the Red Sequence Grew Over The Last 9.5 Billion Years

Gregory H. Rudnick, Kim-Vy Tran, Casey Papovich +2

We study the red sequence in a cluster of galaxies at z=1.62 and follow its evolution over the intervening 9.5 Gyr to the present day. Using deep YJKs imaging with the HAWK-I instr…