2.2k citations · 18k across the 279 of their papers we have counts for
9 papers · 1 filter
Very Strong Emission-Line Galaxies in the WISP Survey and Implications for High-Redshift Galaxies
H. Atek, B. Siana, C. Scarlata +13
The WFC3 Infrared Spectroscopic Parallel Survey (WISP) uses the Hubble Space Telescope (HST) infrared grism capabilities to obtain slitless spectra of thousands of galaxies over a…
Central Powering of the Largest Lyman-alpha Nebula is Revealed by Polarized Radiation
Matthew Hayes, Claudia Scarlata, Brian Siana
High-redshift Lyman-alpha blobs are extended, luminous, but rare structures that appear to be associated with the highest peaks in the matter density of the Universe. Their energy…
A CANDELS WFC3 Grism Study of Emission-Line Galaxies at z~2: A Mix of Nuclear Activity and Low-Metallicity Star Formation
Jonathan R. Trump, Benjamin J. Weiner, Claudia Scarlata +26
We present Hubble Space Telescope Wide Field Camera 3 slitless grism spectroscopy of 28 emission-line galaxies at z~2, in the GOODS-S region of the Cosmic Assembly Near-infrared De…
Extreme Emission Line Galaxies in CANDELS: Broad-Band Selected, Star-Bursting Dwarf Galaxies at z>1
A. van der Wel, A. N. Straughn, H. -W. Rix +29
We identify an abundant population of extreme emission line galaxies (EELGs) at redshift z~1.7 in the Cosmic Assembly Near-IR Deep Extragalactic Legacy Survey (CANDELS) imaging fro…
The relative abundance of compact and normal massive early-type galaxies and its evolution from redshift z~2 to the present
P. Cassata, M. Giavalisco, Yicheng Guo +11
We report on the evolution of the number density and size of early-type galaxies from z~2 to z~0. We select a sample of 563 massive (M>10^{10} Msun), passively evolving (SSFR<10^{-…
The radial and azimuthal profiles of Mg II absorption around 0.5 < z < 0.9 zCOSMOS galaxies of different colors, masses and environments
R. Bordoloi, S. J. Lilly, C. Knobel +50
We map the radial and azimuthal distribution of Mg II gas within 200 kpc (physical) of 4000 galaxies at redshifts 0.5 < z < 0.9 using co-added spectra of more than 5000 background…