281 citations · 1.4k across the 24 of their papers we have counts for
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Clues to the Formation of Lenticular Galaxies Using Spectroscopic Bulge-Disk Decomposition
Evelyn J. Johnston, Alfonso Aragon-Salamanca, Michael R. Merrifield +1
Lenticular galaxies have long been thought of as evolved spirals, but the processes involved to quench the star formation are still unclear. By studying the individual star formati…
Low Masses and High Redshifts: The Evolution of the Mass-Metallicity Relation
Alaina Henry, Claudia Scarlata, Alberto Dominguez +15
We present the first robust measurement of the high redshift mass-metallicity (MZ) relation at 10^{8}< M/M_{\sun} < 10^{10}, obtained by stacking spectra of 83 emission-line galaxi…
HST/WFC3 Near-Infrared spectroscopy of quenched galaxies at z~1.5 from the WISP Survey: Stellar population properties
A. G. Bedregal, C. Scarlata, A. L. Henry +15
We combine Hubble Space Telescope (HST) G102 & G141 NIR grism spectroscopy with HST/WFC3-UVIS, HST/WFC3-IR and Spitzer/IRAC[3.6μm] photometry to assemble a sample of massive (log(M…
Predicting Future Space Near-IR Grism Surveys using the WFC3 Infrared Spectroscopic Parallels Survey
James W. Colbert, Harry Teplitz, Hakim Atek +13
We present near-infrared emission line counts and luminosity functions from the HST WFC3 Infrared Spectroscopic Parallels (WISP) program for 29 fields (0.037 deg^2) observed using…
SINFONI/VLT 3D spectroscopy of massive galaxies: Evidence of rotational support at z~1.4
Fernando Buitrago, Christopher J. Conselice, Benoit Epinat +3
There is cumulative evidence showing that, for the most massive galaxies, the fraction of disk-like objects compared to those with spheroidal properties increases with redshift. Ho…
VLT-SINFONI integral field spectroscopy of low-z luminous and ultraluminous infrared galaxies I. Atlas of the 2D gas structure
J. Piqueras López, L. Colina, S. Arribas +2
We present an atlas of a sample of local (U)LIRGs covering the luminosity range log(L_IR/L_sun)=11.1-12.4. The atlas is based on near-infrared H and K-band VLT-SINFONI IFS, and pre…