281 citations · 1.4k across the 24 of their papers we have counts for
23 papers
The role of quenching time in the evolution of the mass-size relation of passive galaxies from the WISP survey
A. Zanella, C. Scarlata, E. M. Corsini +13
We analyze how passive galaxies at z 1.5 populate the mass-size plane as a function of their stellar age, to understand if the observed size growth with time can be explaine…
Hubble Space Telescope Grism Spectroscopy of Extreme Starbursts Across Cosmic Time: The Role of Dwarf Galaxies in the Star Formation History of the Universe
Hakim Atek, Jean-Paul Kneib, Camilla Pacifici +15
Near infrared slitless spectroscopy with the Wide Field Camera 3, onboard the Hubble Space Telescope, offers a unique opportunity to study low-mass galaxy populations at high-redsh…
Physical Properties of Emission-Line Galaxies at z ~ 2 from Near-Infrared Spectroscopy with Magellan FIRE
Daniel Masters, Patrick McCarthy, Brian Siana +16
We present results from near-infrared spectroscopy of 26 emission-line galaxies at z ~ 2 obtained with the FIRE spectrometer on the Magellan Baade telescope. The sample was selecte…
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…