activity
20042026
most citedNear-Infrared Photometry and Spectroscopy of L and T Dwarfs: the Effects of Temperature, Clouds, and Gravity

543 citations · 8.3k across the 210 of their papers we have counts for

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Showing astro-ph.COShow all

6 papers · 1 filter

astro-ph.CO2025

The Mass-Metallicity Relation and its Observational Effects at z~3-6

Zach Lewis, Michael V. Maseda, Anna de Graaff +21

The correlation between galaxy stellar mass and gas-phase metallicity, known as the mass-metallicity relation (MZR), gives key insights into the processes that govern galaxy evolut…

astro-ph.CO2013★ 132 cited

The Progenitors of the Compact Early-Type Galaxies at High-Redshift

Christina C. Williams, Mauro Giavalisco, Paolo Cassata +19

We use GOODS and CANDELS images to identify progenitors of massive (log M > 10 Msun) compact "early-type" galaxies (ETGs) at z~1.6. Since merging and accretion increase the size of…

astro-ph.CO2012

CANDELS: The progenitors of compact quiescent galaxies at z~2

Guillermo Barro, S. M. Faber, Pablo G. Perez-Gonzalez +29

We combine high-resolution HST/WFC3 images with multi-wavelength photometry to track the evolution of structure and activity of massive (log(M*) > 10) galaxies at redshifts z = 1.4…

astro-ph.CO2011★ 48 cited

Rest-frame UV--Optically Selected Galaxies at 2.3<z<3.5: Searching for Dusty Star-forming and Passively-Evolving Galaxies

Yicheng Guo, Mauro Giavalisco, Paolo Cassata +17

A new set of color selection criteria (VJL) analogous with the BzK method is designed to select both star-forming galaxies (SFGs) and passively-evolving galaxies (PEGs) at 2.3<z<3.…

astro-ph.CO2011★ 307 cited

What turns galaxies off? The different morphologies of star-forming and quiescent galaxies since z~2 from CANDELS

Eric F. Bell, Arjen van der Wel, Casey Papovich +21

We use HST/WFC3 imaging from the CANDELS Multicycle Treasury Survey, in conjunction with the Sloan Digital Sky Survey, to explore the evolution of galactic structure for galaxies w…

astro-ph.CO2011★ 50 cited

On the Clustering of Sub-millimeter Galaxies

Christina C. Williams, Mauro Giavalisco, Cristiano Porciani +14

We measure the angular two-point correlation function of sub-millimeter galaxies (SMGs) from 1.1-millimeter imaging of the COSMOS field with the AzTEC camera and ASTE 10-meter tele…