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most citedWhat do we learn from IRAC observations of galaxies at 2 < z < 3.5?

367 citations · 748 across the 6 of their papers we have counts for

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astro-ph2006367 cited

What do we learn from IRAC observations of galaxies at 2 < z < 3.5?

Stijn Wuyts, Ivo Labbe, Marijn Franx +9

We analyze very deep HST, VLT and Spitzer photometry of galaxies at 2<z<3.5 in the Hubble Deep Field South. The sample is selected from the deepest public K-band imaging currently…

astro-ph2006106 cited

Measuring the Average Evolution of Luminous Galaxies at z<3: The Rest-frame Optical Luminosity Density, Spectral Energy Distribution, and Stellar Mass Density

Gregory Rudnick, Ivo Labbe, Natascha M. Foerster Schreiber +11

(Abridged) We present the evolution of the volume averaged properties of the rest-frame optically luminous galaxy population to z~3, determined from four disjoint deep fields with…

astro-ph200694 cited

Incorporating the molecular gas phase in galaxy-size numerical simulations: first applications in dwarf galaxies

F. I. Pelupessy, P. P. Papadopoulos, P. P. van der Werf

We present models of the evolution of the gaseous and stellar content of galaxies incorporating the formation of H_2 out of HI gas as part of such a model. We do so by formulating…

astro-ph200685 cited

Direct Measurements of the Stellar Continua and Balmer/4000 Angstrom Breaks of Red z>2 Galaxies: Redshifts and Improved Constraints on Stellar Populations

Mariska Kriek, Pieter van Dokkum, Marijn Franx +11

We use near-infrared (NIR) spectroscopy obtained with GNIRS on Gemini, NIRSPEC on KECK, and ISAAC on the VLT to study the rest-frame optical continua of three `Distant Red Galaxies…