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2011 Guillermo Barro, P. G. Pérez-González, J. Gallego

ORCID

, M. L. N. Ashby, M. Kajisawa

ORCID

, S. Miyazaki, V. Villar, T. Yamada, J. Zamorano

Uv-To-Fir Analysis of Spitzer /Irac Sources in the Extended Groth Strip. I. Multi-Wavelength Photometry and Spectral Energy Distributions

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2010 Carlos López-Sanjuan, Marc Balcells, Pablo G. Pérez-González, Guillermo Barro, César Enrique García-Dabó, Jesús Gallego

ORCID

, Jaime Zamorano

The MINOR ROLE OF GAS-RICH MAJOR MERGERS IN THE RISE OF INTERMEDIATE-MASS EARLY TYPES ATz⩽ 1

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2009 Carlos López-Sanjuan, Marc Balcells, Pablo G. Pérez-González, Guillermo Barro, César Enrique García-Dabó, Jesús Gallego

ORCID

, Jaime Zamorano

The Evolution of Passive Galaxies since z=1: Major Mergers vs Secular Processes

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2008 Pablo G. Pérez‐González, Ignacio Trujillo

ORCID

, Guillermo Barro, Jesús Gallego

ORCID

, Jaime Zamorano, Christopher J. Conselice

Exploring the Evolutionary Paths of the Most Massive Galaxies sincez∼ 2

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Víctor Villar, Jesús Gallego

ORCID

, Pablo G. Pérez‐González, Sergio Pascual

ORCID

, Kai Noeske, David C. Koo, Guillermo Barro, Jaime Zamorano

The Hα‐based Star Formation Rate Density of the Universe atz= 0.84

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Pablo G. Pérez‐González, George H. Rieke, Victor Villar, Guillermo Barro, Myra Blaylock, Eiichi Egami, Jesús Gallego

ORCID

, Armando Gil de Paz

ORCID

, Sergio Pascual

ORCID

, Jaime Zamorano, Jennifer L. Donley

ORCID

The Stellar Mass Assembly of Galaxies fromz= 0 toz= 4: Analysis of a Sample Selected in the Rest‐Frame Near‐Infrared withSpitzer

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This paper was not found in any repository; the policy of its publisher is unknown or unclear.

1970 Raymond C. Simons

ORCID

, Susan Kassin, Jonathan Trump, Benjamin Weiner, Guillermo Barro, David C. Koo, Sandra Faber, Yicheng Guo

When are Galaxy Disks Formed? Multi-PA Galaxy Kinematics at z~2 with Keck/MOSFIRE

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