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19952026
most citedPACS Evolutionary Probe (PEP) - A Herschel Key Program

503 citations · 7.8k across the 145 of their papers we have counts for

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Showing 2010Show all

20 papers · 1 filter

astro-ph.CO2010★ 1 cited

The GaLAxy Cluster Evolution Survey (GLACE): introduction and first results

M. Sánchez-Portal, J. Cepa, I. Pintos-Castro +27

Aimed at understanding the evolution of galaxies in clusters, the GLACE survey is mapping a set of optical lines ([OII]3727, [OIII]5007, Hbeta and Halpha/[NII] when possible) in se…

astro-ph.CO2010★ 19 cited

Evolution of the Fundamental Plane of 0.2<z<1.2 Early-type galaxies in the EGS

M. Fernández Lorenzo, J. Cepa, A. Bongiovanni +5

The Fundamental Plane relates the structural properties of early-type galaxies such as its surface brightness and effective radius with its dynamics. The study of its evolution has…

astro-ph.CO2010

Search for H alpha emitters in Galaxy Clusters with Tunable Filters

Ricardo Perez-Martinez, Miguel Sanchez-Portal, Jordi Cepa +2

The studies of the evolution of galaxies in Galaxy Clusters have as a traditional complication the difficulty in establishing cluster membership of those sources detected in the fi…

astro-ph.CO2010★ 166 cited

Evolution of Dust Temperature of Galaxies through Cosmic Time as seen by Herschel

H. S. Hwang, D. Elbaz, G. E. Magdis +112

We study the dust properties of galaxies in the redshift range 0.1<z<2.8 observed by the Herschel Space Observatory in the field of the Great Observatories Origins Deep Survey-Nort…

astro-ph.IM2010★ 10 cited

OTELO survey: optimal emission-line flux determination with OSIRIS/GTC

M. A. Lara-López, J. Cepa, H. Castañeda +10

Emission-line galaxies are important targets for understanding the chemical evolution of galaxies in the universe. Deep, narrow-band imaging surveys allow to detect and study the f…

astro-ph.CO2010★ 13 cited

Herschel FIR counterparts of selected Ly-alpha emitters at z~2.2. Fast evolution since z~3 or missed obscured AGNs?

A. Bongiovanni, I. Oteo, J. Cepa +58

Ly-alpha emitters (LAEs) are seen everywhere in the redshift domain from local to z~7. Far-infrared (FIR) counterparts of LAEs at different epochs could provide direct clues on dus…