activity
20102022
most citedGaia DR2 study of Herbig Ae/Be stars

188 citations · 397 across the 13 of their papers we have counts for

collaborators
Showing astro-ph.COShow all

6 papers · 1 filter

astro-ph.CO2013★ 15 cited

Lyman break and UV-selected galaxies at z ~ 1: II. PACS-100um/160um FIR detections

I. Oteo, G. Magdis, Á. Bongiovanni +53

We report the PACS-100um/160um detections of a sample of 42 GALEX-selected and FIR-detected Lyman break galaxies (LBGs) at z ~ 1 located in the COSMOS field and analyze their ultra…

astro-ph.CO2013★ 39 cited

FIR-detected Lyman break galaxies at z ~ 3: Dust attenuation and dust correction factors at high redshift

I. Oteo, J. Cepa, Á. Bongiovanni +7

Lyman break galaxies (LBGs) represent one of the kinds of star-forming galaxies that are found in the high-redshift universe. The detection of LBGs in the FIR domain can provide ve…

astro-ph.CO2013★ 6 cited

Lyman break and UV-selected galaxies at I. Stellar populations from ALHAMBRA survey

I. Oteo, Á. Bongiovanni, J. Cepa +29

We take advantage of the exceptional photometric coverage provided by the combination of GALEX data in the UV and the ALHAMBRA survey in the optical and near-IR to analyze the phys…

astro-ph.CO2012★ 13 cited

Physical properties of Lyman-alpha emitters at from UV-to-FIR measurements

I. Oteo, A. Bongiovanni, A. M. Pérez García +25

The analysis of the physical properties of low-redshift Ly emitters (LAEs) can provide clues in the study of their high-redshift analogues. At , LAEs are bright enou…

astro-ph.CO2012★ 26 cited

PACS-Herschel FIR detections of Lyman-alpha emitters at 2.0<z<3.5

I. Oteo, A. Bongiovanni, A. M. Pérez García +23

In this work we analyze the physical properties of a sample of 56 spectroscopically selected star-forming (SF) Ly emitting galaxies at 2.0z3.5 using both a s…

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…