Back to Search Start Over

Lyman break and ultraviolet-selected galaxies at z ∼ 1 - I. Stellar populations from the ALHAMBRA survey

Authors :
Ministerio de Economía y Competitividad (España)
Alfred P. Sloan Foundation
National Science Foundation (US)
Department of Energy (US)
National Aeronautics and Space Administration (US)
Japanese Government
Max Planck Society
Higher Education Funding Council for England
Junta de Andalucía
Oteo Gómez, Iván
Bongiovanni, Ángel
Cepa, Jordi
Pérez-García, Ana M.
Ederoclite, Alessandro
Sánchez-Portal, Miguel
Pintos-Castro, Irene
Pérez-Martínez, Ricardo
Polednikova, Jana
Aguerri, J.A.L.
Alfaro, Emilio J.
Aparicio Villegas, Teresa
Benítez, Narciso
Broadhurst, Tom
Cabrera-Caño, Jesús
Castander, Francisco J.
Cerviño, Miguel
Cristóbal-Hornillos, David
Fernández-Soto, Alberto
González Delgado, Rosa M.
Husillos, César
Infante, Leopoldo
Martínez, Vicente J.
Márquez, Isabel
Masegosa, Josefa
Matute, Israel
Moles, Mariano
Molino, Alberto
Olmo, Ascensión del
Perea, Jaime
Pović, Mirjana
Prada, Francisco
Quintana, José María
Viironen, Kerttu
Ministerio de Economía y Competitividad (España)
Alfred P. Sloan Foundation
National Science Foundation (US)
Department of Energy (US)
National Aeronautics and Space Administration (US)
Japanese Government
Max Planck Society
Higher Education Funding Council for England
Junta de Andalucía
Oteo Gómez, Iván
Bongiovanni, Ángel
Cepa, Jordi
Pérez-García, Ana M.
Ederoclite, Alessandro
Sánchez-Portal, Miguel
Pintos-Castro, Irene
Pérez-Martínez, Ricardo
Polednikova, Jana
Aguerri, J.A.L.
Alfaro, Emilio J.
Aparicio Villegas, Teresa
Benítez, Narciso
Broadhurst, Tom
Cabrera-Caño, Jesús
Castander, Francisco J.
Cerviño, Miguel
Cristóbal-Hornillos, David
Fernández-Soto, Alberto
González Delgado, Rosa M.
Husillos, César
Infante, Leopoldo
Martínez, Vicente J.
Márquez, Isabel
Masegosa, Josefa
Matute, Israel
Moles, Mariano
Molino, Alberto
Olmo, Ascensión del
Perea, Jaime
Pović, Mirjana
Prada, Francisco
Quintana, José María
Viironen, Kerttu
Publication Year :
2013

Abstract

We take advantage of the exceptional photometric coverage provided by the combination of GALEX data in the ultraviolet (UV) and the ALHAMBRA survey in the optical and near-infrared to analyse the physical properties of a sample of 1225 GALEX-selected Lyman break galaxies (LBGs) at 0.8 ≲ z ≲ 1.2 that are located in the COSMOS field. This is the largest sample of LBGs studied in this redshift range to date. According to a spectral energy distribution (SED) fitting with synthetic stellar population templates, we find that LBGs at z ̃ 1 are mostly young galaxies with a median age of 341 Myr and have intermediate dust attenuation, (Es(B - V)) ̃ 0.20. Owing to the selection criterion, LBGs at z ̃ 1 are UV-bright galaxies and have a high dust-corrected total star formation rate (SFR), with a median value of 16.9M⊙ yr-1. Their median stellar mass is log (M*/M⊙) = 9.74. We find that the dustcorrected total SFR of LBGs increases with stellar mass and that the specific SFR is lower for more massive galaxies (downsizing scenario). Only 2 per cent of the galaxies selected through the Lyman break criterion have an active galactic nucleus nature. LBGs at z ̃ 1 are located mostly over the blue cloud of the colour-magnitude diagram of galaxies at their redshift, with only the oldest and/or the dustiest deviating towards the green valley and red sequence. Morphologically, 69 per cent of LBGs are disc-like galaxies, with the fractions of interacting, compact, or irregular systems being much lower, below 12 per cent. LBGs have a median effective radius of 2.5 kpc, and larger galaxies have a higher total SFR and stellar mass. Compared with their high-redshift analogues, we find evidence that LBGs at lower redshifts are larger, redder in the UV continuum, and have a major presence of older stellar populations in their SEDs. However, we do not find significant differences in the distributions of stellar mass or dust attenuation. ©2013 The Authors Published by Oxford University Press on be

Details

Database :
OAIster
Notes :
English
Publication Type :
Electronic Resource
Accession number :
edsoai.on1103420553
Document Type :
Electronic Resource