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HerMES: Lyman Break Galaxies Individually Detected at 0.7 ≤ z ≤ 2.0 in GOODS-N with Herschel/SPIRE

Burgarella, D. and Bock, J. and Cooray, A. and Vieira, J. D. and Viero, M. (2011) HerMES: Lyman Break Galaxies Individually Detected at 0.7 ≤ z ≤ 2.0 in GOODS-N with Herschel/SPIRE. Astrophysical Journal Letters, 734 (1). Art. No. L12. ISSN 0004-637X. http://resolver.caltech.edu/CaltechAUTHORS:20110826-141031886

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Abstract

As part of the Herschel Multi-tiered Extragalactic Survey we have investigated the rest-frame far-infrared (FIR) properties of a sample of more than 4800 Lyman break galaxies (LBGs) in the Great Observatories Origins Deep Survey North field. Most LBGs are not detected individually, but we do detect a sub-sample of 12 objects at 0.7 < z < 1.6 and one object at z = 2.0. The ones detected by Herschel SPIRE have redder observed NUV – U and U – R colors than the others, while the undetected ones have colors consistent with average LBGs at z > 2.5. The UV-to-FIR spectral energy distributions of the objects detected in the rest-frame FIR are investigated using the code CIGALE to estimate physical parameters. We find that LBGs detected by SPIRE are high-mass, luminous infrared galaxies. It appears that LBGs are located in a triangle-shaped region in the A_(FUV) versus log L_(FUV) = 0 diagram limited by A_(FUV) = 0 at the bottom and by a diagonal following the temporal evolution of the most massive galaxies from the bottom right to the top left of the diagram. This upper envelop can be used as upper limits for the UV dust attenuation as a function of L_(FUV). The limits of this region are well explained using a closed-box model, where the chemical evolution of galaxies produces metals, which in turn lead to higher dust attenuation when the galaxies age.


Item Type:Article
Related URLs:
URLURL TypeDescription
http://dx.doi.org/10.1088/2041-8205/734/1/L12DOIUNSPECIFIED
http://iopscience.iop.org/2041-8205/734/1/L12PublisherUNSPECIFIED
Additional Information:© 2011 American Astronomical Society. Received 2011 January 31; accepted 2011 April 28; published 2011 May 19. SPIRE has been developed by a consortium of institutes led by Cardiff University (UK) and including University of Lethbridge (Canada); NAOC (China); CEA, OAMP (France); IFSI, University of Padua (Italy); IAC (Spain); Stockholm Observatory (Sweden); Imperial College London, RAL, UCL-MSSL, UKATC, University of Sussex (UK); and Caltech/ JPL, IPAC, University of Colorado (USA). This development has been supported by national funding agencies: CSA (Canada); NAOC (China); CEA, CNES, CNRS (France); ASI (Italy); MCINN (Spain); Stockholm Observatory (Sweden); STFC (UK); and NASA (USA). The data presented in this paper will be released through the Herschel Database in Marseille (HeDaM; http://hedam.oamp.fr/HerMES). This work makes use of TOPCAT (http://www.star.bristol.ac.uk/∼mbt/topcat/).
Group:TAPIR
Funders:
Funding AgencyGrant Number
CSA (Canada) UNSPECIFIED
NAOC (China) UNSPECIFIED
CEA (France)UNSPECIFIED
CNES (France) UNSPECIFIED
CNRS (France)UNSPECIFIED
ASI (Italy) UNSPECIFIED
MCINN (Spain)UNSPECIFIED
Stockholm Observatory (Sweden)UNSPECIFIED
STFC (UK)UNSPECIFIED
NASAUNSPECIFIED
Subject Keywords:galaxies: evolution; galaxies: formation; galaxies: high-redshift; infrared: galaxies; ultraviolet: galaxies
Classification Code:PACS: 95.80.+p; 98.62.Qz; 98.62.Bj; 98.54.Ep; 95.85.Gn; 98.62.Ai
Record Number:CaltechAUTHORS:20110826-141031886
Persistent URL:http://resolver.caltech.edu/CaltechAUTHORS:20110826-141031886
Official Citation:HerMES: Lyman Break Galaxies Individually Detected at 0.7 ≤ z ≤ 2.0 in GOODS-N with Herschel/SPIRE D. Burgarella et al. 2011 ApJ 734 L1
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:25131
Collection:CaltechAUTHORS
Deposited By: Jason Perez
Deposited On:01 Sep 2011 20:51
Last Modified:26 Mar 2014 20:52

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