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Dust Attenuation in UV-selected Starbursts at High Redshift and Their Local Counterparts: Implications for the Cosmic Star Formation Rate Density

Overzier, Roderik A. and Heckman, Timothy M. and Wang, Jing and Armus, Lee and Buat, Veronique and Howell, Justin and Meurer, Gerhardt and Seibert, Mark and Siana, Brian and Basu-Zych, Antara and Charlot, Stéphane and Gonçalves, Thiago S. and Martin, D. Christopher and Neill, James D. and Rich, R. Michael and Salim, Samir and Schiminovich, David (2001) Dust Attenuation in UV-selected Starbursts at High Redshift and Their Local Counterparts: Implications for the Cosmic Star Formation Rate Density. Astrophysical Journal Letters, 726 (1). Art. No. L7. ISSN 2041-8213. https://resolver.caltech.edu/CaltechAUTHORS:20170408-144019952

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Abstract

We present a new analysis of the dust obscuration in starburst galaxies at low and high redshifts. This study is motivated by our unique sample of the most extreme UV-selected starburst galaxies in the nearby universe (z < 0.3), found to be good analogs of high-redshift Lyman break galaxies (LBGs) in most of their physical properties. We find that the dust properties of the Lyman break analogs (LBAs) are consistent with the relation derived previously by Meurer et al. (M99) that is commonly used to dust-correct star formation rate (SFR) measurements at a very wide range of redshifts. We directly compare our results with high-redshift samples (LBGs, "BzK," and submillimeter galaxies at z ~ 2-3) having IR data either from Spitzer or Herschel. The attenuation in typical LBGs at z ~ 2-3 and LBAs is very similar. Because LBAs are much better analogs to LBGs compared to previous local star-forming samples, including M99, the practice of dust-correcting the SFRs of high-redshift galaxies based on the local calibration is now placed on a much more solid ground. We illustrate the importance of this result by showing how the locally calibrated relation between UV measurements and extinction is used to estimate the integrated, dust-corrected SFR density at z ≃ 2-6.


Item Type:Article
Related URLs:
URLURL TypeDescription
http://dx.doi.org/10.1088/2041-8205/726/1/L7DOIArticle
http://arxiv.org/abs/1011.6098arXivDiscussion Paper
ORCID:
AuthorORCID
Armus, Lee0000-0003-3498-2973
Seibert, Mark0000-0002-1143-5515
Siana, Brian0000-0002-4935-9511
Martin, D. Christopher0000-0002-8650-1644
Neill, James D.0000-0002-0466-1119
Rich, R. Michael0000-0003-0427-8387
Salim, Samir0000-0003-2342-7501
Additional Information:© 2011. The American Astronomical Society. Received 2010 November 4; accepted 2010 November 24; published 2010 December 10. We thank Guinevere Kauffmann, Rychard Bouwens, Luca Cortese, and Ranga-Ram Chary for providing useful comments.
Group:Infrared Processing and Analysis Center (IPAC)
Subject Keywords:dust, extinction; galaxies: high-redshift; galaxies: peculiar; galaxies: starburst
Issue or Number:1
Record Number:CaltechAUTHORS:20170408-144019952
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20170408-144019952
Official Citation:Roderik A. Overzier et al 2011 ApJL 726 L7
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:75988
Collection:CaltechAUTHORS
Deposited By: 1Science Import
Deposited On:26 Apr 2017 23:36
Last Modified:03 Oct 2019 16:56

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