The HDUV Survey: A Revised Assessment of the Relationship between UV Slope and Dust Attenuation for High-redshift Galaxies-Reference-Cited by-同舟云学术

The HDUV Survey: A Revised Assessment of the Relationship between UV Slope and Dust Attenuation for High-redshift Galaxies

Published:2018-01-23 Issue:1 Volume:853 Page:56
ISSN:1538-4357
Container-title:The Astrophysical Journal
language:
Short-container-title:ApJ

Author:

Reddy Naveen A.^ORCID,Oesch Pascal A.^ORCID,Bouwens Rychard J.^ORCID,Montes Mireia,Illingworth Garth D.,Steidel Charles C.^ORCID,van Dokkum Pieter G.^ORCID,Atek Hakim^ORCID,Carollo Marcella C.^ORCID,Cibinel Anna^ORCID,Holden Brad^ORCID,Labbé Ivo^ORCID,Magee Dan,Morselli Laura,Nelson Erica J.^ORCID,Wilkins Steve

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://stacks.iop.org/0004-637X/853/i=1/a=56/pdf

Reference186 articles.

1. Multiwavelength Observations of Dusty Star Formation at Low and High Redshift

2. ULTRA-FAINT ULTRAVIOLET GALAXIES ATz∼ 2 BEHIND THE LENSING CLUSTER A1689: THE LUMINOSITY FUNCTION, DUST EXTINCTION, AND STAR FORMATION RATE DENSITY

3. THE EVOLUTION OF THE FAINT END OF THE UV LUMINOSITY FUNCTION DURING THE PEAK EPOCH OF STAR FORMATION $(1\lt z\lt 3)$

4. Obscured Star Formation in the Central Region of the Dwarf Galaxy NGC 5253

5. Dust properties of Lyman-break galaxies atz~ 3

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