THE DUST ATTENUATION LAW IN DISTANT GALAXIES: EVIDENCE FOR VARIATION WITH SPECTRAL TYPE
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- 5 September 2013
- journal article
- Published by American Astronomical Society in The Astrophysical Journal Letters
- Vol. 775 (1) , L16
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- GOODS-Herschel: dust attenuation properties of UV selected high redshift galaxiesAstronomy & Astrophysics, 2012
- UV-CONTINUUM SLOPES ATz∼ 4-7 FROM THE HUDF09+ERS+CANDELS OBSERVATIONS: DISCOVERY OF A WELL-DEFINED UV COLOR-MAGNITUDE RELATIONSHIP FORz⩾ 4 STAR-FORMING GALAXIESThe Astrophysical Journal, 2012
- GOODS-Herschel: evidence of a UV extinction bump in galaxies atz > 1Astronomy & Astrophysics, 2011
- THE NUMBER DENSITY AND MASS DENSITY OF STAR-FORMING AND QUIESCENT GALAXIES AT 0.4 ⩽z⩽ 2.2The Astrophysical Journal, 2011
- EAZY: A Fast, Public Photometric Redshift CodeThe Astrophysical Journal, 2008
- Star formation and dust attenuation properties in galaxies from a statistical ultraviolet-to-far-infrared analysisMonthly Notices of the Royal Astronomical Society, 2005
- Galactic Stellar and Substellar Initial Mass FunctionPublications of the Astronomical Society of the Pacific, 2003
- The Dust Content and Opacity of Actively Star‐forming GalaxiesThe Astrophysical Journal, 2000
- Dust extinction of the stellar continua in starburst galaxies: The ultraviolet and optical extinction lawThe Astrophysical Journal, 1994
- The relationship between infrared, optical, and ultraviolet extinctionThe Astrophysical Journal, 1989