UV to IR luminosities and dust attenuation determined from ∼4000 k-selected galaxies at 1 < z < 3 in the ZFOURGE survey

Article


Forrest, Ben, Tran, Kim-Vy H., Tomczak, Adam R., Broussard, Adam, Labbé, Ivo, Papovich, Casey, Kriek, Mariska, Allen, Rebecca J., Cowley, Michael, Dickinson, Mark, Glazebrook, Karl, van Houdt, Josha, Inami, Hanae, Kacprzak, Glenn G., Kawinwanichakij, Lalitwadee, Kelson, Daniel, McCarthy, Patrick J., Monson, Andrew, Morrison, Glenn, ..., Tilvi, Vithal. 2016. "UV to IR luminosities and dust attenuation determined from ∼4000 k-selected galaxies at 1 < z < 3 in the ZFOURGE survey." The Astrophysical Journal Letters. 818 (2). https://doi.org/10.3847/2041-8205/818/2/L26
Article Title

UV to IR luminosities and dust attenuation determined from ∼4000 k-selected galaxies at 1 < z < 3 in the ZFOURGE survey

ERA Journal ID45091
Article CategoryArticle
AuthorsForrest, Ben, Tran, Kim-Vy H., Tomczak, Adam R., Broussard, Adam, Labbé, Ivo, Papovich, Casey, Kriek, Mariska, Allen, Rebecca J., Cowley, Michael, Dickinson, Mark, Glazebrook, Karl, van Houdt, Josha, Inami, Hanae, Kacprzak, Glenn G., Kawinwanichakij, Lalitwadee, Kelson, Daniel, McCarthy, Patrick J., Monson, Andrew, Morrison, Glenn, Nanayakkara, Themiya, Persson, S. Eric, Quadri, Ryan F., Spitler, Lee R., Straatman, Caroline and Tilvi, Vithal
Journal TitleThe Astrophysical Journal Letters
Journal Citation818 (2)
Article NumberL26
Number of Pages6
Year2016
PublisherIOP Publishing
Place of PublicationUnited Kingdom
ISSN2041-8205
2041-8213
Digital Object Identifier (DOI)https://doi.org/10.3847/2041-8205/818/2/L26
Web Address (URL)https://iopscience.iop.org/article/10.3847/2041-8205/818/2/L26
Abstract

We build a set of composite galaxy spectral energy distributions (SEDs) by de-redshifting and scaling multi-wavelength photometry from galaxies in the ZFOURGE survey, covering the CDFS, COSMOS, and UDS fields. From a sample of ∼4000 Ks-band selected galaxies, we define 38 composite galaxy SEDs that yield continuous low-resolution spectra (R ∼ 45) over the rest-frame range 0.1-4 μm. Additionally, we include far infrared photometry from the Spitzer Space Telescope and the Herschel Space Observatory to characterize the infrared properties of our diverse set of composite SEDs. From these composite SEDs we analyze the rest-frame UVJ colors, as well as the ratio of IR to UV light (IRX) and the UV slope (β) in the IRX-β dust relation at 1 < z < 3. Blue star-forming composite SEDs show IRX and β values consistent with local relations; dusty star-forming galaxies have considerable scatter, as found for local IR bright sources, but on average appear bluer than expected for their IR fluxes. We measure a tight linear relation between rest-frame UVJ colors and dust attenuation for star-forming composites, providing a direct method for estimating dust content from either (U - V) or rest-frame colors for star-forming galaxies at intermediate redshifts.

Keywordsgalaxies: high-redshift; galaxies: star formation; infrared: galaxies; ultraviolet: galaxies
Contains Sensitive ContentDoes not contain sensitive content
ANZSRC Field of Research 20205199. Other physical sciences
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FunderDirectorate for Mathematical and Physical Sciences
Byline AffiliationsTexas A&M University, United States
University of California Davis, United States
Leiden University, Netherlands
University of California Berkeley, United States
Swinburne University of Technology
School of Mathematics, Physics and Computing
National Optical Astronomy Observatory, United States
Carnegie Observatories Pasadena, United States
University of Hawaii, United States
Canada-France-Hawaii Telescope, United States
Australian Astronomical Observatory, Australia
Macquarie University
Arizona State University, United States
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https://research.usq.edu.au/item/w45xy/uv-to-ir-luminosities-and-dust-attenuation-determined-from-4000-k-selected-galaxies-at-1-z-3-in-the-zfourge-survey

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