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- W3102449281 endingPage "77" @default.
- W3102449281 startingPage "77" @default.
- W3102449281 abstract "Though half of cosmic starlight is absorbed by dust and reradiated at long wavelengths (3 μm–3 mm), constraints on the infrared through the millimeter galaxy luminosity function (or the IRLF) are poor in comparison to the rest-frame ultraviolet and optical galaxy luminosity functions, particularly at z ≳ 2.5. Here, we present a backward evolution model for interpreting number counts, redshift distributions, and cross-band flux density correlations in the infrared and submillimeter sky, from 70 μm–2 mm, using a model for the IRLF out to the epoch of reionization. Mock submillimeter maps are generated by injecting sources according to the prescribed IRLF and flux densities drawn from model spectral energy distributions that mirror the distribution of SEDs observed in 0 < z < 5 dusty star-forming galaxies (DSFGs). We explore two extreme hypothetical case studies: a dust-poor early universe model, where DSFGs contribute negligibly (<10%) to the integrated star formation rate density at z > 4; and an alternate dust-rich early universe model, where DSFGs dominate ∼90% of z > 4 star formation. We find that current submm/mm data sets do not clearly rule out either of these extreme models. We suggest that future surveys at 2 mm will be crucial to measuring the IRLF beyond z ∼ 4. The model framework developed in this paper serves as a unique tool for the interpretation of multiwavelength IR/submm extragalactic data sets, and will enable more refined constraints on the IRLF than can be made from direct measurements of individual galaxies' integrated dust emission." @default.
- W3102449281 created "2020-11-23" @default.
- W3102449281 creator A5001948002 @default.
- W3102449281 creator A5020070530 @default.
- W3102449281 creator A5024410226 @default.
- W3102449281 creator A5024515345 @default.
- W3102449281 creator A5039525765 @default.
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- W3102449281 creator A5064669275 @default.
- W3102449281 creator A5079179941 @default.
- W3102449281 creator A5084195858 @default.
- W3102449281 date "2018-07-25" @default.
- W3102449281 modified "2023-10-17" @default.
- W3102449281 title "The Brightest Galaxies in the Dark Ages: Galaxies’ Dust Continuum Emission during the Reionization Era" @default.
- W3102449281 cites W1484400061 @default.
- W3102449281 cites W1524555145 @default.
- W3102449281 cites W1631427681 @default.
- W3102449281 cites W1634409775 @default.
- W3102449281 cites W1681063222 @default.
- W3102449281 cites W1748091613 @default.
- W3102449281 cites W1768185998 @default.
- W3102449281 cites W1842880767 @default.
- W3102449281 cites W1851451509 @default.
- W3102449281 cites W1906992734 @default.
- W3102449281 cites W1908085087 @default.
- W3102449281 cites W1948197607 @default.
- W3102449281 cites W1965700990 @default.
- W3102449281 cites W1968809627 @default.
- W3102449281 cites W1969832966 @default.
- W3102449281 cites W1973808059 @default.
- W3102449281 cites W1973986763 @default.
- W3102449281 cites W1974668797 @default.
- W3102449281 cites W1977843574 @default.
- W3102449281 cites W1986738273 @default.
- W3102449281 cites W1994124960 @default.
- W3102449281 cites W1997638535 @default.
- W3102449281 cites W1998981512 @default.
- W3102449281 cites W2000840256 @default.
- W3102449281 cites W2004557233 @default.
- W3102449281 cites W2007741717 @default.
- W3102449281 cites W2008047915 @default.
- W3102449281 cites W2008991538 @default.
- W3102449281 cites W2012035798 @default.
- W3102449281 cites W2014727289 @default.
- W3102449281 cites W2015297451 @default.
- W3102449281 cites W2017100570 @default.
- W3102449281 cites W2017342089 @default.
- W3102449281 cites W2019562528 @default.
- W3102449281 cites W2020009551 @default.
- W3102449281 cites W2023842147 @default.
- W3102449281 cites W2025105301 @default.
- W3102449281 cites W2025717087 @default.
- W3102449281 cites W2026716300 @default.
- W3102449281 cites W2030954280 @default.
- W3102449281 cites W2031539306 @default.
- W3102449281 cites W2033731878 @default.
- W3102449281 cites W2035830593 @default.
- W3102449281 cites W2036319176 @default.
- W3102449281 cites W2037629290 @default.
- W3102449281 cites W2039833992 @default.
- W3102449281 cites W2039879975 @default.
- W3102449281 cites W2041084195 @default.
- W3102449281 cites W2043533977 @default.
- W3102449281 cites W2044189059 @default.
- W3102449281 cites W2047156688 @default.
- W3102449281 cites W2047758030 @default.
- W3102449281 cites W2047953583 @default.
- W3102449281 cites W2048274049 @default.
- W3102449281 cites W2051510431 @default.
- W3102449281 cites W2053591448 @default.
- W3102449281 cites W2056875413 @default.
- W3102449281 cites W2057589371 @default.
- W3102449281 cites W2057672934 @default.
- W3102449281 cites W2059302115 @default.
- W3102449281 cites W2059795572 @default.
- W3102449281 cites W2060422077 @default.
- W3102449281 cites W2060572005 @default.
- W3102449281 cites W2068577843 @default.
- W3102449281 cites W2074037441 @default.
- W3102449281 cites W2077261927 @default.
- W3102449281 cites W2083821946 @default.
- W3102449281 cites W2084061910 @default.
- W3102449281 cites W2084287642 @default.
- W3102449281 cites W2086328762 @default.
- W3102449281 cites W2087161795 @default.
- W3102449281 cites W2088650185 @default.
- W3102449281 cites W2092063722 @default.
- W3102449281 cites W2094181926 @default.
- W3102449281 cites W2094871238 @default.
- W3102449281 cites W2097790409 @default.
- W3102449281 cites W2099344750 @default.
- W3102449281 cites W2107202970 @default.
- W3102449281 cites W2111573846 @default.
- W3102449281 cites W2111600051 @default.
- W3102449281 cites W2111708005 @default.
- W3102449281 cites W2114880370 @default.
- W3102449281 cites W2116977143 @default.
- W3102449281 cites W2117038440 @default.