Contribution of the first galaxies to the cosmic far-infrared/sub-millimeter background - I. Mean background level

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We study the contribution of the first galaxies to the far-infrared/sub-millimeter (FIR/sub-mm) extragalactic background light (EBL) by implementing an analytical model for dust emission. We explore different dust models, assuming different grain-size distributions and chemical compositions. Accordi...

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Autor principal: De Rossi, María Emilia
Otros Autores: Bromm, V.
Formato: Capítulo de libro
Lenguaje:Inglés
Publicado: Oxford University Press 2017
Acceso en línea:Registro en Scopus
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Biblioteca Central Dr. Luis F. Leloir (FCEN) de Universidad de Buenos Aires
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100 1 |a De Rossi, María Emilia 
245 1 0 |a Contribution of the first galaxies to the cosmic far-infrared/sub-millimeter background - I. Mean background level 
260 |b Oxford University Press  |c 2017 
270 1 0 |m De Rossi, M.E.; Consejo Nacional de Investigaciones Científicas y Técnicas, Av. Rivadavia 1917, Argentina; email: mariaemilia.dr@gmail.com 
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506 |2 openaire  |e Política editorial 
520 3 |a We study the contribution of the first galaxies to the far-infrared/sub-millimeter (FIR/sub-mm) extragalactic background light (EBL) by implementing an analytical model for dust emission. We explore different dust models, assuming different grain-size distributions and chemical compositions. According to our findings, observed reradiated emission from dust in dwarfsize galaxies at z ~ 10 would peak at a wavelength of ~500 μm with observed fluxes of ~10 -3 -10 -2 nJy, which is below the capabilities of current observatories. In order to be detectable, model sources at these high redshifts should exhibit luminosities of ≳10 12 L ⊙ , comparable to that of local ultraluminous systems. The FIR/sub-mm-EBL generated by primeval galaxies peaks at ~500 μm, with an intensity ranging from ~10 -4 to 10 -3 nWm -2 sr -1 , depending on dust properties. These values are ~3-4 orders of magnitude below the absolute measured cosmic background level, suggesting that the first galaxies would not contribute significantly to the observed FIR/sub-mm-EBL. Our model EBL exhibits a strong correlation with the dust-to-metal ratio, where we assume a fiducial value of D = 0.005, increasing almost proportionally to it. Thus, measurements of the FIR/sub-mm-EBL could provide constraints on the amount of dust in the early Universe. Even if the absolute signal from primeval dust emission may be undetectable, it might still be possible to obtain information about it by exploring angular fluctuations at ~500 μm, close to the peak of dust emission from the first galaxies. © 2016 The Authors.  |l eng 
593 |a Consejo Nacional de Investigaciones Científicas y Técnicas, Av. Rivadavia 1917, Buenos Aires, C1033AAJ, Argentina 
593 |a Instituto de Astronomía y Física del Espacio (IAFE, CONICET-UBA), CC 67, Suc. 28, Buenos Aires, 1428, Argentina 
593 |a Department of Astronomy, University of Texas at Austin, 2511 Speedway, Austin, TX 78712, United States 
690 1 0 |a COSMOLOGY: THEORY 
690 1 0 |a GALAXIES: ABUNDANCES 
690 1 0 |a GALAXIES: EVOLUTION 
690 1 0 |a GALAXIES: HALOES 
690 1 0 |a GALAXIES: HIGHREDSHIFT 
690 1 0 |a GALAXIES: STAR FORMATION 
700 1 |a Bromm, V. 
773 0 |d Oxford University Press, 2017  |g v. 465  |h pp. 3668-3679  |k n. 3  |p Mon. Not. R. Astron. Soc.  |x 00358711  |w (AR-BaUEN)CENRE-6169  |t Monthly Notices of the Royal Astronomical Society 
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856 4 0 |u https://doi.org/10.1093/mnras/stw2971  |x doi  |y DOI 
856 4 0 |u https://hdl.handle.net/20.500.12110/paper_00358711_v465_n3_p3668_DeRossi  |x handle  |y Handle 
856 4 0 |u https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_00358711_v465_n3_p3668_DeRossi  |x registro  |y Registro en la Biblioteca Digital 
961 |a paper_00358711_v465_n3_p3668_DeRossi  |b paper  |c PE 
962 |a info:eu-repo/semantics/article  |a info:ar-repo/semantics/artículo  |b info:eu-repo/semantics/publishedVersion 

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