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Abstract:

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.

Registro:

Documento: Artículo
Título:Contribution of the first galaxies to the cosmic far-infrared/sub-millimeter background - I. Mean background level
Autor:De Rossi, M.E.; Bromm, V.
Filiación:Consejo Nacional de Investigaciones Científicas y Técnicas, Av. Rivadavia 1917, Buenos Aires, C1033AAJ, Argentina
Instituto de Astronomía y Física del Espacio (IAFE, CONICET-UBA), CC 67, Suc. 28, Buenos Aires, 1428, Argentina
Department of Astronomy, University of Texas at Austin, 2511 Speedway, Austin, TX 78712, United States
Palabras clave:Cosmology: theory; Galaxies: abundances; Galaxies: evolution; Galaxies: haloes; Galaxies: highredshift; Galaxies: star formation
Año:2017
Volumen:465
Número:3
Página de inicio:3668
Página de fin:3679
DOI: http://dx.doi.org/10.1093/mnras/stw2971
Título revista:Monthly Notices of the Royal Astronomical Society
Título revista abreviado:Mon. Not. R. Astron. Soc.
ISSN:00358711
CODEN:MNRAA
Registro:https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_00358711_v465_n3_p3668_DeRossi

Referencias:

  • Abel, T., Bryan, G.L., Norman, M.L., (2002) Science, 295, p. 93
  • Allende Prieto, C., Lambert, D.L., Asplund, M., (2001) ApJ, 556, p. L63
  • Arendt, R.G., Kashlinsky, A., Moseley, S.H., Mather, J., (2010) ApJS, 186, p. 10
  • Asplund, M., Grevesse, N., Sauval, A.J., (2005) ASP Conf. Ser., Cosmic Abundances as Records of Stellar Evolution and Nucleosynthesis, 336, p. 25. , Barnes T. G., III, Bash F. N., eds, Astron. Soc. Pac., San Francisco
  • Asplund, M., Grevesse, N., Sauval, A.J., Scott, P., (2009) ARA&A, 47, p. 481
  • Barkana, R., Loeb, A., (2001) Phys. Rep, 349, p. 125
  • Beichman, C.A., Helou, G., (1991) ApJ, 370, p. L1
  • Berta, S., (2010) A&A, 518, p. L30
  • Béthermin, M., Dole, H., Cousin, M., Bavouzet, N., (2010) A&A, 516, p. A43
  • Béthermin, M., (2012) A&A, 542, p. A58
  • Bianchi, S., Schneider, R., (2007) MNRAS, 378, p. 973
  • Binney, J., Tremaine, S., (2008) Galactic Dynamics, 2nd edn, , Princeton Univ. Press, Princeton, NJ
  • Bromm, V., (2013) A.A.A. Book Series of the Argentine Astronomical Society, Proceedings of the SecondWorkshop on Numerical and Observational Astrophysics: From the First Structures to the Universe Today, 4, p. 3. , inDe Rossi M. E., Pedrosa S.E., Pellizza L.J., eds. Asociacion Argentina de Astronomia, La Plata, Argentina
  • Bromm, V., (2013) Rep. Prog. Phys, 76
  • Bromm, V., Larson, R.B., (2004) ARA&A, 42, p. 79
  • Bromm, V., Loeb, A., (2003) Nature, 425, p. 812
  • Bromm, V., Yoshida, N., (2011) ARA&A, 49, p. 373
  • Bromm, V., Coppi, P.S., Larson, R.B., (2002) ApJ, 564, p. 23
  • Bromm, V., Yoshida, N., Hernquist, L., McKee, C.F., (2009) Nature, 459, p. 49
  • Burkert, A., (1995) ApJ, 447, p. L25
  • Cai, Z.-Y., (2013) ApJ, 768, p. 21
  • Carniani, S., (2015) A&A, 584, p. A78
  • Carr, B.J., Bond, J.R., Arnett, W.D., (1984) ApJ, 277, p. 445
  • Casey, C.M., Narayanan, D., Cooray, A., (2014) Phys. Rep, 541, p. 45
  • Cen, R., Kimm, T., (2014) ApJ, 782, p. 32
  • Cherchneff, I., Dwek, E., (2010) ApJ, 713, p. 1
  • Chiaki, G., Marassi, S., Nozawa, T., Yoshida, N., Schneider, R., Omukai, K., Limongi, M., Chieffi, A., (2015) MNRAS, 446, p. 2659
  • Condon, J.J., (1974) ApJ, 188, p. 279
  • Cooray, A., Yoshida, N., (2004) MNRAS, 351, p. L71
  • Cooray, A., Bock, J.J., Keatin, B., Lange, A.E., Matsumoto, T., (2004) ApJ, 606, p. 611
  • Coppin, K., (2006) MNRAS, 372, p. 1621
  • Couchman, H.M.P., Rees, M.J., (1986) MNRAS, 221, p. 53
  • Dole, H., (2006) A&A, 451, p. 417
  • Dopcke, G., Glover, S.C.O., Clark, P.C., Klessen, R.S., (2013) ApJ, 766, p. 103
  • Draine, B.T., (2011) Physics of the Interstellar and Intergalactic Medium, , Princeton Univ. Press, Princeton, NJ
  • Draine, B.T., Li, A., (2001) ApJ, 551, p. 807
  • Dwek, E., Krennrich, F., (2013) Astropart. Phys, 43, p. 112
  • Dwek, E., (1998) ApJ, 508, p. 106
  • Eales, S., Lilly, S., Webb, T., Dunne, L., Gear, W., Clements, D., Yun, M., (2000) AJ, 120, p. 2244
  • Ferland, G.J., Korista, K.T., Verner, D.A., Ferguson, J.W., Kingdon, J.B., Verner, E.M., (1998) PASP, 110, p. 761
  • Finkbeiner, D.P., Davis, M., Schlegel, D.J., (2000) ApJ, 544, p. 81
  • Fixsen, D.J., Dwek, E., Mather, J.C., Bennett, C.L., Shafer, R.A., (1998) ApJ, 508, p. 123
  • Frebel, A., Johnson, J.L., Bromm, V., (2007) MNRAS, 380, p. L40
  • Fujimoto, S., Ouchi, M., Ono, Y., Shibuya, T., Ishigaki, M., Nagai, H., Momose, R., (2016) ApJS, 222, p. 1
  • Furlanetto, S.R., Loeb, A., (2003) ApJ, 588, p. 18
  • Gall, C., Hjorth, J., Andersen, A.C., (2011) A&AR, 19, p. 43
  • Greif, T.H., Bromm, V., (2006) MNRAS, 373, p. 128
  • Greif, T.H., Springel, V., White, S.D.M., Glover, S.C.O., Clark, P.C., Smith, R.J., Klessen, R.S., Bromm, V., (2011) ApJ, 737, p. 75
  • Haiman, Z., Thoul, A.A., Loeb, A., (1996) ApJ, 464, p. 523
  • Hatsukade, B., Ohta, K., Seko, A., Yabe, K., Akiyama, M., (2013) ApJ, 769, p. L27
  • Hauser, M.G., Dwek, E., (2001) ARA&A, 39, p. 249
  • Hauser, M.G., (1998) ApJ, 508, p. 25
  • Helgason, K., Ricotti, M., Kashlinsky, A., Bromm, V., (2016) MNRAS, 455, p. 282
  • Hollenbach, D., McKee, C.F., (1979) ApJS, 41, p. 555
  • Ji, A.P., Frebel, A., Bromm, V., (2014) ApJ, 782, p. 95
  • Karlsson, T., Bromm, V., Bland-Hawthorn, J., (2013) Rev. Mod. Phys, 85, p. 809
  • Kashlinsky, A., (2005) Phys. Rep, 409, p. 361
  • Kashlinsky, A., Odenwald, S., (2000) ApJ, 528, p. 74
  • Kashlinsky, A., Mather, J.C., Odenwald, S., Hauser, M.G., (1996) ApJ, 470, p. 681
  • Kashlinsky, A., Mather, J.C., Odenwald, S., (1996) ApJ, 473, p. L9
  • Kashlinsky, A., Odenwald, S., Mather, J., Skrutskie, M.F., Cutri, R.M., (2002) ApJ, 579, p. L53
  • Kashlinsky, A., Arendt, R., Gardner, J.P., Mather, J.C., Moseley, S.H., (2004) ApJ, 608, p. 1
  • Kashlinsky, A., Arendt, R.G., Mather, J., Moseley, S.H., (2005) Nature, 438, p. 45
  • Kashlinsky, A., Arendt, R.G., Mather, J., Moseley, S.H., (2007) ApJ, 654, p. L1
  • Kashlinsky, A., Mather, J.C., Helgason, K., Arendt, R.G., Bromm, V., Moseley, S.H., (2015) ApJ, 804, p. 99
  • Kaufman, M., (1976) Ap&SS, 40, p. 369
  • Kormendy, J., Fisher, D.B., Cornell, M.E., Bender, R., (2009) ApJS, 182, p. 216
  • Kroupa, P., (2001) MNRAS, 322, p. 231
  • Larson, R.B., (1969) MNRAS, 145, p. 405
  • Leitherer, C., (1999) ApJS, 123, p. 3
  • Leiton, R., (2015) A&A, 579, p. A93
  • Loeb, A., (2010) How Did the First Stars and Galaxies Form? Princeton Univ, , Press, Princeton, NJ
  • Loeb, A., Haiman, Z., (1997) ApJ, 490, p. 571
  • Low, F.J., Tucker, W.H., (1968) Phys. Rev. Lett, 21, p. 1538
  • Magliocchetti, M., Salvaterra, R., Ferrara, A., (2003) MNRAS, 342, p. L25
  • Marsden, G., (2009) ApJ, 707, p. 1729
  • Matsuura, S., (2011) ApJ, 737, p. 2
  • Mayer, M., Duschl, W.J., (2005) MNRAS, 358, p. 614
  • Mitchell-Wynne, K., (2015) Nature Commun, 6, p. 7945
  • Navarro, J.F., Frenk, C.S., White, S.D.M., (1997) ApJ, 490, p. 493
  • Nozawa, T., Kozasa, T., (2013) ApJ, 776, p. 24
  • Omukai, K., (2000) ApJ, 534, p. 809
  • Omukai, K., Hosokawa, T., Yoshida, N., (2010) ApJ, 722, p. 1793
  • Ono, Y., Ouchi, M., Kurono, Y., Momose, R., (2014) ApJ, 795, p. 5
  • (2014) A&A, 571, p. A16
  • Pollack, J.B., Hollenbach, D., Beckwith, S., Simonelli, D.P., Roush, T., Fong, W., (1994) ApJ, 421, p. 615
  • Puget, J.-L., Abergel, A., Bernard, J.-P., Boulanger, F., Burton, W.B., Desert, F.-X., Hartmann, D., (1996) A&A, 308, p. L5
  • Safranek-Shrader, C., Bromm, V., Milosavljević, M., (2010) ApJ, 723, p. 1568
  • Safranek-Shrader, C., Milosavljević, M., Bromm, V., (2014) MNRAS, 438, p. 1669
  • Salvaterra, R., Ferrara, A., (2003) MNRAS, 339, p. 973
  • Salvaterra, R., Ferrara, A., (2006) MNRAS, 367, p. L11
  • Santos, M.R., Bromm, V., Kamionkowski, M., (2002) MNRAS, 336, p. 1082
  • Schlegel, D.J., Finkbeiner, D.P., Davis, M., (1998) ApJ, 500, p. 525
  • Schneider, R., Ferrara, A., Salvaterra, R., (2004) MNRAS, 351, p. 1379
  • Schneider, R., Omukai, K., Inoue, A.K., Ferrara, A., (2006) MNRAS, 369, p. 1437
  • Sheth, R.K., Mo, H.J., Tormen, G., (2001) MNRAS, 323, p. 1
  • Smith, A., Safranek-Shrader, C., Bromm, V., Milosavljević, M., (2015) MNRAS, 449, p. 4336
  • Stacy, A., Greif, T.H., Bromm, V., (2010) MNRAS, 403, p. 45
  • Tegmark, M., Silk, J., Rees, M.J., Blanchard, A., Abel, T., Palla, F., (1997) ApJ, 474, p. 1
  • Vázquez, G.A., Leitherer, C., (2005) ApJ, 621, p. 695
  • Viero, M.P., (2013) ApJ, 779, p. 32
  • Weiß, A., (2009) ApJ, 707, p. 1201
  • Wilson, G.W., (2008) MNRAS, 386, p. 807
  • Yoshida, N., Abel, T., Hernquist, L., Sugiyama, N., (2003) ApJ, 592, p. 645
  • Yoshida, N., Bromm, V., Hernquist, L., (2004) ApJ, 605, p. 579
  • Zackrisson, E., Rydberg, C.-E., Schaerer, D., Östlin, G., Tuli, M., (2011) ApJ, 740, p. 13

Citas:

---------- APA ----------
De Rossi, M.E. & Bromm, V. (2017) . Contribution of the first galaxies to the cosmic far-infrared/sub-millimeter background - I. Mean background level. Monthly Notices of the Royal Astronomical Society, 465(3), 3668-3679.
http://dx.doi.org/10.1093/mnras/stw2971
---------- CHICAGO ----------
De Rossi, M.E., Bromm, V. "Contribution of the first galaxies to the cosmic far-infrared/sub-millimeter background - I. Mean background level" . Monthly Notices of the Royal Astronomical Society 465, no. 3 (2017) : 3668-3679.
http://dx.doi.org/10.1093/mnras/stw2971
---------- MLA ----------
De Rossi, M.E., Bromm, V. "Contribution of the first galaxies to the cosmic far-infrared/sub-millimeter background - I. Mean background level" . Monthly Notices of the Royal Astronomical Society, vol. 465, no. 3, 2017, pp. 3668-3679.
http://dx.doi.org/10.1093/mnras/stw2971
---------- VANCOUVER ----------
De Rossi, M.E., Bromm, V. Contribution of the first galaxies to the cosmic far-infrared/sub-millimeter background - I. Mean background level. Mon. Not. R. Astron. Soc. 2017;465(3):3668-3679.
http://dx.doi.org/10.1093/mnras/stw2971