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AGN - Dust-Obscured Galaxies at z~1-3 revealed by near-to-far infrared SED-fitting

Published online by Cambridge University Press:  17 August 2016

Laurie Riguccini
Laurie Riguccini*
Affiliation:
Observatório do Valongo, UFRJ, Brazil (riguccini@astro.ufrj.br) CAPES/BJT Science Without Borders Postdoctoral Fellow, Brazil
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Dust-Obscured galaxies (DOGs, Dey et al. 2008) are bright 24μm-selected sources with extreme obscuration at optical wavelengths (F24μ m/FR > 982). Recent studies (Dey et al. 2008, Bussmann et al. 2009) describe an evolutionary scenario in which the starbursting nature of submillimeter galaxies (SMGs) evolves into the composite nature of DOGs as an underlying AGN grows; this is followed by a quasar phase that terminates star formation (SF), leading to the formation of a passive, massive elliptical galaxy. Within this context, DOGs could provide a key insight to an extremely dusty stage in the evolution of galaxies at z ~ 2, where both AGN and SF activity coexist.

Keywords

galaxies: high-redshiftcosmology: observationsinfrared: galaxies
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 11 , Symposium S319: Galaxies at High Redshift and Their Evolution Over Cosmic Time , August 2015 , pp. 63
Copyright
Copyright © International Astronomical Union 2016 

References

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