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Cambridge University Press (CUP), Proceedings of the International Astronomical Union, S235(2), p. 428-428

DOI: 10.1017/s1743921306010556

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Obtaining the (dust-obscured) star formation history using the VLA-COSMOS survey

Journal article published in 2006 by V. Smolčić, E. Schinnerer ORCID, M. Scodeggio, C. L. Carilli, P. Franzetti, K. Jahnke ORCID
This paper was not found in any repository, but could be made available legally by the author.
This paper was not found in any repository, but could be made available legally by the author.

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Abstract

AbstractUsing the multi-wavelength COSMOS survey (Scoville et al. 2006), we develop a method based on purely photometric data to separate the faint VLA-COSMOS radio population into star-forming (SF) galaxies and active-galactic nuclei (AGN). Based on this classification method we select SF galaxies within our sample and present first results on the cosmic (dust-obscured) star-formation history based on VLA-COSMOS (Schinnerer et al. 2006) radio data.

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