GAMA/G10-COSMOS/3D-HST: the 0 < z < 5 cosmic star formation history, stellar-mass, and dust-mass densities

Abstract We use the energy-balance code magphys to determine stellar and dust masses, and dust corrected star formation rates for over 200 000 GAMA galaxies, 170 000 G10-COSMOS galaxies, and 200 000 3D-HST galaxies. Our values agree well with previously reported measurements and constitute a represe...

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Veröffentlicht in:	Monthly notices of the Royal Astronomical Society 2018-04, Vol.475 (3), p.2891-2935
Hauptverfasser:	Driver, Simon P, Andrews, Stephen K, da Cunha, Elisabete, Davies, Luke J, Lagos, Claudia, Robotham, Aaron S G, Vinsen, Kevin, Wright, Angus H, Alpaslan, Mehmet, Bland-Hawthorn, Joss, Bourne, Nathan, Brough, Sarah, Bremer, Malcolm N, Cluver, Michelle, Colless, Matthew, Conselice, Christopher J, Dunne, Loretta, Eales, Steve A, Gomez, Haley, Holwerda, Benne, Hopkins, Andrew M, Kafle, Prajwal R, Kelvin, Lee S, Loveday, Jon, Liske, Jochen, Maddox, Steve J, Phillipps, Steven, Pimbblet, Kevin, Rowlands, Kate, Sansom, Anne E, Taylor, Edward, Wang, Lingyu, Wilkins, Stephen M
Format:	Artikel
Sprache:	eng
Schlagworte:	Cosmic dust Cosmos Density Dust Ejection Galaxies Initial mass function Interstellar matter Red shift Replenishment Star & galaxy formation Star formation Stellar evolution Stellar mass Universe
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Zusammenfassung:	Abstract We use the energy-balance code magphys to determine stellar and dust masses, and dust corrected star formation rates for over 200 000 GAMA galaxies, 170 000 G10-COSMOS galaxies, and 200 000 3D-HST galaxies. Our values agree well with previously reported measurements and constitute a representative and homogeneous data set spanning a broad range in stellar-mass (108–1012 M⊙), dust-mass (106–109 M⊙), and star formation rates (0.01–100 M⊙yr−1), and over a broad redshift range (0.0
ISSN:	0035-8711 1365-2966
DOI:	10.1093/mnras/stx2728