Files in this item
GAMA/G10-COSMOS/3D-HST : the 0 < z < 5 cosmic star formation history, stellar- and dust-mass densities
Item metadata
dc.contributor.author | Driver, Simon P. | |
dc.contributor.author | Andrews, Stephen K. | |
dc.contributor.author | Cunha, Elisabete da | |
dc.contributor.author | Davies, Luke J. | |
dc.contributor.author | Lagos, Claudia | |
dc.contributor.author | Robotham, Aaron S. G. | |
dc.contributor.author | Vinsen, Kevin | |
dc.contributor.author | Wright, Angus H. | |
dc.contributor.author | Alpaslan, Mehmet | |
dc.contributor.author | Bland-Hawthorn, Joss | |
dc.contributor.author | Bourne, Nathan | |
dc.contributor.author | Brough, Sarah | |
dc.contributor.author | Bremer, Malcolm N. | |
dc.contributor.author | Cluver, Michelle | |
dc.contributor.author | Colless, Matthew | |
dc.contributor.author | Conselice, Christopher J. | |
dc.contributor.author | Dunne, Loretta | |
dc.contributor.author | Eales, Steve A. | |
dc.contributor.author | Gomez, Haley | |
dc.contributor.author | Holwerda, Benne | |
dc.contributor.author | Hopkins, Andrew M. | |
dc.contributor.author | Kafle, Prajwal R. | |
dc.contributor.author | Kelvin, Lee S. | |
dc.contributor.author | Loveday, Jon | |
dc.contributor.author | Liske, Jochen | |
dc.contributor.author | Maddox, Steve J. | |
dc.contributor.author | Phillipps, Steven | |
dc.contributor.author | Pimbblet, Kevin | |
dc.contributor.author | Rowlands, Kate | |
dc.contributor.author | Sansom, Anne E. | |
dc.contributor.author | Taylor, Edward | |
dc.contributor.author | Wang, Lingyu | |
dc.contributor.author | Wilkins, Stephen M. | |
dc.date.accessioned | 2018-01-29T16:30:12Z | |
dc.date.available | 2018-01-29T16:30:12Z | |
dc.date.issued | 2018-04 | |
dc.identifier | 252089984 | |
dc.identifier | 8e5176f2-0fd1-4a00-9be5-38304a5c7dc1 | |
dc.identifier | 000427141900004 | |
dc.identifier | 85095244380 | |
dc.identifier.citation | Driver , S P , Andrews , S K , Cunha , E D , Davies , L J , Lagos , C , Robotham , A S G , Vinsen , K , Wright , A H , Alpaslan , M , Bland-Hawthorn , J , Bourne , N , Brough , S , Bremer , M N , Cluver , M , Colless , M , Conselice , C J , Dunne , L , Eales , S A , Gomez , H , Holwerda , B , Hopkins , A M , Kafle , P R , Kelvin , L S , Loveday , J , Liske , J , Maddox , S J , Phillipps , S , Pimbblet , K , Rowlands , K , Sansom , A E , Taylor , E , Wang , L & Wilkins , S M 2018 , ' GAMA/G10-COSMOS/3D-HST : the 0 < z < 5 cosmic star formation history, stellar- and dust-mass densities ' , Monthly Notices of the Royal Astronomical Society , vol. 475 , no. 3 , pp. 2891-2935 . https://doi.org/10.1093/mnras/stx2728 | en |
dc.identifier.issn | 0035-8711 | |
dc.identifier.other | ArXiv: http://arxiv.org/abs/1710.06628v2 | |
dc.identifier.uri | https://hdl.handle.net/10023/12629 | |
dc.description.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—1012M⊙), dust mass (106—109M⊙), and star-formation rates (0.01—100M⊙yr−1), and over a broad redshift range (0.0 < z < 5.0). We combine these data to measure the cosmic star-formation history (CSFH), the stellar-mass density (SMD), and the dust-mass density (DMD) over a 12 Gyr timeline. The data mostly agree with previous estimates, where they exist, and provide a quasi-homogeneous data set using consistent mass and star-formation estimators with consistent underlying assumptions over the full time range. As a consequence our formal errors are significantly reduced when compared to the historic literature. Integrating our CSFH we precisely reproduce the SMD with an interstellar medium replenishment factor of 0.50 ± 0.07, consistent with our choice of Chabrier intial mass function plus some modest amount of stripped stellar mass. Exploring the cosmic dust density evolution, we find a gradual increase in dust density with lookback time. We build a simple phenomenological model from the CSFH to account for the dust mass evolution, and infer two key conclusions: (1) For every unit of stellar mass which is formed 0.0065—0.004 units of dust mass is also formed; (2) Over the history of the Universe approximately 90 to 95 per cent of all dust formed has been destroyed and/or ejected. | |
dc.format.extent | 24564395 | |
dc.language.iso | eng | |
dc.relation.ispartof | Monthly Notices of the Royal Astronomical Society | en |
dc.subject | Astronomical databases: misc | en |
dc.subject | Galaxies: evolution | en |
dc.subject | Galaxies: general | en |
dc.subject | Galaxies: individual | en |
dc.subject | Galaxies: photometry | en |
dc.subject | Cosmology: observations | en |
dc.subject | QB Astronomy | en |
dc.subject | QC Physics | en |
dc.subject | 3rd-DAS | en |
dc.subject | BDC | en |
dc.subject.lcc | QB | en |
dc.subject.lcc | QC | en |
dc.title | GAMA/G10-COSMOS/3D-HST : the 0 < z < 5 cosmic star formation history, stellar- and dust-mass densities | en |
dc.type | Journal article | en |
dc.contributor.institution | University of St Andrews. School of Physics and Astronomy | en |
dc.identifier.doi | https://doi.org/10.1093/mnras/stx2728 | |
dc.description.status | Peer reviewed | en |
This item appears in the following Collection(s)
Items in the St Andrews Research Repository are protected by copyright, with all rights reserved, unless otherwise indicated.