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Galaxy And Mass Assembly (GAMA) : the stellar mass budget by galaxy type

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Driver_2016_StellarMassBudget_MNRAS_FinalPubVersion.pdf (3.175Mb)
Date
01/04/2016
Author
Moffett, Amanda J.
Ingarfield, Stephen A.
Driver, Simon Peter
Robotham, Aaron S. G.
Kelvin, Lee S.
Lange, Rebecca
Meštrić, Uroš
Alpaslan, Mehmet
Baldry, Ivan K.
Bland-Hawthorn, Joss
Brough, Sarah
Cluver, Michelle E.
Davies, Luke J. M.
Holwerda, Benne W.
Hopkins, Andrew M.
Kafle, Prajwal R.
Kennedy, Rebecca
Norberg, Peder
Taylor, Edward N.
Funder
Science & Technology Facilities Council
Grant ID
Keywords
Galaxies: elliptical and lenticular, cD
Galaxies: fundamental paramaters
Galaxies: luminosity function, mass function
Galaxies: spiral
Galaxies: statistics
QB Astronomy
QC Physics
NDAS
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Abstract
We report an expanded sample of visual morphological classifications from the Galaxy and Mass Assembly survey phase two, which now includes 7556 objects (previously 3727 in phase one). We define a local (z 
Citation
Moffett , A J , Ingarfield , S A , Driver , S P , Robotham , A S G , Kelvin , L S , Lange , R , Meštrić , U , Alpaslan , M , Baldry , I K , Bland-Hawthorn , J , Brough , S , Cluver , M E , Davies , L J M , Holwerda , B W , Hopkins , A M , Kafle , P R , Kennedy , R , Norberg , P & Taylor , E N 2016 , ' Galaxy And Mass Assembly (GAMA) : the stellar mass budget by galaxy type ' , Monthly Notices of the Royal Astronomical Society , vol. 457 , no. 2 , pp. 1308-1319 . https://doi.org/10.1093/mnras/stv2883
Publication
Monthly Notices of the Royal Astronomical Society
Status
Peer reviewed
DOI
https://doi.org/10.1093/mnras/stv2883
ISSN
0035-8711
Type
Journal article
Rights
© 2016 The Authors. Published by Oxford University Press on behalf of the Royal Astronomical Society. . This work is made available online in accordance with the publisher’s policies. This is the final published version of the work, which was originally published at: https://dx.doi.org/10.1093/mnras/stv2883
Description
SPD and AJM acknowledge funding support from the Australian Research Council under Discovery Project grant 130103505. SB acknowledges funding support from the Australian Research Council through a Future Fellowship (FT140101166). GAMA is funded by the STFC (UK), the ARC (Australia), the AAO, and the participating institutions. Funding for the SDSS and SDSS-II has been provided by the Alfred P. Sloan Foundation, the Participating Institutions, the National Science Foundation, the US Department of Energy, the National Aeronautics and Space Administration, the Japanese Monbukagakusho, the Max Planck Society, and the Higher Education Funding Council for England.
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  • University of St Andrews Research
URI
http://hdl.handle.net/10023/8718

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