Galaxy And Mass Assembly (GAMA): stellar mass estimates
| Autor: | William J. Sutherland, Aaron S. G. Robotham, H. Parkinson, Ivan K. Baldry, Sarah Brough, Jon Loveday, Michael J. I. Brown, D. H. P. Jones, Konrad Kuijken, Scott M. Croom, Andrew M. Hopkins, D. Wijesinghe, Matthew Colless, David T. Hill, Joss Bland-Hawthorn, Kevin A. Pimbblet, R. G. Sharp, Jochen Liske, Cristina Popescu, Ewan Cameron, S. Phillipps, Madusha Gunawardhana, Simon P. Driver, John A. Peacock, R. J. Tuffs, Eelco van Kampen, Robert C. Nichol, Edward N. Taylor, C. J. Conselice, Matthew Prescott, Peder Norberg, Steven P. Bamford, Daniel Thomas, Lee S. Kelvin, Carlos S. Frenk |
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| Rok vydání: | 2011 |
| Předmět: |
Physics
Stellar mass Stellar population 010308 nuclear & particles physics Estimator Astronomy and Astrophysics Astrophysics::Cosmology and Extragalactic Astrophysics Astrophysics Redshift survey 01 natural sciences Galaxy Photometry (optics) Space and Planetary Science 0103 physical sciences Astrophysics::Solar and Stellar Astrophysics Astrophysics::Earth and Planetary Astrophysics 010303 astronomy & astrophysics Stellar evolution Data release Astrophysics::Galaxy Astrophysics |
| Zdroj: | Monthly Notices of the Royal Astronomical Society. 418:1587-1620 |
| ISSN: | 0035-8711 |
| Popis: | This paper describes the first catalogue of photometrically-derived stellar mass estimates for intermediate-redshift (z < 0.65) galaxies in the Galaxy And Mass Assembly (GAMA) spectroscopic redshift survey. These masses, as well as the full set of ancillary stellar population parameters, will be made public as part of GAMA data release 2. Although the GAMA database does include NIR photometry, we show that the quality of our stellar population synthesis fits is significantly poorer when these NIR data are included. Further, for a large fraction of galaxies, the stellar population parameters inferred from the optical-plus-NIR photometry are formally inconsistent with those inferred from the optical data alone. This may indicate problems in our stellar population library, or NIR data issues, or both; these issues will be addressed for future versions of the catalogue. For now, we have chosen to base our stellar mass estimates on optical photometry only. In light of our decision to ignore the available NIR data, we examine how well stellar mass can be constrained based on optical data alone. We use generic properties of stellar population synthesis models to demonstrate that restframe colour alone is in principle a very good estimator of stellar mass-to-light ratio, M*/Li. Further, we use the observed relation between restframe (g-i) and M*/Li for real GAMA galaxies to argue that, modulo uncertainties in the stellar evolution models themselves, (g-i) colour can in practice be used to estimate M*/Li to an accuracy of < ~0.1 dex. This 'empirically calibrated' (g-i)-M*/Li relation offers a simple and transparent means for estimating galaxies' stellar masses based on minimal data, and so provides a solid basis for other surveys to compare their results to z < ~0.4 measurements from GAMA. |
| Databáze: | OpenAIRE |
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