Liske, J and Baldry, IK and Driver, SP and Tuffs, RJ and Alpaslan, M and Andrae, E and Brough, S and Cluver, ME and Grootes, MW and Gunawardhana, MLP and Kelvin, LS and Loveday, J and Robotham, ASG and Taylor, EN and Bamford, SP and Bland-Hawthorn, J and Brown, MJI and Drinkwater, MJ and Hopkins, AM and Meyer, MJ et al and Norberg, P and Peacock, JA and Agius, NK and Andrews, SK and Bauer, AE and Ching, JHY and Colless, M and Conselice, CJ and Croom, SM and Davies, LJM and Propris, RD and Dunne, L and Eardley, EM and Ellis, S and Foster, C and Frenk, CS and Häußler, B and Holwerda, BW and Howlett, C and Ibarra, H and Jarvis, MJ and Jones, DH and Kafle, PR and Lacey, CG and Lange, R and Lara-López, MA and López-Sánchez, ÁR and Maddox, S and Madore, BF and McNaught-Roberts, T and Moffett, AJ and Nichol, RC and Owers, MS and Palamara, D and Penny, SJ and Phillipps, S and Pimbblet, KA and Popescu, CC and Prescott, M and Proctor, R and Sadler, EM and Sansom, AE and Seibert, M and Sharp, R and Sutherland, W and Vázquez-Mata, JA and Kampen, EV and Wilkins, SM and Williams, R and Wright, AH (2015) Galaxy And Mass Assembly (GAMA): end of survey report and data release 2. Monthly Notices of the Royal Astronomical Society, 452 (2). pp. 2087-2126. ISSN 0035-8711
This is the latest version of this item.
1506.08222v1.pdf - Accepted Version
The Galaxy And Mass Assembly (GAMA) survey is one of the largest contemporary spectroscopic surveys of low-redshift galaxies. Covering an area of ~286 deg^2 (split among five survey regions) down to a limiting magnitude of r < 19.8 mag, we have collected spectra and reliable redshifts for 238,000 objects using the AAOmega spectrograph on the Anglo-Australian Telescope. In addition, we have assembled imaging data from a number of independent surveys in order to generate photometry spanning the wavelength range 1 nm - 1 m. Here we report on the recently completed spectroscopic survey and present a series of diagnostics to assess its final state and the quality of the redshift data. We also describe a number of survey aspects and procedures, or updates thereof, including changes to the input catalogue, redshifting and re-redshifting, and the derivation of ultraviolet, optical and near-infrared photometry. Finally, we present the second public release of GAMA data. In this release we provide input catalogue and targeting information, spectra, redshifts, ultraviolet, optical and near-infrared photometry, single-component S\'ersic fits, stellar masses, H$\alpha$-derived star formation rates, environment information, and group properties for all galaxies with r < 19.0 mag in two of our survey regions, and for all galaxies with r < 19.4 mag in a third region (72,225 objects in total). The database serving these data is available at http://www.gama-survey.org/.
|Additional Information:||This is a pre-copyedited, author-produced PDF of an article accepted for publication in Monthly Notices of the Royal Astronomical Society following peer review. The version of record MNRAS (September 11, 2015) 452(2): 2087-2126 is available online at: http://dx.doi.org/10.1093/mnras/stv1436|
|Uncontrolled Keywords:||0201 Astronomical And Space Sciences|
|Subjects:||Q Science > QB Astronomy|
|Divisions:||Astrophysics Research Institute|
|Publisher:||Oxford University Press|
|Date Deposited:||26 Oct 2015 14:06|
|Last Modified:||26 Oct 2015 14:06|
|DOI or Identification number:||10.1093/mnras/stv1436|
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Galaxy And Mass Assembly (GAMA): end of survey report and data release 2. (deposited 09 Jul 2015 09:14)
- Galaxy And Mass Assembly (GAMA): end of survey report and data release 2. (deposited 26 Oct 2015 14:06) [Currently Displayed]
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