Galaxy And Mass Assembly (GAMA) DR1 (Driver+, 2011)

S. P. Driver, D. T. Hill, L. S. Kelvin, A. S. G. Robotham, J. Liske, P. Norberg, I. K. Baldry, S. P. Bamford, A. M. Hopkins, J. Loveday, J. A. Peacock, E. Andrae, J. Bland-Hawthorn, S. Brough, M. J. I. Brown, E. Cameron, J. H. Y. Ching, M. Colless, C. J. Conselice, S. M. CroomN. J. G. Cross, R. de Propris, S. Dye, M. J. Drinkwater, S. Ellis, A. W. Graham, M. W. Grootes, M. Gunawardhana, D. H. Jones, E. van Kampen, C. Maraston, R. C. Nichol, H. R. Parkinson, S. Phillipps, K. Pimbblet, C. C. Popescu, M. Prescott, I. G. Roseboom, E. M. Sadler, A. E. Sansom, R. G. Sharp, D. J. B. Smith, E. Taylor, D. Thomas, R. J. Tuffs, D. Wijesinghe, L. Dunne, C. S. Frenk, M. J. Jarvis, B. F. Madore, M. J. Meyer, M. Seibert, L. Staveley-Smith, W. J. Sutherland, S. J. Warren

Research output: Contribution to journalArticlepeer-review

Abstract / Description of output

All GAMA 2dF pointings (tiles) were observed during dark or grey time with exposure times mostly ranging from 3000 to 5000s (in three to five exposures) depending on seeing and sky brightness. Observations were generally conducted at an hour angle of less than 2h (the median zenith distance of the observations is 35°) and with the Atmospheric Dispersion Corrector engaged. We used the 580V and 385R gratings with central wavelengths of 4800 and 7250Å in the blue and red arms, respectively, separated by a 5700Å dichroic. This set-up yielded a continuous wavelength coverage of 3720-8850Å at a resolution of ~3.5Å (in the blue channel) and ~5.5Å (in the red channel). (2 data files).
Original languageEnglish
Pages (from-to)30971
JournalVizieR On-line Data Catalog
Publication statusPublished - 1 Sept 2012


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