Galaxy And Mass Assembly (GAMA): Spectroscopic analysis

The Galaxy And Mass Assembly (GAMA) survey is a multiwavelength photometric and spectroscopic survey, using the AAOmega spectrograph on the Anglo-Australian Telescope to obtain spectra for up to ~300000 galaxies over 280 square degrees, to a limiting magnitude of r_pet < 19.8 mag. The target gala...

Full description

Saved in:
Bibliographic Details
Published in:arXiv.org 2013-01
Main Authors: Hopkins, A M, Driver, S P, Brough, S, Owers, M S, Bauer, A E, Gunawardhana, M L P, Cluver, M E, Colless, M, Foster, C, Lara-Lopez, M A, Roseboom, I, Sharp, R, Steele, O, Thomas, D, Baldry, I K, Brown, M J I, Liske, J, Norberg, P, Robotham, A S G, Bamford, S, Bland-Hawthorn, J, Drinkwater, M J, Loveday, J, Meyer, M, Peacock, J A, Tuffs, R, Agius, N, Alpaslan, M, Andrae, E, Cameron, E, Cole, S, Ching, J H Y, Christodoulou, L, Conselice, C, Croom, S, Cross, N J G, De Propris, R, Delhaize, J, Dunne, L, Eales, S, Ellis, S, Frenk, C S, Graham, A, Grootes, M W, Haussler, B, Heymans, C, Hill, D, Hoyle, B, Hudson, M, Jarvis, M, Johansson, J, Jones, D H, E van Kampen, Kelvin, L, Kuijken, K, Lopez-Sanchez, A, Maddox, S, Madore, B, Maraston, C, McNaught-Roberts, T, Nichol, R C, Oliver, S, Parkinson, H, Penny, S, Phillipps, S, Pimbblet, K A, Ponman, T, Popescu, C C, Prescott, M, Proctor, R, Sadler, E M, Sansom, A E, Seibert, M, Staveley-Smith, L, Sutherland, W, Taylor, E, L Van Waerbeke, Vazquez-Mata, J A, Warren, S, Wijesinghe, D B, Wild, V, Wilkins, S
Format: Article
Language:English
Subjects:
Assembly
Dependence
Diagnostic systems
Galaxies
Galaxy distribution
Luminosity
Photometry
Quality control
Quasars
Red shift
Reliability analysis
Robust control
Spectra
Spectroscopic analysis
Star formation
Stars & galaxies
Online Access:Get full text
Tags: Add Tag
No Tags, Be the first to tag this record!
Description
Summary:The Galaxy And Mass Assembly (GAMA) survey is a multiwavelength photometric and spectroscopic survey, using the AAOmega spectrograph on the Anglo-Australian Telescope to obtain spectra for up to ~300000 galaxies over 280 square degrees, to a limiting magnitude of r_pet < 19.8 mag. The target galaxies are distributed over 0
ISSN:2331-8422
DOI:10.48550/arxiv.1301.7127