Galaxy And Mass Assembly (GAMA): Spectroscopic analysis

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Abstract

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 ~300 000 galaxies over 280 deg2, to a limiting magnitude of rpet < 19.8 mag. The target galaxies are distributed over 0

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Hopkins, A. M., Driver, S. P., Brough, S., Owers, M. S., Bauer, A. E., Gunawardhana, M. L. P., … Wilkins, S. (2013). Galaxy And Mass Assembly (GAMA): Spectroscopic analysis. Monthly Notices of the Royal Astronomical Society, 430(3), 2047–2066. https://doi.org/10.1093/mnras/stt030

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