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Galaxy And Mass Assembly (GAMA): spectroscopic analysis

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-López, 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, Alister W.; Grootes, M. W.; Häußler, B.; Heymans, C.; Hill, D.; Hoyle, B.; Hudson, M.; Jarvis, M.; Johansson, J.; Jones, D. H.; van Kampen, E.; Kelvin, L.; Kuijken, K.; López-Sánchez, Á.; 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...

Authors

A. M. Hopkins

S. P. Driver

S. Brough

M. S. Owers

A. E. Bauer

M. L. P. Gunawardhana

M. E. Cluver

M. Colless

C. Foster

M. A. Lara-López

I. Roseboom

R. Sharp

O. Steele

D. Thomas

I. K. Baldry

M. J. I. Brown

J. Liske

P. Norberg

A. S. G. Robotham

S. Bamford

J. Bland-Hawthorn

M. J. Drinkwater

J. Loveday

M. Meyer

J. A. Peacock

R. Tuffs

N. Agius

M. Alpaslan

E. Andrae

E. Cameron

S. Cole

J. H. Y. Ching

L. Christodoulou

C. Conselice

S. Croom

N. J. G. Cross

R. De Propris

J. Delhaize

L. Dunne

S. Eales

S. Ellis

C. S. Frenk

Alister W. Graham

M. W. Grootes

B. Häußler

C. Heymans

D. Hill

B. Hoyle

M. Hudson

M. Jarvis

J. Johansson

D. H. Jones

E. van Kampen

L. Kelvin

K. Kuijken

Á. López-Sánchez

S. Maddox

B. Madore

C. Maraston

T. McNaught-Roberts

R. C. Nichol

S. Oliver

H. Parkinson

S. Penny

S. Phillipps

T. Ponman

C. C. Popescu

M. Prescott

R. Proctor

E. M. Sadler

A. E. Sansom

M. Seibert

L. Staveley-Smith

W. Sutherland

E. Taylor

L. Van Waerbeke

J. A. Vázquez-Mata

S. Warren

D. B. Wijesinghe

V. Wild

S. Wilkins



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 < z ≲ 0.5 with a median redshift of z ≈ 0.2, although the redshift distribution includes a small number of systems, primarily quasars, at higher redshifts, up to and beyond z = 1. The redshift accuracy ranges from σ v ≈ 50 km s-1 to σ v ≈ 100 km s-1 depending on the signal-to-noise ratio of the spectrum. Here we describe the GAMA spectroscopic reduction and analysis pipeline. We present the steps involved in taking the raw two-dimensional spectroscopic images through to flux-calibrated one-dimensional spectra. The resulting GAMA spectra cover an observed wavelength range of 3750 λ 8850Å at a resolution of R ≈ 1300. The final flux calibration is typically accurate to 10-20 per cent, although the reliability is worse at the extreme wavelength ends, and poorer in the blue than the red. We present details of the measurement of emission and absorption features in the GAMA spectra. These measurements are characterized through a variety of quality control analyses detailing the robustness and reliability of the measurements. We illustrate the quality of the measurements with a brief exploration of elementary emission line properties of the galaxies in the GAMA sample. We demonstrate the luminosity dependence of the Balmer decrement, consistent with previously published results, and explore further how Balmer decrement varies with galaxy mass and redshift. We also investigate the mass and redshift dependencies of the [NII] /Hα versus [OIII]/Hβ spectral diagnostic diagram, commonly used to discriminate between star forming and nuclear activity in galaxies. © 2013 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society.

Citation

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-López, 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., …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

Journal Article Type Article
Acceptance Date Jan 4, 2013
Online Publication Date Feb 7, 2013
Publication Date Apr 11, 2013
Deposit Date Aug 2, 2018
Publicly Available Date Aug 14, 2018
Journal Monthly Notices of the Royal Astronomical Society
Print ISSN 0035-8711
Electronic ISSN 1365-2966
Publisher Oxford University Press
Peer Reviewed Peer Reviewed
Volume 430
Issue 3
Pages 2047-2066
DOI https://doi.org/10.1093/mnras/stt030
Keywords Galaxies: evolution; Galaxies: formation; Galaxies: general
Public URL https://hull-repository.worktribe.com/output/591041
Publisher URL https://academic.oup.com/mnras/article/430/3/2047/980679
Contract Date Aug 2, 2018

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Copyright Statement
© 2013 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society






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