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Oxford University Press (OUP), Monthly Notices of the Royal Astronomical Society, 3(441), p. 2440-2451

DOI: 10.1093/mnras/stu727

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Galaxy And Mass Assembly (GAMA): autoz spectral redshift measurements, confidence and errors

Journal article published in 2014 by I. K. Baldry, M. Alpaslan ORCID, A. E. Bauer, J. Bland-Hawthorn, S. Brough, M. E. Cluver, S. M. Croom, L. J. M. Davies, S. P. Driver ORCID, M. L. P. Gunawardhana, Benne W. Holwerda, A. M. Hopkins, L. S. Kelvin, J. Liske ORCID, A. R. Lopez-Sanchez and other authors.
This paper is made freely available by the publisher.
This paper is made freely available by the publisher.

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Abstract

The Galaxy And Mass Assembly (GAMA) survey has obtained spectra of over 230000 targets using the Anglo-Australian Telescope. To homogenise the redshift measurements and improve the reliability, a fully automatic redshift code was developed (autoz). The measurements were made using a cross-correlation method for both absorption-line and emission-line spectra. Large deviations in the high-pass filtered spectra are partially clipped in order to be robust against uncorrected artefacts and to reduce the weight given to single-line matches. A single figure of merit (FOM) was developed that puts all template matches onto a similar confidence scale. The redshift confidence as a function of the FOM was fitted with a tanh function using a maximum likelihood method applied to repeat observations of targets. The method could be adapted to provide robust automatic redshifts for other large galaxy redshift surveys. For the GAMA survey, there was a substantial improvement in the reliability of assigned redshifts and in the lowering of redshift uncertainties with a median velocity uncertainty of 33 km/s. ; Comment: 13 pages, 12 figures, accepted by MNRAS, IDL routines for the autoz code are available from http://www.astro.ljmu.ac.uk/~ikb/research/autoz_code/