A new method to measure evolution of the galaxy luminosity function

Dye, Simon and Eales, Stephen Anthony ORCID: https://orcid.org/0000-0002-7394-426X 2010. A new method to measure evolution of the galaxy luminosity function. Monthly Notices of the Royal Astronomical Society 405 (4) , pp. 2406-2418. 10.1111/j.1365-2966.2010.16623.x

Full text not available from this repository.

Abstract

We present a new efficient technique for measuring evolution of the galaxy luminosity function. The method reconstructs the evolution over the luminosity-redshift plane using any combination of three input data set types: (i) number counts, (ii) galaxy redshifts and (iii) integrated background flux measurements. The evolution is reconstructed in adaptively sized regions of the plane according to the input data as determined by a Bayesian formalism. We demonstrate the performance of the method using a range of different synthetic input data sets. We also make predictions of the accuracy with which forthcoming surveys conducted with Submillimetre Common-User Bolometer Array 2 and the Herschel Space Satellite will be able to measure evolution of the submillimetre luminosity function using the method.

Item Type:	Article
Date Type:	Publication
Status:	Published
Schools:	Schools > Physics and Astronomy
Subjects:	Q Science > QB Astronomy
Uncontrolled Keywords:	galaxies: evolution; methods: statistical
Publisher:	Wiley
ISSN:	0035-8711
Last Modified:	20 Oct 2022 09:20
URI:	https://orca.cardiff.ac.uk/id/eprint/31493

Citation Data

Cited 1 time in Scopus. View in Scopus. Powered By Scopus® Data

Actions (repository staff only)

Edit Item