Cookies

We use cookies to ensure that we give you the best experience on our website. By continuing to browse this repository, you give consent for essential cookies to be used. You can read more about our Privacy and Cookie Policy.


Durham Research Online
You are in:

New constraints on the faint end of the UV luminosity function at z ~ 7-8 using the gravitational lensing of the Hubble Frontier Fields cluster A2744.

Atek, H. and Richard, J. and Kneib, J.-P. and Jauzac, M. and Schaerer, D. and Clément, B. and Limousin, M. and Jullo, E. and Natarajan, P. and Egami, E. and Ebeling, H. (2015) 'New constraints on the faint end of the UV luminosity function at z ~ 7-8 using the gravitational lensing of the Hubble Frontier Fields cluster A2744.', Astrophysical journal., 800 (1). p. 18.

Abstract

Exploiting the power of gravitational lensing, the Hubble Frontier Fields (HFF) program aims at observing six massive galaxy clusters to explore the distant universe far beyond the limits of blank field surveys. Using the complete Hubble Space Telescope observations of the first HFF cluster A2744, we report the detection of 50 galaxy candidates at z ~ 7 and eight candidates at z ~ 8 in a total survey area of 0.96 arcmin2 in the source plane. Three of these galaxies are multiply imaged by the lensing cluster. Using an updated model of the mass distribution in the cluster we were able to calculate the magnification factor and the effective survey volume for each galaxy in order to compute the ultraviolet galaxy luminosity function (LF) at both redshifts 7 and 8. Our new measurements reliably extend the z ~ 7 UV LF down to an absolute magnitude of M UV ~ –15.5. We find a characteristic magnitude of $M^{\star }_{{\rm UV}} = -20.90^{+0.90}_{-0.73}$ mag and a faint-end slope $\alpha =-2.01^{+0.20}_{-0.28}$, close to previous determinations in blank fields. We show here for the first time that this slope remains steep down to very faint luminosities of 0.01 L sstarf. Although prone to large uncertainties, our results at z ~ 8 also seem to confirm a steep faint-end slope below 0.1 L sstarf. The HFF program is therefore providing an extremely efficient way to study the faintest galaxy populations at z > 7 that would otherwise be inaccessible with current instrumentation. The full sample of six galaxy clusters will provide even better constraints on the buildup of galaxies at early epochs and their contribution to cosmic reionization.

Item Type:Article
Keywords:Galaxies: evolution, Galaxies: high-redshift, Galaxies: luminosity function, mass function, Gravitational lensing: strong.
Full text:(VoR) Version of Record
Download PDF
(3013Kb)
Status:Peer-reviewed
Publisher Web site:http://dx.doi.org/10.1088/0004-637X/800/1/18
Publisher statement:© 2015. The American Astronomical Society. All rights reserved.
Date accepted:01 December 2014
Date deposited:06 November 2015
Date of first online publication:04 February 2015
Date first made open access:No date available

Save or Share this output

Export:
Export
Look up in GoogleScholar