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The ASTRODEEP Frontier Fields Catalogues: II - Photometric redshifts and rest-frame properties in Abell-2744 and MACS-J0416

Authors :
Castellano, M.
Amorín, R.
Merlin, E.
Fontana, A.
McLure, R. J.
Mármol-Queraltó, E.
Mortlock, A.
Parsa, S.
Dunlop, J. S.
Elbaz, D.
Balestra, I.
Boucaud, A.
Bourne, N.
Boutsia, K.
Brammer, G.
Bruce, V. A.
Buitrago, F.
Capak, P.
Cappelluti, N.
Ciesla, L.
Comastri, A.
Cullen, F.
Derriere, S.
Faber, S. M.
Giallongo, E.
Grazian, A.
Grillo, C.
Mercurio, A.
Michałowski, M. J.
Nonino, M.
Paris, D.
Pentericci, L.
Pilo, S.
Rosati, P.
Santini, P.
Schreiber, C.
Shu, X.
Wang, T.
Source :
A&A 590, A31 (2016)
Publication Year :
2016

Abstract

We present the first public release of photometric redshifts, galaxy rest-frame properties and associated magnification values in the cluster and parallel pointings of the first two Frontier Fields, Abell-2744 and MACS-J0416. We exploit a multi-wavelength catalogue ranging from HST to ground-based K and Spitzer IRAC which is specifically designed to enable detection and measurement of accurate fluxes in crowded cluster regions. The multi-band information is used to derive photometric redshifts and physical properties of sources detected either in the H-band image alone or from a stack of four WFC3 bands. To minimize systematics median photometric redshifts are assembled from six different approaches to photo-z estimates. Their reliability is assessed through a comparison with available spectroscopic samples. State of the art lensing models are used to derive magnification values on an object-by-object basis by taking into account sources positions and redshifts. We show that photometric redshifts reach a remarkable ~3-5% accuracy. After accounting for magnification the H band number counts are found in agreement at bright magnitudes with number counts from the CANDELS fields, while extending the presently available samples to galaxies intrinsically as faint as H160~32-33 thanks to strong gravitational lensing. The Frontier Fields allow to probe the galaxy stellar mass distribution at 0.5-1.5 dex lower masses, depending on magnification, with respect to extragalactic wide fields, including sources at Mstar~ 10^7-10^8 Msun at z>5. Similarly, they allow the detection of objects with intrinsic SFRs>1dex lower than in the CANDELS fields reaching 0.1-1 Msun/yr at z~6-10. [abridged]<br />Comment: 10 pages, 9 figures, accepted for publication on A&A. CDS images and catalogues interface at http://astrodeep.u-strasbg.fr/ff/ . Full catalogues available for download from the ASTRODEEP website at http://www.astrodeep.eu/frontier-fields/

Details

Database :
arXiv
Journal :
A&A 590, A31 (2016)
Publication Type :
Report
Accession number :
edsarx.1603.02461
Document Type :
Working Paper
Full Text :
https://doi.org/10.1051/0004-6361/201527514