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The ASTRODEEP-GS43 catalogue: New photometry and redshifts for the CANDELS GOODS-South field
Indexado
WoS WOS:000655028000003
Scopus SCOPUS_ID:85105393581
DOI 10.1051/0004-6361/202140310
Año 2021
Tipo artículo de investigación

Citas Totales

Autores Afiliación Chile

Instituciones Chile

% Participación
Internacional

Autores
Afiliación Extranjera

Instituciones
Extranjeras


Abstract



Context. We present ASTRODEEP-GS43, a new multi-wavelength photometric catalogue of the GOODS-South field, which builds and improves upon the previously released CANDELS catalogue.Aims. We provide photometric fluxes and corresponding uncertainties in 43 optical and infrared bands (25 wide and 18 medium filters), as well as the photometric redshifts and physical properties of the 34930 CANDELS H-detected objects, plus an additional sample of 178 H-dropout sources, of which 173 are Ks-detected and five are IRAC-detected.Methods. We keep the CANDELS photometry in seven bands (CTIO U, Hubble Space Telescope WFC3, and ISAAC-K) and measure from scratch the fluxes in the other 36 (23 from Subaru SuprimeCAM and Magellan Baade FourStar and the rest from VIMOS, HST ACS, HAWK-I Ks, and Spitzer IRAC) with state-of-the-art template-fitting techniques. We then compute new photometric redshifts with three different software tools and take the median value as a best estimate. We finally evaluate new physical parameters from spectral energy distribution (SED) fitting, comparing them to previously published ones.Results. Comparing to a sample of 3931 high quality spectroscopic redshifts, for the new photometric redshifts we obtain a normalised median absolute deviation of 0.015, with 3.01% of outliers on the full catalogue (0.011 and 0.22% on the bright end at I814< 22.5). This is similar to the best available published samples of photometric redshifts, such as the COSMOS UltraVISTA catalogue.Conclusions. The ASTRODEEP-GS43 results are in qualitative agreement with previously published catalogues of the GOODS-South field, improving on them particularly in terms of SED sampling and photometric redshift estimates. The catalogue is available for download from the ASTRODEEP website.

Revista



Revista ISSN
Astronomy & Astrophysics 0004-6361

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Disciplinas de Investigación



WOS
Astronomy & Astrophysics
Scopus
Sin Disciplinas
SciELO
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Publicaciones WoS (Ediciones: ISSHP, ISTP, AHCI, SSCI, SCI), Scopus, SciELO Chile.

Colaboración Institucional



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Autores - Afiliación



Ord. Autor Género Institución - País
1 Merlin, Emiliano Hombre Istituto Nazionale di Astrofisica - Italia
Istituto Nazionale Di Astrofisica, Rome - Italia
INAF OAR - Italia
2 Castellano, Marco Hombre Istituto Nazionale di Astrofisica - Italia
Istituto Nazionale Di Astrofisica, Rome - Italia
INAF OAR - Italia
3 Santini, Paola Mujer Istituto Nazionale di Astrofisica - Italia
Istituto Nazionale Di Astrofisica, Rome - Italia
INAF OAR - Italia
4 Cipolletta, G. - Istituto Nazionale di Astrofisica - Italia
Istituto Nazionale Di Astrofisica, Rome - Italia
INAF OAR - Italia
5 Boutsia, Konstantina Mujer Observatorio Las Campanas - Chile
Las Campanas Observatory - Chile
Carnegie Observ - Chile
6 Schreiber, Corentin Hombre UNIV OXFORD - Reino Unido
University of Oxford - Reino Unido
7 Buitrago, Fernando Hombre Univ Lisbon - Portugal
Universidade de Lisboa - Portugal
8 Fontana, A. Hombre Istituto Nazionale di Astrofisica - Italia
Istituto Nazionale Di Astrofisica, Rome - Italia
INAF OAR - Italia
9 Elbaz, David Hombre Univ Paris Diderot - Francia
Astrophysique, Instrumentation et Modélisation de Paris-Saclay - Francia
10 Dunlop, J. - UNIV EDINBURGH - Reino Unido
11 Grazian, A. Mujer Istituto Nazionale di Astrofisica - Italia
Osservatorio Astronomico di Padova - Italia
INAF Osservatorio Astron Padova - Italia
12 McLure, R. - UNIV EDINBURGH - Reino Unido
13 McLeod, Derek Hombre UNIV EDINBURGH - Reino Unido
University of Edinburgh, Institute for Astronomy - Reino Unido
14 Nonino, M. Hombre Istituto Nazionale di Astrofisica - Italia
Osservatorio Astronomico di Trieste - Italia
INAF Osservatorio Astron Trieste - Italia
15 Milvang-Jensen, B. - Univ Copenhagen - Dinamarca
Niels Bohr Institute - Dinamarca
Københavns Universitet - Dinamarca
16 Derriere, S. - Univ Strasbourg - Francia
Université de Strasbourg - Francia
17 Dole, H. - Space Telescope Sci Inst - Estados Unidos
Space Telescope Science Institute - Estados Unidos
18 Pentericci, Laura Mujer Istituto Nazionale di Astrofisica - Italia
Istituto Nazionale Di Astrofisica, Rome - Italia
INAF OAR - Italia
19 Fortuni, F. - Istituto Nazionale di Astrofisica - Italia
Istituto Nazionale Di Astrofisica, Rome - Italia
INAF OAR - Italia
20 Calabro, A. Hombre Istituto Nazionale di Astrofisica - Italia
Istituto Nazionale Di Astrofisica, Rome - Italia
INAF OAR - Italia

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Financiamiento



Fuente
Ministerio de Economía y Competitividad
European Commission
Seventh Framework Programme
Spanish MINECO
Danish National Research Foundation
EU
Danmarks Grundforskningsfond
Danmarks Frie Forskningsfond
Independent Research Fund Denmark grant
EU FP7SPACE

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Agradecimientos



Agradecimiento
Part of this study was funded using the EU FP7SPACE project ASTRODEEP (ref. no: 312725), supported by the European Commission. This work is partly based on tools and data products produced by GAZPAR operated by CeSAM-LAM and IAP. This research has made use of the SVO Filter Profile Service (http://svo2.cab.inta-csic.es/theory/fps/) supported from the Spanish MINECO through grant AYA2017-84089. The Cosmic Dawn Center is funded by the Danish National Research Foundation under grant no. 140. BMJ is supported in part by Independent Research Fund Denmark grant DFF - 7014-00017. The authors thank Tao Wang and Mengyuan Xiao for their contributions to the work.
Acknowledgements. Part of this study was funded using the EU FP7SPACE project ASTRODEEP (ref. no: 312725), supported by the European Commission. This work is partly based on tools and data products produced by GAZPAR operated by CeSAM-LAM and IAP. This research has made use of the SVO Filter Profile Service (http://svo2.cab.inta-csic.es/theory/fps/) supported from the Spanish MINECO through grant AYA2017-84089. The Cosmic Dawn Center is funded by the Danish National Research Foundation under grant no. 140. BMJ is supported in part by Independent Research Fund Denmark grant DFF – 7014-00017. The authors thank Tao Wang and Mengyuan Xiao for their contributions to the work.

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