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| 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
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.
| 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 |
| 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 |
| 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. |