Gaia Data Release 3: The Galaxy in your preferred colours. Synthetic photometry from Gaia low-resolution spectra

Gaia Data Release 3 provides novel flux-calibrated low-resolution spectrophotometry for about 220 million sources in the wavelength range 330nm - 1050nm (XP spectra). Synthetic photometry directly tied to a flux in physical units can be obtained from these spectra for any passband fully enclosed in...

Descripción completa

Detalles Bibliográficos
Autores: Gaia Collaboration, Antoja, T. (Teresa), Luri Carrascoso, Xavier, Jordi i Nebot, Carme, Carrasco, José Manuel (Carrasco Martínez), Monguió i Montells, Maria, Masana Fresno, Eduard, Castañeda Pons, Javier Bernardo, Romero Gómez, Mercè, Fabricius, Claus
Tipo de recurso: artículo
Estado:Versión publicada
Fecha de publicación:2022
País:España
Institución:Varias* (Consorci de Biblioteques Universitáries de Catalunya, Centre de Serveis Científics i Acadèmics de Catalunya)
Repositorio:Recercat. Dipósit de la Recerca de Catalunya
OAI Identifier:oai:recercat.cat:2445/215705
Acceso en línea:https://hdl.handle.net/2445/215705
Access Level:acceso abierto
Palabra clave:Estels
Fotometria
Astrometria
Stars
Photometry
Astrometry
id ES_5622ea0f8c8a4767d689bdca4d897c8d
oai_identifier_str oai:recercat.cat:2445/215705
network_acronym_str ES
network_name_str España
repository_id_str
spelling Gaia Data Release 3: The Galaxy in your preferred colours. Synthetic photometry from Gaia low-resolution spectraGaia CollaborationAntoja, T. (Teresa)Luri Carrascoso, XavierJordi i Nebot, CarmeCarrasco, José Manuel (Carrasco Martínez)Monguió i Montells, MariaMasana Fresno, EduardCastañeda Pons, Javier BernardoRomero Gómez, MercèFabricius, ClausEstelsFotometriaAstrometriaStarsPhotometryAstrometryGaia Data Release 3 provides novel flux-calibrated low-resolution spectrophotometry for about 220 million sources in the wavelength range 330nm - 1050nm (XP spectra). Synthetic photometry directly tied to a flux in physical units can be obtained from these spectra for any passband fully enclosed in this wavelength range. We describe how synthetic photometry can be obtained from XP spectra, illustrating the performance that can be achieved under a range of different conditions - for example passband width and wavelength range - as well as the limits and the problems affecting it. Existing top-quality photometry can be reproduced within a few per cent over a wide range of magnitudes and colour, for wide and medium bands, and with up to millimag accuracy when synthetic photometry is standardised with respect to these external sources. Some examples of potential scientific application are presented, including the detection of multiple populations in globular clusters, the estimation of metallicity extended to the very metal-poor regime, and the classification of white dwarfs. A catalogue providing standardised photometry for ~220 million sources in several wide bands of widely used photometric systems is provided (Gaia Synthetic Photometry Catalogue; GSPC) as well as a catalogue of ≃105 white dwarfs with DA/non-DA classification obtained with a Random Forest algorithm (Gaia Synthetic Photometry Catalogue for White Dwarfs; GSPC-WD).EDP Sciences2024202420222024info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersion59 p.application/pdfhttps://hdl.handle.net/2445/215705Articles publicats en revistes (Física Quàntica i Astrofísica)reponame:Recercat. Dipósit de la Recerca de Catalunyainstname:Varias* (Consorci de Biblioteques Universitáries de Catalunya, Centre de Serveis Científics i Acadèmics de Catalunya)InglésReproducció del document publicat a: https://doi.org/10.1051/0004-6361/202243709Astronomy & Astrophysics, 2022, p. 1-59https://doi.org/10.1051/0004-6361/202243709(c) The European Southern Observatory (ESO), 2022info:eu-repo/semantics/openAccessoai:recercat.cat:2445/2157052026-05-29T05:05:01Z
dc.title.none.fl_str_mv Gaia Data Release 3: The Galaxy in your preferred colours. Synthetic photometry from Gaia low-resolution spectra
title Gaia Data Release 3: The Galaxy in your preferred colours. Synthetic photometry from Gaia low-resolution spectra
spellingShingle Gaia Data Release 3: The Galaxy in your preferred colours. Synthetic photometry from Gaia low-resolution spectra
Gaia Collaboration
Estels
Fotometria
Astrometria
Stars
Photometry
Astrometry
title_short Gaia Data Release 3: The Galaxy in your preferred colours. Synthetic photometry from Gaia low-resolution spectra
title_full Gaia Data Release 3: The Galaxy in your preferred colours. Synthetic photometry from Gaia low-resolution spectra
title_fullStr Gaia Data Release 3: The Galaxy in your preferred colours. Synthetic photometry from Gaia low-resolution spectra
title_full_unstemmed Gaia Data Release 3: The Galaxy in your preferred colours. Synthetic photometry from Gaia low-resolution spectra
title_sort Gaia Data Release 3: The Galaxy in your preferred colours. Synthetic photometry from Gaia low-resolution spectra
dc.creator.none.fl_str_mv Gaia Collaboration
Antoja, T. (Teresa)
Luri Carrascoso, Xavier
Jordi i Nebot, Carme
Carrasco, José Manuel (Carrasco Martínez)
Monguió i Montells, Maria
Masana Fresno, Eduard
Castañeda Pons, Javier Bernardo
Romero Gómez, Mercè
Fabricius, Claus
author Gaia Collaboration
author_facet Gaia Collaboration
Antoja, T. (Teresa)
Luri Carrascoso, Xavier
Jordi i Nebot, Carme
Carrasco, José Manuel (Carrasco Martínez)
Monguió i Montells, Maria
Masana Fresno, Eduard
Castañeda Pons, Javier Bernardo
Romero Gómez, Mercè
Fabricius, Claus
author_role author
author2 Antoja, T. (Teresa)
Luri Carrascoso, Xavier
Jordi i Nebot, Carme
Carrasco, José Manuel (Carrasco Martínez)
Monguió i Montells, Maria
Masana Fresno, Eduard
Castañeda Pons, Javier Bernardo
Romero Gómez, Mercè
Fabricius, Claus
author2_role author
author
author
author
author
author
author
author
author
dc.subject.none.fl_str_mv Estels
Fotometria
Astrometria
Stars
Photometry
Astrometry
topic Estels
Fotometria
Astrometria
Stars
Photometry
Astrometry
description Gaia Data Release 3 provides novel flux-calibrated low-resolution spectrophotometry for about 220 million sources in the wavelength range 330nm - 1050nm (XP spectra). Synthetic photometry directly tied to a flux in physical units can be obtained from these spectra for any passband fully enclosed in this wavelength range. We describe how synthetic photometry can be obtained from XP spectra, illustrating the performance that can be achieved under a range of different conditions - for example passband width and wavelength range - as well as the limits and the problems affecting it. Existing top-quality photometry can be reproduced within a few per cent over a wide range of magnitudes and colour, for wide and medium bands, and with up to millimag accuracy when synthetic photometry is standardised with respect to these external sources. Some examples of potential scientific application are presented, including the detection of multiple populations in globular clusters, the estimation of metallicity extended to the very metal-poor regime, and the classification of white dwarfs. A catalogue providing standardised photometry for ~220 million sources in several wide bands of widely used photometric systems is provided (Gaia Synthetic Photometry Catalogue; GSPC) as well as a catalogue of ≃105 white dwarfs with DA/non-DA classification obtained with a Random Forest algorithm (Gaia Synthetic Photometry Catalogue for White Dwarfs; GSPC-WD).
publishDate 2022
dc.date.none.fl_str_mv 2022
2024
2024
2024
dc.type.none.fl_str_mv info:eu-repo/semantics/article
info:eu-repo/semantics/publishedVersion
format article
status_str publishedVersion
dc.identifier.none.fl_str_mv https://hdl.handle.net/2445/215705
url https://hdl.handle.net/2445/215705
dc.language.none.fl_str_mv Inglés
language_invalid_str_mv Inglés
dc.relation.none.fl_str_mv Reproducció del document publicat a: https://doi.org/10.1051/0004-6361/202243709
Astronomy & Astrophysics, 2022, p. 1-59
https://doi.org/10.1051/0004-6361/202243709
dc.rights.none.fl_str_mv (c) The European Southern Observatory (ESO), 2022
info:eu-repo/semantics/openAccess
rights_invalid_str_mv (c) The European Southern Observatory (ESO), 2022
eu_rights_str_mv openAccess
dc.format.none.fl_str_mv 59 p.
application/pdf
dc.publisher.none.fl_str_mv EDP Sciences
publisher.none.fl_str_mv EDP Sciences
dc.source.none.fl_str_mv Articles publicats en revistes (Física Quàntica i Astrofísica)
reponame:Recercat. Dipósit de la Recerca de Catalunya
instname:Varias* (Consorci de Biblioteques Universitáries de Catalunya, Centre de Serveis Científics i Acadèmics de Catalunya)
instname_str Varias* (Consorci de Biblioteques Universitáries de Catalunya, Centre de Serveis Científics i Acadèmics de Catalunya)
reponame_str Recercat. Dipósit de la Recerca de Catalunya
collection Recercat. Dipósit de la Recerca de Catalunya
repository.name.fl_str_mv
repository.mail.fl_str_mv
_version_ 1869408358237208576
score 15.811543