VICS82: The VISTA-CFHT Stripe 82 Near-infrared Survey

Autores
Geach, J. E.; Lin, Y. -T.; Makler, M.; Kneib, Jean Paul; Ross, N. P.; Wang, W.-H.; Hsieh, B.-C.; Leauthaud, A.; Bundy, K.; McCracken, H.J.; Comparat, J.; Caminha, G. B.; Hudelot, P.; Lin, L.; Waerbeke, L. Van; Pereira, M. E. S.; Mast, Damian
Año de publicación
2017
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
We present the VISTA-CFHT Stripe 82 (VICS82) survey: a near-infrared (J+K s ) survey covering 150 square degrees of the Sloan Digital Sky Survey (SDSS) equatorial Stripe 82 to an average depth of J = 21.9 AB mag and K s = 21.4 AB mag (80% completeness limits; 5σ point-source depths are approximately 0.5 mag brighter). VICS82 contributes to the growing legacy of multiwavelength data in the Stripe 82 footprint. The addition of near-infrared photometry to the existing SDSS Stripe 82 coadd ugriz photometry reduces the scatter in stellar mass estimates to σ log(M ∗ ) ≈ 0.3 dex for galaxies with M ∗ > 10 9 M ⊙ at z ≈ 0.5, and offers improvement compared to optical-only estimates out to z ≈ 1, with stellar masses constrained within a factor of approximately 2.5. When combined with other multiwavelength imaging of the Stripe, including moderate-to-deep ultraviolet (GALEX), optical and mid-infrared (Spitzer-IRAC) coverage, as well as tens of thousands of spectroscopic redshifts, VICS82 gives access to approximately 0.5 Gpc 3 of comoving volume. Some of the main science drivers of VICS82 include (a) measuring the stellar mass function of L ∗ galaxies out to z ∼ 1; (b) detecting intermediate-redshift quasars at 2 ≲ z ≲ 3.5;(c) measuring the stellar mass function and baryon census of clusters of galaxies, and (d) performing cross-correlation experiments of cosmic microwave background lensing in the optical/near-infrared that link stellar mass to large-scale dark matter structure. Here we define and describe the survey, highlight some early science results, and present the first public data release, which includes an SDSS-matched catalog as well as the calibrated pixel data themselves.
Fil: Geach, J. E.. University Of Hertfordshire; Reino Unido
Fil: Lin, Y. -T.. Institute Of Astrophysics And Astronomy, Academia Sinica Taiwan; China
Fil: Makler, M.. Centro Brasileiro de Pesquisas Físicas; Brasil
Fil: Kneib, Jean Paul. Ecole Polytechnique Federale de Lausanne; Suiza. Laboratoire D'astrophysique de Marseille; Francia
Fil: Ross, N. P.. University of Edinburgh; Reino Unido
Fil: Wang, W.-H.. Institute Of Astrophysics And Astronomy, Academia Sinica Taiwan; China
Fil: Hsieh, B.-C.. Institute Of Astrophysics And Astronomy, Academia Sinica Taiwan; China
Fil: Leauthaud, A.. University Of California; Estados Unidos
Fil: Bundy, K.. University Of California; Estados Unidos
Fil: McCracken, H.J.. Institut D 'astrophysique de Paris; Francia
Fil: Comparat, J.. Universidad Autónoma de Madrid; España
Fil: Caminha, G. B.. Università di Ferrara; Italia
Fil: Hudelot, P.. Institut D 'astrophysique de Paris; Francia
Fil: Lin, L.. Institute Of Astrophysics And Astronomy, Academia Sinica Taiwan; China
Fil: Waerbeke, L. Van. University of British Columbia; Canadá
Fil: Pereira, M. E. S.. Centro Brasileiro de Pesquisas Físicas; Brasil
Fil: Mast, Damian. Centro Brasileiro de Pesquisas Físicas; Brasil. Observatorio Astronómico de Córdoba; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba; Argentina
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acceso abierto
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https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
Repositorio
CONICET Digital (CONICET)
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Consejo Nacional de Investigaciones Científicas y Técnicas
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oai:ri.conicet.gov.ar:11336/76270
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spelling VICS82: The VISTA-CFHT Stripe 82 Near-infrared SurveyGeach, J. E.Lin, Y. -T.Makler, M.Kneib, Jean PaulRoss, N. P.Wang, W.-H.Hsieh, B.-C.Leauthaud, A.Bundy, K.McCracken, H.J.Comparat, J.Caminha, G. B.Hudelot, P.Lin, L.Waerbeke, L. VanPereira, M. E. S.Mast, DamianCATALOGSINFRARED: GENERALSURVEYShttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1We present the VISTA-CFHT Stripe 82 (VICS82) survey: a near-infrared (J+K s ) survey covering 150 square degrees of the Sloan Digital Sky Survey (SDSS) equatorial Stripe 82 to an average depth of J = 21.9 AB mag and K s = 21.4 AB mag (80% completeness limits; 5σ point-source depths are approximately 0.5 mag brighter). VICS82 contributes to the growing legacy of multiwavelength data in the Stripe 82 footprint. The addition of near-infrared photometry to the existing SDSS Stripe 82 coadd ugriz photometry reduces the scatter in stellar mass estimates to σ log(M ∗ ) ≈ 0.3 dex for galaxies with M ∗ > 10 9 M ⊙ at z ≈ 0.5, and offers improvement compared to optical-only estimates out to z ≈ 1, with stellar masses constrained within a factor of approximately 2.5. When combined with other multiwavelength imaging of the Stripe, including moderate-to-deep ultraviolet (GALEX), optical and mid-infrared (Spitzer-IRAC) coverage, as well as tens of thousands of spectroscopic redshifts, VICS82 gives access to approximately 0.5 Gpc 3 of comoving volume. Some of the main science drivers of VICS82 include (a) measuring the stellar mass function of L ∗ galaxies out to z ∼ 1; (b) detecting intermediate-redshift quasars at 2 ≲ z ≲ 3.5;(c) measuring the stellar mass function and baryon census of clusters of galaxies, and (d) performing cross-correlation experiments of cosmic microwave background lensing in the optical/near-infrared that link stellar mass to large-scale dark matter structure. Here we define and describe the survey, highlight some early science results, and present the first public data release, which includes an SDSS-matched catalog as well as the calibrated pixel data themselves.Fil: Geach, J. E.. University Of Hertfordshire; Reino UnidoFil: Lin, Y. -T.. Institute Of Astrophysics And Astronomy, Academia Sinica Taiwan; ChinaFil: Makler, M.. Centro Brasileiro de Pesquisas Físicas; BrasilFil: Kneib, Jean Paul. Ecole Polytechnique Federale de Lausanne; Suiza. Laboratoire D'astrophysique de Marseille; FranciaFil: Ross, N. P.. University of Edinburgh; Reino UnidoFil: Wang, W.-H.. Institute Of Astrophysics And Astronomy, Academia Sinica Taiwan; ChinaFil: Hsieh, B.-C.. Institute Of Astrophysics And Astronomy, Academia Sinica Taiwan; ChinaFil: Leauthaud, A.. University Of California; Estados UnidosFil: Bundy, K.. University Of California; Estados UnidosFil: McCracken, H.J.. Institut D 'astrophysique de Paris; FranciaFil: Comparat, J.. Universidad Autónoma de Madrid; EspañaFil: Caminha, G. B.. Università di Ferrara; ItaliaFil: Hudelot, P.. Institut D 'astrophysique de Paris; FranciaFil: Lin, L.. Institute Of Astrophysics And Astronomy, Academia Sinica Taiwan; ChinaFil: Waerbeke, L. Van. University of British Columbia; CanadáFil: Pereira, M. E. S.. Centro Brasileiro de Pesquisas Físicas; BrasilFil: Mast, Damian. Centro Brasileiro de Pesquisas Físicas; Brasil. Observatorio Astronómico de Córdoba; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba; ArgentinaIOP Publishing2017-07info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/76270Geach, J. E.; Lin, Y. -T.; Makler, M.; Kneib, Jean Paul; Ross, N. P.; et al.; VICS82: The VISTA-CFHT Stripe 82 Near-infrared Survey; IOP Publishing; Astrophysical Journal Supplement Series; 231; 1; 7-20170067-00491538-4365CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/doi/10.3847/1538-4365/aa74b6info:eu-repo/semantics/altIdentifier/url/https://iopscience.iop.org/article/10.3847/1538-4365/aa74b6/metainfo:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T10:06:10Zoai:ri.conicet.gov.ar:11336/76270instacron:CONICETInstitucionalhttp://ri.conicet.gov.ar/Organismo científico-tecnológicoNo correspondehttp://ri.conicet.gov.ar/oai/requestdasensio@conicet.gov.ar; lcarlino@conicet.gov.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:34982025-09-29 10:06:10.649CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv VICS82: The VISTA-CFHT Stripe 82 Near-infrared Survey
title VICS82: The VISTA-CFHT Stripe 82 Near-infrared Survey
spellingShingle VICS82: The VISTA-CFHT Stripe 82 Near-infrared Survey
Geach, J. E.
CATALOGS
INFRARED: GENERAL
SURVEYS
title_short VICS82: The VISTA-CFHT Stripe 82 Near-infrared Survey
title_full VICS82: The VISTA-CFHT Stripe 82 Near-infrared Survey
title_fullStr VICS82: The VISTA-CFHT Stripe 82 Near-infrared Survey
title_full_unstemmed VICS82: The VISTA-CFHT Stripe 82 Near-infrared Survey
title_sort VICS82: The VISTA-CFHT Stripe 82 Near-infrared Survey
dc.creator.none.fl_str_mv Geach, J. E.
Lin, Y. -T.
Makler, M.
Kneib, Jean Paul
Ross, N. P.
Wang, W.-H.
Hsieh, B.-C.
Leauthaud, A.
Bundy, K.
McCracken, H.J.
Comparat, J.
Caminha, G. B.
Hudelot, P.
Lin, L.
Waerbeke, L. Van
Pereira, M. E. S.
Mast, Damian
author Geach, J. E.
author_facet Geach, J. E.
Lin, Y. -T.
Makler, M.
Kneib, Jean Paul
Ross, N. P.
Wang, W.-H.
Hsieh, B.-C.
Leauthaud, A.
Bundy, K.
McCracken, H.J.
Comparat, J.
Caminha, G. B.
Hudelot, P.
Lin, L.
Waerbeke, L. Van
Pereira, M. E. S.
Mast, Damian
author_role author
author2 Lin, Y. -T.
Makler, M.
Kneib, Jean Paul
Ross, N. P.
Wang, W.-H.
Hsieh, B.-C.
Leauthaud, A.
Bundy, K.
McCracken, H.J.
Comparat, J.
Caminha, G. B.
Hudelot, P.
Lin, L.
Waerbeke, L. Van
Pereira, M. E. S.
Mast, Damian
author2_role author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
dc.subject.none.fl_str_mv CATALOGS
INFRARED: GENERAL
SURVEYS
topic CATALOGS
INFRARED: GENERAL
SURVEYS
purl_subject.fl_str_mv https://purl.org/becyt/ford/1.3
https://purl.org/becyt/ford/1
dc.description.none.fl_txt_mv We present the VISTA-CFHT Stripe 82 (VICS82) survey: a near-infrared (J+K s ) survey covering 150 square degrees of the Sloan Digital Sky Survey (SDSS) equatorial Stripe 82 to an average depth of J = 21.9 AB mag and K s = 21.4 AB mag (80% completeness limits; 5σ point-source depths are approximately 0.5 mag brighter). VICS82 contributes to the growing legacy of multiwavelength data in the Stripe 82 footprint. The addition of near-infrared photometry to the existing SDSS Stripe 82 coadd ugriz photometry reduces the scatter in stellar mass estimates to σ log(M ∗ ) ≈ 0.3 dex for galaxies with M ∗ > 10 9 M ⊙ at z ≈ 0.5, and offers improvement compared to optical-only estimates out to z ≈ 1, with stellar masses constrained within a factor of approximately 2.5. When combined with other multiwavelength imaging of the Stripe, including moderate-to-deep ultraviolet (GALEX), optical and mid-infrared (Spitzer-IRAC) coverage, as well as tens of thousands of spectroscopic redshifts, VICS82 gives access to approximately 0.5 Gpc 3 of comoving volume. Some of the main science drivers of VICS82 include (a) measuring the stellar mass function of L ∗ galaxies out to z ∼ 1; (b) detecting intermediate-redshift quasars at 2 ≲ z ≲ 3.5;(c) measuring the stellar mass function and baryon census of clusters of galaxies, and (d) performing cross-correlation experiments of cosmic microwave background lensing in the optical/near-infrared that link stellar mass to large-scale dark matter structure. Here we define and describe the survey, highlight some early science results, and present the first public data release, which includes an SDSS-matched catalog as well as the calibrated pixel data themselves.
Fil: Geach, J. E.. University Of Hertfordshire; Reino Unido
Fil: Lin, Y. -T.. Institute Of Astrophysics And Astronomy, Academia Sinica Taiwan; China
Fil: Makler, M.. Centro Brasileiro de Pesquisas Físicas; Brasil
Fil: Kneib, Jean Paul. Ecole Polytechnique Federale de Lausanne; Suiza. Laboratoire D'astrophysique de Marseille; Francia
Fil: Ross, N. P.. University of Edinburgh; Reino Unido
Fil: Wang, W.-H.. Institute Of Astrophysics And Astronomy, Academia Sinica Taiwan; China
Fil: Hsieh, B.-C.. Institute Of Astrophysics And Astronomy, Academia Sinica Taiwan; China
Fil: Leauthaud, A.. University Of California; Estados Unidos
Fil: Bundy, K.. University Of California; Estados Unidos
Fil: McCracken, H.J.. Institut D 'astrophysique de Paris; Francia
Fil: Comparat, J.. Universidad Autónoma de Madrid; España
Fil: Caminha, G. B.. Università di Ferrara; Italia
Fil: Hudelot, P.. Institut D 'astrophysique de Paris; Francia
Fil: Lin, L.. Institute Of Astrophysics And Astronomy, Academia Sinica Taiwan; China
Fil: Waerbeke, L. Van. University of British Columbia; Canadá
Fil: Pereira, M. E. S.. Centro Brasileiro de Pesquisas Físicas; Brasil
Fil: Mast, Damian. Centro Brasileiro de Pesquisas Físicas; Brasil. Observatorio Astronómico de Córdoba; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba; Argentina
description We present the VISTA-CFHT Stripe 82 (VICS82) survey: a near-infrared (J+K s ) survey covering 150 square degrees of the Sloan Digital Sky Survey (SDSS) equatorial Stripe 82 to an average depth of J = 21.9 AB mag and K s = 21.4 AB mag (80% completeness limits; 5σ point-source depths are approximately 0.5 mag brighter). VICS82 contributes to the growing legacy of multiwavelength data in the Stripe 82 footprint. The addition of near-infrared photometry to the existing SDSS Stripe 82 coadd ugriz photometry reduces the scatter in stellar mass estimates to σ log(M ∗ ) ≈ 0.3 dex for galaxies with M ∗ > 10 9 M ⊙ at z ≈ 0.5, and offers improvement compared to optical-only estimates out to z ≈ 1, with stellar masses constrained within a factor of approximately 2.5. When combined with other multiwavelength imaging of the Stripe, including moderate-to-deep ultraviolet (GALEX), optical and mid-infrared (Spitzer-IRAC) coverage, as well as tens of thousands of spectroscopic redshifts, VICS82 gives access to approximately 0.5 Gpc 3 of comoving volume. Some of the main science drivers of VICS82 include (a) measuring the stellar mass function of L ∗ galaxies out to z ∼ 1; (b) detecting intermediate-redshift quasars at 2 ≲ z ≲ 3.5;(c) measuring the stellar mass function and baryon census of clusters of galaxies, and (d) performing cross-correlation experiments of cosmic microwave background lensing in the optical/near-infrared that link stellar mass to large-scale dark matter structure. Here we define and describe the survey, highlight some early science results, and present the first public data release, which includes an SDSS-matched catalog as well as the calibrated pixel data themselves.
publishDate 2017
dc.date.none.fl_str_mv 2017-07
dc.type.none.fl_str_mv info:eu-repo/semantics/article
info:eu-repo/semantics/publishedVersion
http://purl.org/coar/resource_type/c_6501
info:ar-repo/semantics/articulo
format article
status_str publishedVersion
dc.identifier.none.fl_str_mv http://hdl.handle.net/11336/76270
Geach, J. E.; Lin, Y. -T.; Makler, M.; Kneib, Jean Paul; Ross, N. P.; et al.; VICS82: The VISTA-CFHT Stripe 82 Near-infrared Survey; IOP Publishing; Astrophysical Journal Supplement Series; 231; 1; 7-2017
0067-0049
1538-4365
CONICET Digital
CONICET
url http://hdl.handle.net/11336/76270
identifier_str_mv Geach, J. E.; Lin, Y. -T.; Makler, M.; Kneib, Jean Paul; Ross, N. P.; et al.; VICS82: The VISTA-CFHT Stripe 82 Near-infrared Survey; IOP Publishing; Astrophysical Journal Supplement Series; 231; 1; 7-2017
0067-0049
1538-4365
CONICET Digital
CONICET
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/doi/10.3847/1538-4365/aa74b6
info:eu-repo/semantics/altIdentifier/url/https://iopscience.iop.org/article/10.3847/1538-4365/aa74b6/meta
dc.rights.none.fl_str_mv info:eu-repo/semantics/openAccess
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
eu_rights_str_mv openAccess
rights_invalid_str_mv https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
dc.format.none.fl_str_mv application/pdf
application/pdf
dc.publisher.none.fl_str_mv IOP Publishing
publisher.none.fl_str_mv IOP Publishing
dc.source.none.fl_str_mv reponame:CONICET Digital (CONICET)
instname:Consejo Nacional de Investigaciones Científicas y Técnicas
reponame_str CONICET Digital (CONICET)
collection CONICET Digital (CONICET)
instname_str Consejo Nacional de Investigaciones Científicas y Técnicas
repository.name.fl_str_mv CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicas
repository.mail.fl_str_mv dasensio@conicet.gov.ar; lcarlino@conicet.gov.ar
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score 13.070432

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