The S-PLUS 12-band Photometry as a Powerful Tool for Discovery and Classification: Ten Cataclysmic Variables in a Proof-of-concept Study

Autores
Lopes de Oliveira, Raimundo; de Araújo, Amanda S.; Krabbe, Angela C.; Mendes de Oliveira, Claudia Lucia; Mukai, Koji; Gutierrez Soto, Luis Angel; Kanaan, Antonio; Eleutério, Romualdo; Borges Fernandes, Marcelo; Quispe-Huaynasi, Fredi; Schoenell, William; Ribeiro, Tiago
Año de publicación
2025
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
Multiband photometric surveys provide a straightforward way to discover and classify astrophysical objectssystematically, enabling the study of a large number of targets at relatively low cost. Here we introduce analternative approach to select accreting white dwarf (AWD) candidates following their spectral energy distribution,entirely supported by the twelve photometric bands of the Southern Photometric Local Universe Survey (S-PLUS).The method was validated with optical spectroscopic follow-up with the Gemini South telescope, whichunambiguously established ten systems as cataclysmic variables (CVs), alongside Swift X-ray observations of fourof them. Among the ten CVs presented here are those that may be low-luminosity intermediate polars or WZ Sge-type dwarf novae with rare outbursts, two subclasses that can be easily missed in time-domain and X-ray surveys,the two methods currently dominating the discovery of new CVs. Our approach based on S-PLUS provides animportant complementary tool to uncover the total population of CVs and the complete set of its subclasses, whichis an important step toward a full understanding of close binary evolution, including the origin of magnetic fields inwhite dwarfs and the physics of accretion. Finally, we highlight the potential of S-PLUS beyond AWDs, servingother surveys in the characterization of their sources.
Fil: Lopes de Oliveira, Raimundo. Universidade Federal de Sergipe; Brasil
Fil: de Araújo, Amanda S.. Universidade Federal de Sergipe; Brasil
Fil: Krabbe, Angela C.. Universidade Do Sao Paulo. Instituto Astronomia, Geofísica E Ciencias Atmosfericas. Departamento de Astronomia; Brasil
Fil: Mendes de Oliveira, Claudia Lucia. Universidade Do Sao Paulo. Instituto Astronomia, Geofísica E Ciencias Atmosfericas. Departamento de Astronomia; Brasil
Fil: Mukai, Koji. University of Maryland; Estados Unidos
Fil: Gutierrez Soto, Luis Angel. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; Argentina
Fil: Kanaan, Antonio. Universidade Federal de Santa Catarina; Brasil
Fil: Eleutério, Romualdo. Ministério de Ciencia, Tecnologia e Innovacao. Observatorio Nacional; Brasil
Fil: Borges Fernandes, Marcelo. Ministério de Ciencia, Tecnologia e Innovacao. Observatorio Nacional; Brasil
Fil: Quispe-Huaynasi, Fredi. Ministério de Ciencia, Tecnologia e Innovacao. Observatorio Nacional; Brasil
Fil: Schoenell, William. The Observatories Of The Carnegie; Estados Unidos
Fil: Ribeiro, Tiago. No especifíca;
Materia
Cataclysmic variable stars
Nivel de accesibilidad
acceso abierto
Condiciones de uso
https://creativecommons.org/licenses/by/2.5/ar/
Repositorio
CONICET Digital (CONICET)
Institución
Consejo Nacional de Investigaciones Científicas y Técnicas
OAI Identificador
oai:ri.conicet.gov.ar:11336/290714
Acceder
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network_acronym_str CONICETDig
repository_id_str 3498
network_name_str CONICET Digital (CONICET)
spelling The S-PLUS 12-band Photometry as a Powerful Tool for Discovery and Classification: Ten Cataclysmic Variables in a Proof-of-concept StudyLopes de Oliveira, Raimundode Araújo, Amanda S.Krabbe, Angela C.Mendes de Oliveira, Claudia LuciaMukai, KojiGutierrez Soto, Luis AngelKanaan, AntonioEleutério, RomualdoBorges Fernandes, MarceloQuispe-Huaynasi, FrediSchoenell, WilliamRibeiro, TiagoCataclysmic variable starshttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1Multiband photometric surveys provide a straightforward way to discover and classify astrophysical objectssystematically, enabling the study of a large number of targets at relatively low cost. Here we introduce analternative approach to select accreting white dwarf (AWD) candidates following their spectral energy distribution,entirely supported by the twelve photometric bands of the Southern Photometric Local Universe Survey (S-PLUS).The method was validated with optical spectroscopic follow-up with the Gemini South telescope, whichunambiguously established ten systems as cataclysmic variables (CVs), alongside Swift X-ray observations of fourof them. Among the ten CVs presented here are those that may be low-luminosity intermediate polars or WZ Sge-type dwarf novae with rare outbursts, two subclasses that can be easily missed in time-domain and X-ray surveys,the two methods currently dominating the discovery of new CVs. Our approach based on S-PLUS provides animportant complementary tool to uncover the total population of CVs and the complete set of its subclasses, whichis an important step toward a full understanding of close binary evolution, including the origin of magnetic fields inwhite dwarfs and the physics of accretion. Finally, we highlight the potential of S-PLUS beyond AWDs, servingother surveys in the characterization of their sources.Fil: Lopes de Oliveira, Raimundo. Universidade Federal de Sergipe; BrasilFil: de Araújo, Amanda S.. Universidade Federal de Sergipe; BrasilFil: Krabbe, Angela C.. Universidade Do Sao Paulo. Instituto Astronomia, Geofísica E Ciencias Atmosfericas. Departamento de Astronomia; BrasilFil: Mendes de Oliveira, Claudia Lucia. Universidade Do Sao Paulo. Instituto Astronomia, Geofísica E Ciencias Atmosfericas. Departamento de Astronomia; BrasilFil: Mukai, Koji. University of Maryland; Estados UnidosFil: Gutierrez Soto, Luis Angel. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; ArgentinaFil: Kanaan, Antonio. Universidade Federal de Santa Catarina; BrasilFil: Eleutério, Romualdo. Ministério de Ciencia, Tecnologia e Innovacao. Observatorio Nacional; BrasilFil: Borges Fernandes, Marcelo. Ministério de Ciencia, Tecnologia e Innovacao. Observatorio Nacional; BrasilFil: Quispe-Huaynasi, Fredi. Ministério de Ciencia, Tecnologia e Innovacao. Observatorio Nacional; BrasilFil: Schoenell, William. The Observatories Of The Carnegie; Estados UnidosFil: Ribeiro, Tiago. No especifíca;IOP Publishing2025-02-07info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/290714Lopes de Oliveira, Raimundo; de Araújo, Amanda S.; Krabbe, Angela C.; Mendes de Oliveira, Claudia Lucia; Mukai, Koji; et al.; The S-PLUS 12-band Photometry as a Powerful Tool for Discovery and Classification: Ten Cataclysmic Variables in a Proof-of-concept Study; IOP Publishing; The Astrophysical Journal Letters; 981; 1; 7-2-2025; 1-82041-82052041-8213CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/url/https://iopscience.iop.org/article/10.3847/2041-8213/adb0c8info:eu-repo/semantics/altIdentifier/doi/10.3847/2041-8213/adb0c8info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2026-08-25T15:09:06Zoai:ri.conicet.gov.ar:11336/290714instacron: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:34982026-08-25 15:09:07.984CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv The S-PLUS 12-band Photometry as a Powerful Tool for Discovery and Classification: Ten Cataclysmic Variables in a Proof-of-concept Study
title The S-PLUS 12-band Photometry as a Powerful Tool for Discovery and Classification: Ten Cataclysmic Variables in a Proof-of-concept Study
spellingShingle The S-PLUS 12-band Photometry as a Powerful Tool for Discovery and Classification: Ten Cataclysmic Variables in a Proof-of-concept Study
Lopes de Oliveira, Raimundo
Cataclysmic variable stars
title_short The S-PLUS 12-band Photometry as a Powerful Tool for Discovery and Classification: Ten Cataclysmic Variables in a Proof-of-concept Study
title_full The S-PLUS 12-band Photometry as a Powerful Tool for Discovery and Classification: Ten Cataclysmic Variables in a Proof-of-concept Study
title_fullStr The S-PLUS 12-band Photometry as a Powerful Tool for Discovery and Classification: Ten Cataclysmic Variables in a Proof-of-concept Study
title_full_unstemmed The S-PLUS 12-band Photometry as a Powerful Tool for Discovery and Classification: Ten Cataclysmic Variables in a Proof-of-concept Study
title_sort The S-PLUS 12-band Photometry as a Powerful Tool for Discovery and Classification: Ten Cataclysmic Variables in a Proof-of-concept Study
dc.creator.none.fl_str_mv Lopes de Oliveira, Raimundo
de Araújo, Amanda S.
Krabbe, Angela C.
Mendes de Oliveira, Claudia Lucia
Mukai, Koji
Gutierrez Soto, Luis Angel
Kanaan, Antonio
Eleutério, Romualdo
Borges Fernandes, Marcelo
Quispe-Huaynasi, Fredi
Schoenell, William
Ribeiro, Tiago
author Lopes de Oliveira, Raimundo
author_facet Lopes de Oliveira, Raimundo
de Araújo, Amanda S.
Krabbe, Angela C.
Mendes de Oliveira, Claudia Lucia
Mukai, Koji
Gutierrez Soto, Luis Angel
Kanaan, Antonio
Eleutério, Romualdo
Borges Fernandes, Marcelo
Quispe-Huaynasi, Fredi
Schoenell, William
Ribeiro, Tiago
author_role author
author2 de Araújo, Amanda S.
Krabbe, Angela C.
Mendes de Oliveira, Claudia Lucia
Mukai, Koji
Gutierrez Soto, Luis Angel
Kanaan, Antonio
Eleutério, Romualdo
Borges Fernandes, Marcelo
Quispe-Huaynasi, Fredi
Schoenell, William
Ribeiro, Tiago
author2_role author
author
author
author
author
author
author
author
author
author
author
dc.subject.none.fl_str_mv Cataclysmic variable stars
topic Cataclysmic variable stars
purl_subject.fl_str_mv https://purl.org/becyt/ford/1.3
https://purl.org/becyt/ford/1
dc.description.none.fl_txt_mv Multiband photometric surveys provide a straightforward way to discover and classify astrophysical objectssystematically, enabling the study of a large number of targets at relatively low cost. Here we introduce analternative approach to select accreting white dwarf (AWD) candidates following their spectral energy distribution,entirely supported by the twelve photometric bands of the Southern Photometric Local Universe Survey (S-PLUS).The method was validated with optical spectroscopic follow-up with the Gemini South telescope, whichunambiguously established ten systems as cataclysmic variables (CVs), alongside Swift X-ray observations of fourof them. Among the ten CVs presented here are those that may be low-luminosity intermediate polars or WZ Sge-type dwarf novae with rare outbursts, two subclasses that can be easily missed in time-domain and X-ray surveys,the two methods currently dominating the discovery of new CVs. Our approach based on S-PLUS provides animportant complementary tool to uncover the total population of CVs and the complete set of its subclasses, whichis an important step toward a full understanding of close binary evolution, including the origin of magnetic fields inwhite dwarfs and the physics of accretion. Finally, we highlight the potential of S-PLUS beyond AWDs, servingother surveys in the characterization of their sources.
Fil: Lopes de Oliveira, Raimundo. Universidade Federal de Sergipe; Brasil
Fil: de Araújo, Amanda S.. Universidade Federal de Sergipe; Brasil
Fil: Krabbe, Angela C.. Universidade Do Sao Paulo. Instituto Astronomia, Geofísica E Ciencias Atmosfericas. Departamento de Astronomia; Brasil
Fil: Mendes de Oliveira, Claudia Lucia. Universidade Do Sao Paulo. Instituto Astronomia, Geofísica E Ciencias Atmosfericas. Departamento de Astronomia; Brasil
Fil: Mukai, Koji. University of Maryland; Estados Unidos
Fil: Gutierrez Soto, Luis Angel. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; Argentina
Fil: Kanaan, Antonio. Universidade Federal de Santa Catarina; Brasil
Fil: Eleutério, Romualdo. Ministério de Ciencia, Tecnologia e Innovacao. Observatorio Nacional; Brasil
Fil: Borges Fernandes, Marcelo. Ministério de Ciencia, Tecnologia e Innovacao. Observatorio Nacional; Brasil
Fil: Quispe-Huaynasi, Fredi. Ministério de Ciencia, Tecnologia e Innovacao. Observatorio Nacional; Brasil
Fil: Schoenell, William. The Observatories Of The Carnegie; Estados Unidos
Fil: Ribeiro, Tiago. No especifíca;
description Multiband photometric surveys provide a straightforward way to discover and classify astrophysical objectssystematically, enabling the study of a large number of targets at relatively low cost. Here we introduce analternative approach to select accreting white dwarf (AWD) candidates following their spectral energy distribution,entirely supported by the twelve photometric bands of the Southern Photometric Local Universe Survey (S-PLUS).The method was validated with optical spectroscopic follow-up with the Gemini South telescope, whichunambiguously established ten systems as cataclysmic variables (CVs), alongside Swift X-ray observations of fourof them. Among the ten CVs presented here are those that may be low-luminosity intermediate polars or WZ Sge-type dwarf novae with rare outbursts, two subclasses that can be easily missed in time-domain and X-ray surveys,the two methods currently dominating the discovery of new CVs. Our approach based on S-PLUS provides animportant complementary tool to uncover the total population of CVs and the complete set of its subclasses, whichis an important step toward a full understanding of close binary evolution, including the origin of magnetic fields inwhite dwarfs and the physics of accretion. Finally, we highlight the potential of S-PLUS beyond AWDs, servingother surveys in the characterization of their sources.
publishDate 2025
dc.date.none.fl_str_mv 2025-02-07
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/11336/290714
Lopes de Oliveira, Raimundo; de Araújo, Amanda S.; Krabbe, Angela C.; Mendes de Oliveira, Claudia Lucia; Mukai, Koji; et al.; The S-PLUS 12-band Photometry as a Powerful Tool for Discovery and Classification: Ten Cataclysmic Variables in a Proof-of-concept Study; IOP Publishing; The Astrophysical Journal Letters; 981; 1; 7-2-2025; 1-8
2041-8205
2041-8213
CONICET Digital
CONICET
url http://hdl.handle.net/11336/290714
identifier_str_mv Lopes de Oliveira, Raimundo; de Araújo, Amanda S.; Krabbe, Angela C.; Mendes de Oliveira, Claudia Lucia; Mukai, Koji; et al.; The S-PLUS 12-band Photometry as a Powerful Tool for Discovery and Classification: Ten Cataclysmic Variables in a Proof-of-concept Study; IOP Publishing; The Astrophysical Journal Letters; 981; 1; 7-2-2025; 1-8
2041-8205
2041-8213
CONICET Digital
CONICET
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/url/https://iopscience.iop.org/article/10.3847/2041-8213/adb0c8
info:eu-repo/semantics/altIdentifier/doi/10.3847/2041-8213/adb0c8
dc.rights.none.fl_str_mv info:eu-repo/semantics/openAccess
https://creativecommons.org/licenses/by/2.5/ar/
eu_rights_str_mv openAccess
rights_invalid_str_mv https://creativecommons.org/licenses/by/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 13.265058

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