The S-PLUS Fornax Project (S+FP): Mapping Globular Clusters Systems within 5 Virial Radii around NGC 1399
- Autores
- Lomelí Núñez, Luis; Cortesi, A.; Smith Castelli, Analia Viviana; Buzzo, M. L.; Mayya, Y. D.; Fragkou, Vasiliki; Alzate Trujillo, J. A.; Haack, Rodrigo Facundo; Calderón, Juan Pablo; Reis Lopes, Amanda; Hilker, Michael; Grossi, M.; Menéndez Delmestre, Karín; Gonçalves, Thiago S.; Chies Santos, Ana L.; Gutierrez Soto, Luis Angel; Lima Dias, Ciria; Werner, S. V.; Humire, Pedro K.; Thom de Souza, R. C.; Alvarez Candal, A.; Panda, Swayamtrupta; Chaturvedi, Avinash; Telles, E.; Mendes de Oliveira, C.; Kanaan, A.; Ribeiro, T.; Schoenell, W.
- Año de publicación
- 2025
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- We present the largest sample (∼13,000 candidates, ∼3000 of which are bona fide candidates) of globular cluster (GCs) candidates reported in the Fornax cluster so far. The survey is centered on the NGC 1399 galaxy, extending out to 5 virial radii (Rvir) of the cluster. We carried out a photometric study using images observed in the 12-band system of the Southern Photometric Local Universe Survey (S-PLUS), corresponding to 106 pointings, covering a sky area of ∼208 square degrees. Studying the properties of spectroscopically confirmed GCs, we have designed a method to select GC candidates using structural and photometric parameters. We found evidence of color bimodality in two broadband colors, namely (g − i)0 and (g − z)0, while, in the narrow bands, we did not find strong statistical evidence to confirm bimodality in any color. We analyzed the GCs luminosity functions (GCLF) in the 12 bands of S-PLUS, and we can highlight two points: (a) due to the relatively shallow depth of S-PLUS, it is only possible to observe the bright end of the GCLF and, (b) at that level, in all of the bands, it can be considered to be the log-normal distribution typical for GC systems. With the spatial coverage reached in this study, we are able, for the first time, to explore the large-scale distribution of GCs within and around a galaxy cluster. In particular, we noted that the GCs might be clustered along substructures, which trace the current cluster buildup.
Fil: Lomelí Núñez, Luis. Universidade Federal do Rio de Janeiro; Brasil
Fil: Cortesi, A.. Universidade Federal do Rio de Janeiro; Brasil
Fil: Smith Castelli, Analia Viviana. 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: Buzzo, M. L.. Swinburne University; Australia
Fil: Mayya, Y. D.. Instituto Nacional de Astrofísica, Óptica y Electrónica; México
Fil: Fragkou, Vasiliki. Universidade Federal do Rio de Janeiro; Brasil
Fil: Alzate Trujillo, J. A.. Centro de Estudios de Física del Cosmos de Aragón; España
Fil: Haack, Rodrigo Facundo. 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: Calderón, Juan Pablo. 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: Reis Lopes, Amanda. 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: Hilker, Michael. European Southern Observatory; Chile
Fil: Grossi, M.. Universidade Federal do Rio de Janeiro; Brasil
Fil: Menéndez Delmestre, Karín. Universidade Federal do Rio de Janeiro; Brasil
Fil: Gonçalves, Thiago S.. Universidade Federal do Rio de Janeiro; Brasil
Fil: Chies Santos, Ana L.. Universidade Federal do Rio Grande do Sul; Brasil
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: Lima Dias, Ciria. Universidad de La Serena; Chile
Fil: Werner, S. V.. University of Durham; Reino Unido
Fil: Humire, Pedro K.. Universidade de Sao Paulo; Brasil
Fil: Thom de Souza, R. C.. Universidade Federal do Paraná; Brasil
Fil: Alvarez Candal, A.. Consejo Superior de Investigaciones Científicas; España
Fil: Panda, Swayamtrupta. No especifíca;
Fil: Chaturvedi, Avinash. No especifíca;
Fil: Telles, E.. Ministério de Ciencia, Tecnologia e Innovacao. Observatorio Nacional; Brasil
Fil: Mendes de Oliveira, C.. Universidade de Sao Paulo; Brasil
Fil: Kanaan, A.. Universidade Federal de Santa Catarina; Brasil
Fil: Ribeiro, T.. No especifíca;
Fil: Schoenell, W.. No especifíca; - Materia
-
Globular star clusters
Galaxy clusters
Surveys - Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- https://creativecommons.org/licenses/by/2.5/ar/
- Repositorio
.jpg)
- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/290944
Ver los metadatos del registro completo
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The S-PLUS Fornax Project (S+FP): Mapping Globular Clusters Systems within 5 Virial Radii around NGC 1399Lomelí Núñez, LuisCortesi, A.Smith Castelli, Analia VivianaBuzzo, M. L.Mayya, Y. D.Fragkou, VasilikiAlzate Trujillo, J. A.Haack, Rodrigo FacundoCalderón, Juan PabloReis Lopes, AmandaHilker, MichaelGrossi, M.Menéndez Delmestre, KarínGonçalves, Thiago S.Chies Santos, Ana L.Gutierrez Soto, Luis AngelLima Dias, CiriaWerner, S. V.Humire, Pedro K.Thom de Souza, R. C.Alvarez Candal, A.Panda, SwayamtruptaChaturvedi, AvinashTelles, E.Mendes de Oliveira, C.Kanaan, A.Ribeiro, T.Schoenell, W.Globular star clustersGalaxy clustersSurveyshttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1We present the largest sample (∼13,000 candidates, ∼3000 of which are bona fide candidates) of globular cluster (GCs) candidates reported in the Fornax cluster so far. The survey is centered on the NGC 1399 galaxy, extending out to 5 virial radii (Rvir) of the cluster. We carried out a photometric study using images observed in the 12-band system of the Southern Photometric Local Universe Survey (S-PLUS), corresponding to 106 pointings, covering a sky area of ∼208 square degrees. Studying the properties of spectroscopically confirmed GCs, we have designed a method to select GC candidates using structural and photometric parameters. We found evidence of color bimodality in two broadband colors, namely (g − i)0 and (g − z)0, while, in the narrow bands, we did not find strong statistical evidence to confirm bimodality in any color. We analyzed the GCs luminosity functions (GCLF) in the 12 bands of S-PLUS, and we can highlight two points: (a) due to the relatively shallow depth of S-PLUS, it is only possible to observe the bright end of the GCLF and, (b) at that level, in all of the bands, it can be considered to be the log-normal distribution typical for GC systems. With the spatial coverage reached in this study, we are able, for the first time, to explore the large-scale distribution of GCs within and around a galaxy cluster. In particular, we noted that the GCs might be clustered along substructures, which trace the current cluster buildup.Fil: Lomelí Núñez, Luis. Universidade Federal do Rio de Janeiro; BrasilFil: Cortesi, A.. Universidade Federal do Rio de Janeiro; BrasilFil: Smith Castelli, Analia Viviana. 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: Buzzo, M. L.. Swinburne University; AustraliaFil: Mayya, Y. D.. Instituto Nacional de Astrofísica, Óptica y Electrónica; MéxicoFil: Fragkou, Vasiliki. Universidade Federal do Rio de Janeiro; BrasilFil: Alzate Trujillo, J. A.. Centro de Estudios de Física del Cosmos de Aragón; EspañaFil: Haack, Rodrigo Facundo. 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: Calderón, Juan Pablo. 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: Reis Lopes, Amanda. 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: Hilker, Michael. European Southern Observatory; ChileFil: Grossi, M.. Universidade Federal do Rio de Janeiro; BrasilFil: Menéndez Delmestre, Karín. Universidade Federal do Rio de Janeiro; BrasilFil: Gonçalves, Thiago S.. Universidade Federal do Rio de Janeiro; BrasilFil: Chies Santos, Ana L.. Universidade Federal do Rio Grande do Sul; BrasilFil: 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: Lima Dias, Ciria. Universidad de La Serena; ChileFil: Werner, S. V.. University of Durham; Reino UnidoFil: Humire, Pedro K.. Universidade de Sao Paulo; BrasilFil: Thom de Souza, R. C.. Universidade Federal do Paraná; BrasilFil: Alvarez Candal, A.. Consejo Superior de Investigaciones Científicas; EspañaFil: Panda, Swayamtrupta. No especifíca;Fil: Chaturvedi, Avinash. No especifíca;Fil: Telles, E.. Ministério de Ciencia, Tecnologia e Innovacao. Observatorio Nacional; BrasilFil: Mendes de Oliveira, C.. Universidade de Sao Paulo; BrasilFil: Kanaan, A.. Universidade Federal de Santa Catarina; BrasilFil: Ribeiro, T.. No especifíca;Fil: Schoenell, W.. No especifíca;IOP Publishing2025-04info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/290944Lomelí Núñez, Luis; Cortesi, A.; Smith Castelli, Analia Viviana; Buzzo, M. L.; Mayya, Y. D.; et al.; The S-PLUS Fornax Project (S+FP): Mapping Globular Clusters Systems within 5 Virial Radii around NGC 1399; IOP Publishing; Astronomical Journal; 169; 5; 4-2025; 1-260004-6256CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/url/https://iopscience.iop.org/article/10.3847/1538-3881/adbf0cinfo:eu-repo/semantics/altIdentifier/doi/10.3847/1538-3881/adbf0cinfo:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2026-08-25T14:34:25Zoai:ri.conicet.gov.ar:11336/290944instacron: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 14:34:25.595CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
| dc.title.none.fl_str_mv |
The S-PLUS Fornax Project (S+FP): Mapping Globular Clusters Systems within 5 Virial Radii around NGC 1399 |
| title |
The S-PLUS Fornax Project (S+FP): Mapping Globular Clusters Systems within 5 Virial Radii around NGC 1399 |
| spellingShingle |
The S-PLUS Fornax Project (S+FP): Mapping Globular Clusters Systems within 5 Virial Radii around NGC 1399 Lomelí Núñez, Luis Globular star clusters Galaxy clusters Surveys |
| title_short |
The S-PLUS Fornax Project (S+FP): Mapping Globular Clusters Systems within 5 Virial Radii around NGC 1399 |
| title_full |
The S-PLUS Fornax Project (S+FP): Mapping Globular Clusters Systems within 5 Virial Radii around NGC 1399 |
| title_fullStr |
The S-PLUS Fornax Project (S+FP): Mapping Globular Clusters Systems within 5 Virial Radii around NGC 1399 |
| title_full_unstemmed |
The S-PLUS Fornax Project (S+FP): Mapping Globular Clusters Systems within 5 Virial Radii around NGC 1399 |
| title_sort |
The S-PLUS Fornax Project (S+FP): Mapping Globular Clusters Systems within 5 Virial Radii around NGC 1399 |
| dc.creator.none.fl_str_mv |
Lomelí Núñez, Luis Cortesi, A. Smith Castelli, Analia Viviana Buzzo, M. L. Mayya, Y. D. Fragkou, Vasiliki Alzate Trujillo, J. A. Haack, Rodrigo Facundo Calderón, Juan Pablo Reis Lopes, Amanda Hilker, Michael Grossi, M. Menéndez Delmestre, Karín Gonçalves, Thiago S. Chies Santos, Ana L. Gutierrez Soto, Luis Angel Lima Dias, Ciria Werner, S. V. Humire, Pedro K. Thom de Souza, R. C. Alvarez Candal, A. Panda, Swayamtrupta Chaturvedi, Avinash Telles, E. Mendes de Oliveira, C. Kanaan, A. Ribeiro, T. Schoenell, W. |
| author |
Lomelí Núñez, Luis |
| author_facet |
Lomelí Núñez, Luis Cortesi, A. Smith Castelli, Analia Viviana Buzzo, M. L. Mayya, Y. D. Fragkou, Vasiliki Alzate Trujillo, J. A. Haack, Rodrigo Facundo Calderón, Juan Pablo Reis Lopes, Amanda Hilker, Michael Grossi, M. Menéndez Delmestre, Karín Gonçalves, Thiago S. Chies Santos, Ana L. Gutierrez Soto, Luis Angel Lima Dias, Ciria Werner, S. V. Humire, Pedro K. Thom de Souza, R. C. Alvarez Candal, A. Panda, Swayamtrupta Chaturvedi, Avinash Telles, E. Mendes de Oliveira, C. Kanaan, A. Ribeiro, T. Schoenell, W. |
| author_role |
author |
| author2 |
Cortesi, A. Smith Castelli, Analia Viviana Buzzo, M. L. Mayya, Y. D. Fragkou, Vasiliki Alzate Trujillo, J. A. Haack, Rodrigo Facundo Calderón, Juan Pablo Reis Lopes, Amanda Hilker, Michael Grossi, M. Menéndez Delmestre, Karín Gonçalves, Thiago S. Chies Santos, Ana L. Gutierrez Soto, Luis Angel Lima Dias, Ciria Werner, S. V. Humire, Pedro K. Thom de Souza, R. C. Alvarez Candal, A. Panda, Swayamtrupta Chaturvedi, Avinash Telles, E. Mendes de Oliveira, C. Kanaan, A. Ribeiro, T. Schoenell, W. |
| author2_role |
author author author author author author author author author author author author author author author author author author author author author author author author author author author |
| dc.subject.none.fl_str_mv |
Globular star clusters Galaxy clusters Surveys |
| topic |
Globular star clusters Galaxy clusters 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 largest sample (∼13,000 candidates, ∼3000 of which are bona fide candidates) of globular cluster (GCs) candidates reported in the Fornax cluster so far. The survey is centered on the NGC 1399 galaxy, extending out to 5 virial radii (Rvir) of the cluster. We carried out a photometric study using images observed in the 12-band system of the Southern Photometric Local Universe Survey (S-PLUS), corresponding to 106 pointings, covering a sky area of ∼208 square degrees. Studying the properties of spectroscopically confirmed GCs, we have designed a method to select GC candidates using structural and photometric parameters. We found evidence of color bimodality in two broadband colors, namely (g − i)0 and (g − z)0, while, in the narrow bands, we did not find strong statistical evidence to confirm bimodality in any color. We analyzed the GCs luminosity functions (GCLF) in the 12 bands of S-PLUS, and we can highlight two points: (a) due to the relatively shallow depth of S-PLUS, it is only possible to observe the bright end of the GCLF and, (b) at that level, in all of the bands, it can be considered to be the log-normal distribution typical for GC systems. With the spatial coverage reached in this study, we are able, for the first time, to explore the large-scale distribution of GCs within and around a galaxy cluster. In particular, we noted that the GCs might be clustered along substructures, which trace the current cluster buildup. Fil: Lomelí Núñez, Luis. Universidade Federal do Rio de Janeiro; Brasil Fil: Cortesi, A.. Universidade Federal do Rio de Janeiro; Brasil Fil: Smith Castelli, Analia Viviana. 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: Buzzo, M. L.. Swinburne University; Australia Fil: Mayya, Y. D.. Instituto Nacional de Astrofísica, Óptica y Electrónica; México Fil: Fragkou, Vasiliki. Universidade Federal do Rio de Janeiro; Brasil Fil: Alzate Trujillo, J. A.. Centro de Estudios de Física del Cosmos de Aragón; España Fil: Haack, Rodrigo Facundo. 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: Calderón, Juan Pablo. 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: Reis Lopes, Amanda. 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: Hilker, Michael. European Southern Observatory; Chile Fil: Grossi, M.. Universidade Federal do Rio de Janeiro; Brasil Fil: Menéndez Delmestre, Karín. Universidade Federal do Rio de Janeiro; Brasil Fil: Gonçalves, Thiago S.. Universidade Federal do Rio de Janeiro; Brasil Fil: Chies Santos, Ana L.. Universidade Federal do Rio Grande do Sul; Brasil 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: Lima Dias, Ciria. Universidad de La Serena; Chile Fil: Werner, S. V.. University of Durham; Reino Unido Fil: Humire, Pedro K.. Universidade de Sao Paulo; Brasil Fil: Thom de Souza, R. C.. Universidade Federal do Paraná; Brasil Fil: Alvarez Candal, A.. Consejo Superior de Investigaciones Científicas; España Fil: Panda, Swayamtrupta. No especifíca; Fil: Chaturvedi, Avinash. No especifíca; Fil: Telles, E.. Ministério de Ciencia, Tecnologia e Innovacao. Observatorio Nacional; Brasil Fil: Mendes de Oliveira, C.. Universidade de Sao Paulo; Brasil Fil: Kanaan, A.. Universidade Federal de Santa Catarina; Brasil Fil: Ribeiro, T.. No especifíca; Fil: Schoenell, W.. No especifíca; |
| description |
We present the largest sample (∼13,000 candidates, ∼3000 of which are bona fide candidates) of globular cluster (GCs) candidates reported in the Fornax cluster so far. The survey is centered on the NGC 1399 galaxy, extending out to 5 virial radii (Rvir) of the cluster. We carried out a photometric study using images observed in the 12-band system of the Southern Photometric Local Universe Survey (S-PLUS), corresponding to 106 pointings, covering a sky area of ∼208 square degrees. Studying the properties of spectroscopically confirmed GCs, we have designed a method to select GC candidates using structural and photometric parameters. We found evidence of color bimodality in two broadband colors, namely (g − i)0 and (g − z)0, while, in the narrow bands, we did not find strong statistical evidence to confirm bimodality in any color. We analyzed the GCs luminosity functions (GCLF) in the 12 bands of S-PLUS, and we can highlight two points: (a) due to the relatively shallow depth of S-PLUS, it is only possible to observe the bright end of the GCLF and, (b) at that level, in all of the bands, it can be considered to be the log-normal distribution typical for GC systems. With the spatial coverage reached in this study, we are able, for the first time, to explore the large-scale distribution of GCs within and around a galaxy cluster. In particular, we noted that the GCs might be clustered along substructures, which trace the current cluster buildup. |
| publishDate |
2025 |
| dc.date.none.fl_str_mv |
2025-04 |
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info:eu-repo/semantics/article info:eu-repo/semantics/publishedVersion http://purl.org/coar/resource_type/c_6501 info:ar-repo/semantics/articulo |
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article |
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http://hdl.handle.net/11336/290944 Lomelí Núñez, Luis; Cortesi, A.; Smith Castelli, Analia Viviana; Buzzo, M. L.; Mayya, Y. D.; et al.; The S-PLUS Fornax Project (S+FP): Mapping Globular Clusters Systems within 5 Virial Radii around NGC 1399; IOP Publishing; Astronomical Journal; 169; 5; 4-2025; 1-26 0004-6256 CONICET Digital CONICET |
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http://hdl.handle.net/11336/290944 |
| identifier_str_mv |
Lomelí Núñez, Luis; Cortesi, A.; Smith Castelli, Analia Viviana; Buzzo, M. L.; Mayya, Y. D.; et al.; The S-PLUS Fornax Project (S+FP): Mapping Globular Clusters Systems within 5 Virial Radii around NGC 1399; IOP Publishing; Astronomical Journal; 169; 5; 4-2025; 1-26 0004-6256 CONICET Digital CONICET |
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eng |
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eng |
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IOP Publishing |
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IOP Publishing |
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CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicas |
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dasensio@conicet.gov.ar; lcarlino@conicet.gov.ar |
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