PHANGS-HST Catalogs for ∼100,000 Star Clusters and Compact Associations in 38 Galaxies. I. Observed Properties

Autores: Maschmann, Daniel; Lee, Janice C.; Thilker, David A.; Whitmore, Bradley C.; Deger, Sinan; Boquien, Médéric; Chandar, Rupali; Dale, Daniel A.; Wofford, Aida; Hannon, Stephen; Larson, Kirsten L.; Leroy, Adam K.; Schinnerer, Eva; Rosolowsky, Erik; Úbeda, Leonardo; Barnes, Ashley T.; Emsellem, Eric; Grasha, Kathryn; Groves, Brent; Indebetouw, Rémy; Kim, Hwihyun; Klessen, Ralf S.; Kreckel, Kathryn; Levy, Rebecca C.; Pinna, Francesca; Rodriguez, Maria Jimena; Tian, Qiushi; Williams, Thomas G.
Año de publicación: 2024
Idioma: inglés
Tipo de recurso: artículo
Estado: versión publicada
Descripción: We present the largest catalog to date of star clusters and compact associations in nearby galaxies. We have performed a V-band-selected census of clusters across the 38 spiral galaxies of the PHANGS–Hubble Space Telescope (HST) Treasury Survey, and measured integrated, aperture-corrected near-ultraviolet-U-B-V-I photometry. This work has resulted in uniform catalogs that contain ∼20,000 clusters and compact associations, which have passed human inspection and morphological classification, and a larger sample of ∼100,000 classified by neural network models. Here, we report on the observed properties of these samples, and demonstrate that tremendous insight can be gained from just the observed properties of clusters, even in the absence of their transformation into physical quantities. In particular, we show the utility of the UBVI color–color diagram, and the three principal features revealed by the PHANGS-HST cluster sample: the young cluster locus, the middle-age plume, and the old globular cluster clump. We present an atlas of maps of the 2D spatial distribution of clusters and compact associations in the context of the molecular clouds from PHANGS–Atacama Large Millimeter/submillimeter Array. We explore new ways of understanding this large data set in a multiscale context by bringing together once-separate techniques for the characterization of clusters (color–color diagrams and spatial distributions) and their parent galaxies (galaxy morphology and location relative to the galaxy main sequence). A companion paper presents the physical properties: ages, masses, and dust reddenings derived using improved spectral energy distribution fitting techniques.
Fil: Maschmann, Daniel. University of Arizona; Estados Unidos
Fil: Lee, Janice C.. Space Telescope Science Institute; Estados Unidos
Fil: Thilker, David A.. University Johns Hopkins; Estados Unidos
Fil: Whitmore, Bradley C.. Space Telescope Science Institute; Estados Unidos
Fil: Deger, Sinan. Kavli Institute for Cosmology Cambridge; Reino Unido. University of Cambridge; Estados Unidos
Fil: Boquien, Médéric. Université Côte d’Azur; Francia
Fil: Chandar, Rupali. University Of Toledo (utoledo); Estados Unidos
Fil: Dale, Daniel A.. Space Telescope Science Institute; Estados Unidos. University of Wyoming; Estados Unidos
Fil: Wofford, Aida. Universidad Nacional Autónoma de México; México
Fil: Hannon, Stephen. Max Planck Institute For Astronomy; Alemania
Fil: Larson, Kirsten L.. Space Telescope Science Institute; Estados Unidos
Fil: Leroy, Adam K.. Space Telescope Science Institute; Estados Unidos
Fil: Schinnerer, Eva. Ohio State University; Estados Unidos
Fil: Rosolowsky, Erik. University of Alberta; Canadá
Fil: Úbeda, Leonardo. Space Telescope Science Institute; Estados Unidos
Fil: Barnes, Ashley T.. European Southern Observatory; Alemania
Fil: Emsellem, Eric. European Southern Observatory; Alemania. Universite Claude Bernard Lyon 1. Institut de Physique Nucléaire de Lyon.; Francia
Fil: Grasha, Kathryn. Australian National University; Australia. ARC Centre of Excellence for All Sky Astrophysics in 3 Dimensions; Alemania
Fil: Groves, Brent. University of Western Australia; Australia
Fil: Indebetouw, Rémy. University of Virginia; Estados Unidos
Fil: Kim, Hwihyun. Gemini Observatory; Estados Unidos
Fil: Klessen, Ralf S.. Ruprecht Karls Universitat Heidelberg; Alemania
Fil: Kreckel, Kathryn. Ruprecht Karls Universitat Heidelberg; Alemania
Fil: Levy, Rebecca C.. No especifíca;
Fil: Pinna, Francesca. Max-Planck-Institut für Astronomie; Alemania
Fil: Rodriguez, Maria Jimena. 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: Tian, Qiushi. Ohio Wesleyan University.; Estados Unidos
Fil: Williams, Thomas G.. University of Oxford; Reino Unido
Materia: STAR FORMATION
STAR CLUSTERS
GALAXY EVOLUTION
Nivel de accesibilidad: acceso abierto
Condiciones de uso: https://creativecommons.org/licenses/by/2.5/ar/
Repositorio
Institución: Consejo Nacional de Investigaciones Científicas y Técnicas
OAI Identificador: oai:ri.conicet.gov.ar:11336/275784

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spelling	PHANGS-HST Catalogs for ∼100,000 Star Clusters and Compact Associations in 38 Galaxies. I. Observed PropertiesMaschmann, DanielLee, Janice C.Thilker, David A.Whitmore, Bradley C.Deger, SinanBoquien, MédéricChandar, RupaliDale, Daniel A.Wofford, AidaHannon, StephenLarson, Kirsten L.Leroy, Adam K.Schinnerer, EvaRosolowsky, ErikÚbeda, LeonardoBarnes, Ashley T.Emsellem, EricGrasha, KathrynGroves, BrentIndebetouw, RémyKim, HwihyunKlessen, Ralf S.Kreckel, KathrynLevy, Rebecca C.Pinna, FrancescaRodriguez, Maria JimenaTian, QiushiWilliams, Thomas G.STAR FORMATIONSTAR CLUSTERSGALAXY EVOLUTIONhttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1We present the largest catalog to date of star clusters and compact associations in nearby galaxies. We have performed a V-band-selected census of clusters across the 38 spiral galaxies of the PHANGS–Hubble Space Telescope (HST) Treasury Survey, and measured integrated, aperture-corrected near-ultraviolet-U-B-V-I photometry. This work has resulted in uniform catalogs that contain ∼20,000 clusters and compact associations, which have passed human inspection and morphological classification, and a larger sample of ∼100,000 classified by neural network models. Here, we report on the observed properties of these samples, and demonstrate that tremendous insight can be gained from just the observed properties of clusters, even in the absence of their transformation into physical quantities. In particular, we show the utility of the UBVI color–color diagram, and the three principal features revealed by the PHANGS-HST cluster sample: the young cluster locus, the middle-age plume, and the old globular cluster clump. We present an atlas of maps of the 2D spatial distribution of clusters and compact associations in the context of the molecular clouds from PHANGS–Atacama Large Millimeter/submillimeter Array. We explore new ways of understanding this large data set in a multiscale context by bringing together once-separate techniques for the characterization of clusters (color–color diagrams and spatial distributions) and their parent galaxies (galaxy morphology and location relative to the galaxy main sequence). A companion paper presents the physical properties: ages, masses, and dust reddenings derived using improved spectral energy distribution fitting techniques.Fil: Maschmann, Daniel. University of Arizona; Estados UnidosFil: Lee, Janice C.. Space Telescope Science Institute; Estados UnidosFil: Thilker, David A.. University Johns Hopkins; Estados UnidosFil: Whitmore, Bradley C.. Space Telescope Science Institute; Estados UnidosFil: Deger, Sinan. Kavli Institute for Cosmology Cambridge; Reino Unido. University of Cambridge; Estados UnidosFil: Boquien, Médéric. Université Côte d’Azur; FranciaFil: Chandar, Rupali. University Of Toledo (utoledo); Estados UnidosFil: Dale, Daniel A.. Space Telescope Science Institute; Estados Unidos. University of Wyoming; Estados UnidosFil: Wofford, Aida. Universidad Nacional Autónoma de México; MéxicoFil: Hannon, Stephen. Max Planck Institute For Astronomy; AlemaniaFil: Larson, Kirsten L.. Space Telescope Science Institute; Estados UnidosFil: Leroy, Adam K.. Space Telescope Science Institute; Estados UnidosFil: Schinnerer, Eva. Ohio State University; Estados UnidosFil: Rosolowsky, Erik. University of Alberta; CanadáFil: Úbeda, Leonardo. Space Telescope Science Institute; Estados UnidosFil: Barnes, Ashley T.. European Southern Observatory; AlemaniaFil: Emsellem, Eric. European Southern Observatory; Alemania. Universite Claude Bernard Lyon 1. Institut de Physique Nucléaire de Lyon.; FranciaFil: Grasha, Kathryn. Australian National University; Australia. ARC Centre of Excellence for All Sky Astrophysics in 3 Dimensions; AlemaniaFil: Groves, Brent. University of Western Australia; AustraliaFil: Indebetouw, Rémy. University of Virginia; Estados UnidosFil: Kim, Hwihyun. Gemini Observatory; Estados UnidosFil: Klessen, Ralf S.. Ruprecht Karls Universitat Heidelberg; AlemaniaFil: Kreckel, Kathryn. Ruprecht Karls Universitat Heidelberg; AlemaniaFil: Levy, Rebecca C.. No especifíca;Fil: Pinna, Francesca. Max-Planck-Institut für Astronomie; AlemaniaFil: Rodriguez, Maria Jimena. 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: Tian, Qiushi. Ohio Wesleyan University.; Estados UnidosFil: Williams, Thomas G.. University of Oxford; Reino UnidoIOP Publishing2024-07-07info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/275784Maschmann, Daniel; Lee, Janice C.; Thilker, David A.; Whitmore, Bradley C.; Deger, Sinan; et al.; PHANGS-HST Catalogs for ∼100,000 Star Clusters and Compact Associations in 38 Galaxies. I. Observed Properties; IOP Publishing; Astrophysical Journal Supplement Series; 273; 1; 7-7-2024; 1-300067-0049CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/url/https://iopscience.iop.org/article/10.3847/1538-4365/ad3cd3info:eu-repo/semantics/altIdentifier/doi/10.3847/1538-4365/ad3cd3info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-12-23T13:13:57Zoai:ri.conicet.gov.ar:11336/275784instacron: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:34982025-12-23 13:13:57.489CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv	PHANGS-HST Catalogs for ∼100,000 Star Clusters and Compact Associations in 38 Galaxies. I. Observed Properties
title	PHANGS-HST Catalogs for ∼100,000 Star Clusters and Compact Associations in 38 Galaxies. I. Observed Properties
spellingShingle	PHANGS-HST Catalogs for ∼100,000 Star Clusters and Compact Associations in 38 Galaxies. I. Observed Properties Maschmann, Daniel STAR FORMATION STAR CLUSTERS GALAXY EVOLUTION
title_short	PHANGS-HST Catalogs for ∼100,000 Star Clusters and Compact Associations in 38 Galaxies. I. Observed Properties
title_full	PHANGS-HST Catalogs for ∼100,000 Star Clusters and Compact Associations in 38 Galaxies. I. Observed Properties
title_fullStr	PHANGS-HST Catalogs for ∼100,000 Star Clusters and Compact Associations in 38 Galaxies. I. Observed Properties
title_full_unstemmed	PHANGS-HST Catalogs for ∼100,000 Star Clusters and Compact Associations in 38 Galaxies. I. Observed Properties
title_sort	PHANGS-HST Catalogs for ∼100,000 Star Clusters and Compact Associations in 38 Galaxies. I. Observed Properties
dc.creator.none.fl_str_mv	Maschmann, Daniel Lee, Janice C. Thilker, David A. Whitmore, Bradley C. Deger, Sinan Boquien, Médéric Chandar, Rupali Dale, Daniel A. Wofford, Aida Hannon, Stephen Larson, Kirsten L. Leroy, Adam K. Schinnerer, Eva Rosolowsky, Erik Úbeda, Leonardo Barnes, Ashley T. Emsellem, Eric Grasha, Kathryn Groves, Brent Indebetouw, Rémy Kim, Hwihyun Klessen, Ralf S. Kreckel, Kathryn Levy, Rebecca C. Pinna, Francesca Rodriguez, Maria Jimena Tian, Qiushi Williams, Thomas G.
author	Maschmann, Daniel
author_facet	Maschmann, Daniel Lee, Janice C. Thilker, David A. Whitmore, Bradley C. Deger, Sinan Boquien, Médéric Chandar, Rupali Dale, Daniel A. Wofford, Aida Hannon, Stephen Larson, Kirsten L. Leroy, Adam K. Schinnerer, Eva Rosolowsky, Erik Úbeda, Leonardo Barnes, Ashley T. Emsellem, Eric Grasha, Kathryn Groves, Brent Indebetouw, Rémy Kim, Hwihyun Klessen, Ralf S. Kreckel, Kathryn Levy, Rebecca C. Pinna, Francesca Rodriguez, Maria Jimena Tian, Qiushi Williams, Thomas G.
author_role	author
author2	Lee, Janice C. Thilker, David A. Whitmore, Bradley C. Deger, Sinan Boquien, Médéric Chandar, Rupali Dale, Daniel A. Wofford, Aida Hannon, Stephen Larson, Kirsten L. Leroy, Adam K. Schinnerer, Eva Rosolowsky, Erik Úbeda, Leonardo Barnes, Ashley T. Emsellem, Eric Grasha, Kathryn Groves, Brent Indebetouw, Rémy Kim, Hwihyun Klessen, Ralf S. Kreckel, Kathryn Levy, Rebecca C. Pinna, Francesca Rodriguez, Maria Jimena Tian, Qiushi Williams, Thomas G.
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	STAR FORMATION STAR CLUSTERS GALAXY EVOLUTION
topic	STAR FORMATION STAR CLUSTERS GALAXY EVOLUTION
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 catalog to date of star clusters and compact associations in nearby galaxies. We have performed a V-band-selected census of clusters across the 38 spiral galaxies of the PHANGS–Hubble Space Telescope (HST) Treasury Survey, and measured integrated, aperture-corrected near-ultraviolet-U-B-V-I photometry. This work has resulted in uniform catalogs that contain ∼20,000 clusters and compact associations, which have passed human inspection and morphological classification, and a larger sample of ∼100,000 classified by neural network models. Here, we report on the observed properties of these samples, and demonstrate that tremendous insight can be gained from just the observed properties of clusters, even in the absence of their transformation into physical quantities. In particular, we show the utility of the UBVI color–color diagram, and the three principal features revealed by the PHANGS-HST cluster sample: the young cluster locus, the middle-age plume, and the old globular cluster clump. We present an atlas of maps of the 2D spatial distribution of clusters and compact associations in the context of the molecular clouds from PHANGS–Atacama Large Millimeter/submillimeter Array. We explore new ways of understanding this large data set in a multiscale context by bringing together once-separate techniques for the characterization of clusters (color–color diagrams and spatial distributions) and their parent galaxies (galaxy morphology and location relative to the galaxy main sequence). A companion paper presents the physical properties: ages, masses, and dust reddenings derived using improved spectral energy distribution fitting techniques. Fil: Maschmann, Daniel. University of Arizona; Estados Unidos Fil: Lee, Janice C.. Space Telescope Science Institute; Estados Unidos Fil: Thilker, David A.. University Johns Hopkins; Estados Unidos Fil: Whitmore, Bradley C.. Space Telescope Science Institute; Estados Unidos Fil: Deger, Sinan. Kavli Institute for Cosmology Cambridge; Reino Unido. University of Cambridge; Estados Unidos Fil: Boquien, Médéric. Université Côte d’Azur; Francia Fil: Chandar, Rupali. University Of Toledo (utoledo); Estados Unidos Fil: Dale, Daniel A.. Space Telescope Science Institute; Estados Unidos. University of Wyoming; Estados Unidos Fil: Wofford, Aida. Universidad Nacional Autónoma de México; México Fil: Hannon, Stephen. Max Planck Institute For Astronomy; Alemania Fil: Larson, Kirsten L.. Space Telescope Science Institute; Estados Unidos Fil: Leroy, Adam K.. Space Telescope Science Institute; Estados Unidos Fil: Schinnerer, Eva. Ohio State University; Estados Unidos Fil: Rosolowsky, Erik. University of Alberta; Canadá Fil: Úbeda, Leonardo. Space Telescope Science Institute; Estados Unidos Fil: Barnes, Ashley T.. European Southern Observatory; Alemania Fil: Emsellem, Eric. European Southern Observatory; Alemania. Universite Claude Bernard Lyon 1. Institut de Physique Nucléaire de Lyon.; Francia Fil: Grasha, Kathryn. Australian National University; Australia. ARC Centre of Excellence for All Sky Astrophysics in 3 Dimensions; Alemania Fil: Groves, Brent. University of Western Australia; Australia Fil: Indebetouw, Rémy. University of Virginia; Estados Unidos Fil: Kim, Hwihyun. Gemini Observatory; Estados Unidos Fil: Klessen, Ralf S.. Ruprecht Karls Universitat Heidelberg; Alemania Fil: Kreckel, Kathryn. Ruprecht Karls Universitat Heidelberg; Alemania Fil: Levy, Rebecca C.. No especifíca; Fil: Pinna, Francesca. Max-Planck-Institut für Astronomie; Alemania Fil: Rodriguez, Maria Jimena. 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: Tian, Qiushi. Ohio Wesleyan University.; Estados Unidos Fil: Williams, Thomas G.. University of Oxford; Reino Unido
description	We present the largest catalog to date of star clusters and compact associations in nearby galaxies. We have performed a V-band-selected census of clusters across the 38 spiral galaxies of the PHANGS–Hubble Space Telescope (HST) Treasury Survey, and measured integrated, aperture-corrected near-ultraviolet-U-B-V-I photometry. This work has resulted in uniform catalogs that contain ∼20,000 clusters and compact associations, which have passed human inspection and morphological classification, and a larger sample of ∼100,000 classified by neural network models. Here, we report on the observed properties of these samples, and demonstrate that tremendous insight can be gained from just the observed properties of clusters, even in the absence of their transformation into physical quantities. In particular, we show the utility of the UBVI color–color diagram, and the three principal features revealed by the PHANGS-HST cluster sample: the young cluster locus, the middle-age plume, and the old globular cluster clump. We present an atlas of maps of the 2D spatial distribution of clusters and compact associations in the context of the molecular clouds from PHANGS–Atacama Large Millimeter/submillimeter Array. We explore new ways of understanding this large data set in a multiscale context by bringing together once-separate techniques for the characterization of clusters (color–color diagrams and spatial distributions) and their parent galaxies (galaxy morphology and location relative to the galaxy main sequence). A companion paper presents the physical properties: ages, masses, and dust reddenings derived using improved spectral energy distribution fitting techniques.
publishDate	2024
dc.date.none.fl_str_mv	2024-07-07
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/11336/275784 Maschmann, Daniel; Lee, Janice C.; Thilker, David A.; Whitmore, Bradley C.; Deger, Sinan; et al.; PHANGS-HST Catalogs for ∼100,000 Star Clusters and Compact Associations in 38 Galaxies. I. Observed Properties; IOP Publishing; Astrophysical Journal Supplement Series; 273; 1; 7-7-2024; 1-30 0067-0049 CONICET Digital CONICET
url	http://hdl.handle.net/11336/275784
identifier_str_mv	Maschmann, Daniel; Lee, Janice C.; Thilker, David A.; Whitmore, Bradley C.; Deger, Sinan; et al.; PHANGS-HST Catalogs for ∼100,000 Star Clusters and Compact Associations in 38 Galaxies. I. Observed Properties; IOP Publishing; Astrophysical Journal Supplement Series; 273; 1; 7-7-2024; 1-30 0067-0049 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/10.3847/1538-4365/ad3cd3 info:eu-repo/semantics/altIdentifier/doi/10.3847/1538-4365/ad3cd3
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)
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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	12.441415

PHANGS-HST Catalogs for ∼100,000 Star Clusters and Compact Associations in 38 Galaxies. I. Observed Properties

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