Low X-Ray Luminosity Galaxy Clusters: Main goals, sample selection, photometric and spectroscopic observations
- Autores
- Nilo Castellon, Jose Luis Emilio; Alonso, Maria Victoria; Garcia Lambas, Diego Rodolfo; Valotto, Carlos Alberto; O'Mill, Ana Laura; Cuevas, Héctor; Carrasco, Eleazar Rodrigo; Ramírez, Amelia; Astudillo, José M.; Ramos Almendares, Felipe Alberto; Jaque Arancibia, Marcelo Daniel; Ulloa, Natalie; Órdenes, Yasna
- Año de publicación
- 2016
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- We present our study of 19 low X-ray luminosity galaxy clusters (L 0.5-45 × 1043 erg s-1), selected from the ROSAT Position Sensitive Proportional Counters Pointed Observations and the revised version of Mullis et al. in the redshift range of 0.16-0.7. This is the introductory paper of a series presenting the sample selection, photometric and spectroscopic observations, and data reduction. Photometric data in different passbands were taken for eight galaxy clusters at Las Campanas Observatory; three clusters at Cerro Tololo Interamerican Observatory; and eight clusters at the Gemini Observatory. Spectroscopic data were collected for only four galaxy clusters using Gemini telescopes. Using the photometry, the galaxies were defined based on the star-galaxy separation taking into account photometric parameters. For each galaxy cluster, the catalogs contain the point-spread function and aperture magnitudes of galaxies within the 90% completeness limit. They are used together with structural parameters to study the galaxy morphology and to estimate photometric redshifts. With the spectroscopy, the derived galaxy velocity dispersion of our clusters ranged from 507 km s-1 for [VMF98]022 to 775 km s-1 for [VMF98]097 with signs of substructure. Cluster membership has been extensively discussed taking into account spectroscopic and photometric redshift estimates. In this sense, members are the galaxies within a projected radius of 0.75 Mpc from the X-ray emission peak and with clustercentric velocities smaller than the cluster velocity dispersion or 6000 km s-1, respectively. These results will be used in forthcoming papers to study, among the main topics, the red cluster sequence, blue cloud and green populations, the galaxy luminosity function, and cluster dynamics.
Fil: Nilo Castellon, Jose Luis Emilio. Universidad de La Serena; Chile. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina
Fil: Alonso, Maria Victoria. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Astronomía Teórica y Experimental. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Instituto de Astronomía Teórica y Experimental; Argentina. Universidad Nacional de Cordoba. Observatorio Astronomico de Cordoba; Argentina
Fil: Garcia Lambas, Diego Rodolfo. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Astronomía Teórica y Experimental. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Instituto de Astronomía Teórica y Experimental; Argentina. Universidad Nacional de Cordoba. Observatorio Astronomico de Cordoba; Argentina
Fil: Valotto, Carlos Alberto. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Astronomía Teórica y Experimental. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Instituto de Astronomía Teórica y Experimental; Argentina. Universidad Nacional de Cordoba. Observatorio Astronomico de Cordoba; Argentina
Fil: O'Mill, Ana Laura. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Astronomía Teórica y Experimental. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Instituto de Astronomía Teórica y Experimental; Argentina. Universidad Nacional de Cordoba. Observatorio Astronomico de Cordoba; Argentina
Fil: Cuevas, Héctor. Universidad de La Serena; Chile
Fil: Carrasco, Eleazar Rodrigo. Gemini Observatory; Chile
Fil: Ramírez, Amelia. Universidad de La Serena; Chile
Fil: Astudillo, José M.. Universidad Andrés Bello; Chile
Fil: Ramos Almendares, Felipe Alberto. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Astronomía Teórica y Experimental. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Instituto de Astronomía Teórica y Experimental; Argentina
Fil: Jaque Arancibia, Marcelo Daniel. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - San Juan. Instituto de Ciencias Astronómicas, de la Tierra y del Espacio. Universidad Nacional de San Juan. Instituto de Ciencias Astronómicas, de la Tierra y del Espacio; Argentina
Fil: Ulloa, Natalie. Universidad de La Serena; Chile
Fil: Órdenes, Yasna. Universitat Bonn; Alemania - Materia
-
GALAXIES: CLUSTERS: GENERAL
GALAXIES: FUNDAMENTAL PARAMETERS
GALAXIES: PHOTOMETRY - Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
- Repositorio
.jpg)
- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/62686
Ver los metadatos del registro completo
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Low X-Ray Luminosity Galaxy Clusters: Main goals, sample selection, photometric and spectroscopic observationsNilo Castellon, Jose Luis EmilioAlonso, Maria VictoriaGarcia Lambas, Diego RodolfoValotto, Carlos AlbertoO'Mill, Ana LauraCuevas, HéctorCarrasco, Eleazar RodrigoRamírez, AmeliaAstudillo, José M.Ramos Almendares, Felipe AlbertoJaque Arancibia, Marcelo DanielUlloa, NatalieÓrdenes, YasnaGALAXIES: CLUSTERS: GENERALGALAXIES: FUNDAMENTAL PARAMETERSGALAXIES: PHOTOMETRYhttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1We present our study of 19 low X-ray luminosity galaxy clusters (L 0.5-45 × 1043 erg s-1), selected from the ROSAT Position Sensitive Proportional Counters Pointed Observations and the revised version of Mullis et al. in the redshift range of 0.16-0.7. This is the introductory paper of a series presenting the sample selection, photometric and spectroscopic observations, and data reduction. Photometric data in different passbands were taken for eight galaxy clusters at Las Campanas Observatory; three clusters at Cerro Tololo Interamerican Observatory; and eight clusters at the Gemini Observatory. Spectroscopic data were collected for only four galaxy clusters using Gemini telescopes. Using the photometry, the galaxies were defined based on the star-galaxy separation taking into account photometric parameters. For each galaxy cluster, the catalogs contain the point-spread function and aperture magnitudes of galaxies within the 90% completeness limit. They are used together with structural parameters to study the galaxy morphology and to estimate photometric redshifts. With the spectroscopy, the derived galaxy velocity dispersion of our clusters ranged from 507 km s-1 for [VMF98]022 to 775 km s-1 for [VMF98]097 with signs of substructure. Cluster membership has been extensively discussed taking into account spectroscopic and photometric redshift estimates. In this sense, members are the galaxies within a projected radius of 0.75 Mpc from the X-ray emission peak and with clustercentric velocities smaller than the cluster velocity dispersion or 6000 km s-1, respectively. These results will be used in forthcoming papers to study, among the main topics, the red cluster sequence, blue cloud and green populations, the galaxy luminosity function, and cluster dynamics.Fil: Nilo Castellon, Jose Luis Emilio. Universidad de La Serena; Chile. Consejo Nacional de Investigaciones Científicas y Técnicas; ArgentinaFil: Alonso, Maria Victoria. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Astronomía Teórica y Experimental. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Instituto de Astronomía Teórica y Experimental; Argentina. Universidad Nacional de Cordoba. Observatorio Astronomico de Cordoba; ArgentinaFil: Garcia Lambas, Diego Rodolfo. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Astronomía Teórica y Experimental. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Instituto de Astronomía Teórica y Experimental; Argentina. Universidad Nacional de Cordoba. Observatorio Astronomico de Cordoba; ArgentinaFil: Valotto, Carlos Alberto. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Astronomía Teórica y Experimental. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Instituto de Astronomía Teórica y Experimental; Argentina. Universidad Nacional de Cordoba. Observatorio Astronomico de Cordoba; ArgentinaFil: O'Mill, Ana Laura. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Astronomía Teórica y Experimental. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Instituto de Astronomía Teórica y Experimental; Argentina. Universidad Nacional de Cordoba. Observatorio Astronomico de Cordoba; ArgentinaFil: Cuevas, Héctor. Universidad de La Serena; ChileFil: Carrasco, Eleazar Rodrigo. Gemini Observatory; ChileFil: Ramírez, Amelia. Universidad de La Serena; ChileFil: Astudillo, José M.. Universidad Andrés Bello; ChileFil: Ramos Almendares, Felipe Alberto. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Astronomía Teórica y Experimental. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Instituto de Astronomía Teórica y Experimental; ArgentinaFil: Jaque Arancibia, Marcelo Daniel. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - San Juan. Instituto de Ciencias Astronómicas, de la Tierra y del Espacio. Universidad Nacional de San Juan. Instituto de Ciencias Astronómicas, de la Tierra y del Espacio; ArgentinaFil: Ulloa, Natalie. Universidad de La Serena; ChileFil: Órdenes, Yasna. Universitat Bonn; AlemaniaIOP Publishing2016-06info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfapplication/pdfapplication/pdfapplication/pdfapplication/pdfapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/62686Nilo Castellon, Jose Luis Emilio; Alonso, Maria Victoria; Garcia Lambas, Diego Rodolfo; Valotto, Carlos Alberto; O'Mill, Ana Laura; et al.; Low X-Ray Luminosity Galaxy Clusters: Main goals, sample selection, photometric and spectroscopic observations; IOP Publishing; Astronomical Journal; 151; 6; 6-2016; 151-1640004-6256CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/doi/10.3847/0004-6256/151/6/151info:eu-repo/semantics/altIdentifier/url/http://iopscience.iop.org/article/10.3847/0004-6256/151/6/151/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 Técnicas2025-09-29T09:59:48Zoai:ri.conicet.gov.ar:11336/62686instacron: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 09:59:48.487CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
| dc.title.none.fl_str_mv |
Low X-Ray Luminosity Galaxy Clusters: Main goals, sample selection, photometric and spectroscopic observations |
| title |
Low X-Ray Luminosity Galaxy Clusters: Main goals, sample selection, photometric and spectroscopic observations |
| spellingShingle |
Low X-Ray Luminosity Galaxy Clusters: Main goals, sample selection, photometric and spectroscopic observations Nilo Castellon, Jose Luis Emilio GALAXIES: CLUSTERS: GENERAL GALAXIES: FUNDAMENTAL PARAMETERS GALAXIES: PHOTOMETRY |
| title_short |
Low X-Ray Luminosity Galaxy Clusters: Main goals, sample selection, photometric and spectroscopic observations |
| title_full |
Low X-Ray Luminosity Galaxy Clusters: Main goals, sample selection, photometric and spectroscopic observations |
| title_fullStr |
Low X-Ray Luminosity Galaxy Clusters: Main goals, sample selection, photometric and spectroscopic observations |
| title_full_unstemmed |
Low X-Ray Luminosity Galaxy Clusters: Main goals, sample selection, photometric and spectroscopic observations |
| title_sort |
Low X-Ray Luminosity Galaxy Clusters: Main goals, sample selection, photometric and spectroscopic observations |
| dc.creator.none.fl_str_mv |
Nilo Castellon, Jose Luis Emilio Alonso, Maria Victoria Garcia Lambas, Diego Rodolfo Valotto, Carlos Alberto O'Mill, Ana Laura Cuevas, Héctor Carrasco, Eleazar Rodrigo Ramírez, Amelia Astudillo, José M. Ramos Almendares, Felipe Alberto Jaque Arancibia, Marcelo Daniel Ulloa, Natalie Órdenes, Yasna |
| author |
Nilo Castellon, Jose Luis Emilio |
| author_facet |
Nilo Castellon, Jose Luis Emilio Alonso, Maria Victoria Garcia Lambas, Diego Rodolfo Valotto, Carlos Alberto O'Mill, Ana Laura Cuevas, Héctor Carrasco, Eleazar Rodrigo Ramírez, Amelia Astudillo, José M. Ramos Almendares, Felipe Alberto Jaque Arancibia, Marcelo Daniel Ulloa, Natalie Órdenes, Yasna |
| author_role |
author |
| author2 |
Alonso, Maria Victoria Garcia Lambas, Diego Rodolfo Valotto, Carlos Alberto O'Mill, Ana Laura Cuevas, Héctor Carrasco, Eleazar Rodrigo Ramírez, Amelia Astudillo, José M. Ramos Almendares, Felipe Alberto Jaque Arancibia, Marcelo Daniel Ulloa, Natalie Órdenes, Yasna |
| author2_role |
author author author author author author author author author author author author |
| dc.subject.none.fl_str_mv |
GALAXIES: CLUSTERS: GENERAL GALAXIES: FUNDAMENTAL PARAMETERS GALAXIES: PHOTOMETRY |
| topic |
GALAXIES: CLUSTERS: GENERAL GALAXIES: FUNDAMENTAL PARAMETERS GALAXIES: PHOTOMETRY |
| 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 our study of 19 low X-ray luminosity galaxy clusters (L 0.5-45 × 1043 erg s-1), selected from the ROSAT Position Sensitive Proportional Counters Pointed Observations and the revised version of Mullis et al. in the redshift range of 0.16-0.7. This is the introductory paper of a series presenting the sample selection, photometric and spectroscopic observations, and data reduction. Photometric data in different passbands were taken for eight galaxy clusters at Las Campanas Observatory; three clusters at Cerro Tololo Interamerican Observatory; and eight clusters at the Gemini Observatory. Spectroscopic data were collected for only four galaxy clusters using Gemini telescopes. Using the photometry, the galaxies were defined based on the star-galaxy separation taking into account photometric parameters. For each galaxy cluster, the catalogs contain the point-spread function and aperture magnitudes of galaxies within the 90% completeness limit. They are used together with structural parameters to study the galaxy morphology and to estimate photometric redshifts. With the spectroscopy, the derived galaxy velocity dispersion of our clusters ranged from 507 km s-1 for [VMF98]022 to 775 km s-1 for [VMF98]097 with signs of substructure. Cluster membership has been extensively discussed taking into account spectroscopic and photometric redshift estimates. In this sense, members are the galaxies within a projected radius of 0.75 Mpc from the X-ray emission peak and with clustercentric velocities smaller than the cluster velocity dispersion or 6000 km s-1, respectively. These results will be used in forthcoming papers to study, among the main topics, the red cluster sequence, blue cloud and green populations, the galaxy luminosity function, and cluster dynamics. Fil: Nilo Castellon, Jose Luis Emilio. Universidad de La Serena; Chile. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina Fil: Alonso, Maria Victoria. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Astronomía Teórica y Experimental. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Instituto de Astronomía Teórica y Experimental; Argentina. Universidad Nacional de Cordoba. Observatorio Astronomico de Cordoba; Argentina Fil: Garcia Lambas, Diego Rodolfo. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Astronomía Teórica y Experimental. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Instituto de Astronomía Teórica y Experimental; Argentina. Universidad Nacional de Cordoba. Observatorio Astronomico de Cordoba; Argentina Fil: Valotto, Carlos Alberto. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Astronomía Teórica y Experimental. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Instituto de Astronomía Teórica y Experimental; Argentina. Universidad Nacional de Cordoba. Observatorio Astronomico de Cordoba; Argentina Fil: O'Mill, Ana Laura. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Astronomía Teórica y Experimental. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Instituto de Astronomía Teórica y Experimental; Argentina. Universidad Nacional de Cordoba. Observatorio Astronomico de Cordoba; Argentina Fil: Cuevas, Héctor. Universidad de La Serena; Chile Fil: Carrasco, Eleazar Rodrigo. Gemini Observatory; Chile Fil: Ramírez, Amelia. Universidad de La Serena; Chile Fil: Astudillo, José M.. Universidad Andrés Bello; Chile Fil: Ramos Almendares, Felipe Alberto. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Astronomía Teórica y Experimental. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Instituto de Astronomía Teórica y Experimental; Argentina Fil: Jaque Arancibia, Marcelo Daniel. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - San Juan. Instituto de Ciencias Astronómicas, de la Tierra y del Espacio. Universidad Nacional de San Juan. Instituto de Ciencias Astronómicas, de la Tierra y del Espacio; Argentina Fil: Ulloa, Natalie. Universidad de La Serena; Chile Fil: Órdenes, Yasna. Universitat Bonn; Alemania |
| description |
We present our study of 19 low X-ray luminosity galaxy clusters (L 0.5-45 × 1043 erg s-1), selected from the ROSAT Position Sensitive Proportional Counters Pointed Observations and the revised version of Mullis et al. in the redshift range of 0.16-0.7. This is the introductory paper of a series presenting the sample selection, photometric and spectroscopic observations, and data reduction. Photometric data in different passbands were taken for eight galaxy clusters at Las Campanas Observatory; three clusters at Cerro Tololo Interamerican Observatory; and eight clusters at the Gemini Observatory. Spectroscopic data were collected for only four galaxy clusters using Gemini telescopes. Using the photometry, the galaxies were defined based on the star-galaxy separation taking into account photometric parameters. For each galaxy cluster, the catalogs contain the point-spread function and aperture magnitudes of galaxies within the 90% completeness limit. They are used together with structural parameters to study the galaxy morphology and to estimate photometric redshifts. With the spectroscopy, the derived galaxy velocity dispersion of our clusters ranged from 507 km s-1 for [VMF98]022 to 775 km s-1 for [VMF98]097 with signs of substructure. Cluster membership has been extensively discussed taking into account spectroscopic and photometric redshift estimates. In this sense, members are the galaxies within a projected radius of 0.75 Mpc from the X-ray emission peak and with clustercentric velocities smaller than the cluster velocity dispersion or 6000 km s-1, respectively. These results will be used in forthcoming papers to study, among the main topics, the red cluster sequence, blue cloud and green populations, the galaxy luminosity function, and cluster dynamics. |
| publishDate |
2016 |
| dc.date.none.fl_str_mv |
2016-06 |
| 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/11336/62686 Nilo Castellon, Jose Luis Emilio; Alonso, Maria Victoria; Garcia Lambas, Diego Rodolfo; Valotto, Carlos Alberto; O'Mill, Ana Laura; et al.; Low X-Ray Luminosity Galaxy Clusters: Main goals, sample selection, photometric and spectroscopic observations; IOP Publishing; Astronomical Journal; 151; 6; 6-2016; 151-164 0004-6256 CONICET Digital CONICET |
| url |
http://hdl.handle.net/11336/62686 |
| identifier_str_mv |
Nilo Castellon, Jose Luis Emilio; Alonso, Maria Victoria; Garcia Lambas, Diego Rodolfo; Valotto, Carlos Alberto; O'Mill, Ana Laura; et al.; Low X-Ray Luminosity Galaxy Clusters: Main goals, sample selection, photometric and spectroscopic observations; IOP Publishing; Astronomical Journal; 151; 6; 6-2016; 151-164 0004-6256 CONICET Digital CONICET |
| dc.language.none.fl_str_mv |
eng |
| language |
eng |
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info:eu-repo/semantics/altIdentifier/doi/10.3847/0004-6256/151/6/151 info:eu-repo/semantics/altIdentifier/url/http://iopscience.iop.org/article/10.3847/0004-6256/151/6/151/meta |
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info:eu-repo/semantics/openAccess https://creativecommons.org/licenses/by-nc-sa/2.5/ar/ |
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openAccess |
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https://creativecommons.org/licenses/by-nc-sa/2.5/ar/ |
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IOP Publishing |
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IOP Publishing |
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dasensio@conicet.gov.ar; lcarlino@conicet.gov.ar |
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