The EDGE-CALIFA Survey: Interferometric Observations of 126 Galaxies with CARMA
- Autores
- Bolatto, Alberto; Wong, Tony; Utomo, Dyas; Blitz, Leo; Vogel, Stuart N.; Sánchez, Sebastián F.; Barrera-Ballesteros, Jorge; Cao, Yixian; Colombo, Dario; Dannerbauer, Helmut; García-Benito, Rubén; Herrera-Camus, Rodrigo; Husemann, Bernd; Kalinova, Veselina; Leroy, Adam K.; Leung, Gigi; Levy, Rebecca C.; Mast, Damian; Ostriker, Eve; Rosolowsky, Erik; Sandstrom, Karin M.; Teuben, Peter; Van De Ven, Glenn; Walter, Fabian
- Año de publicación
- 2017
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- We present interferometric CO observations, made with the Combined Array for Millimeter-wave Astronomy (CARMA) interferometer, of galaxies from the Extragalactic Database for Galaxy Evolution survey (EDGE). These galaxies are selected from the Calar Alto Legacy Integral Field Area (CALIFA) sample, mapped with optical integral field spectroscopy. EDGE provides good-quality CO data (3σ sensitivity before inclination correction, resolution ∼1.4 kpc) for 126 galaxies, constituting the largest interferometric CO survey of galaxies in the nearby universe. We describe the survey and data characteristics and products, then present initial science results. We find that the exponential scale lengths of the molecular, stellar, and star-forming disks are approximately equal, and galaxies that are more compact in molecular gas than in stars tend to show signs of interaction. We characterize the molecular-to-stellar ratio as a function of Hubble type and stellar mass and present preliminary results on the resolved relations between the molecular gas, stars, and star-formation rate. We then discuss the dependence of the resolved molecular depletion time on stellar surface density, nebular extinction, and gas metallicity. EDGE provides a key data set to address outstanding topics regarding gas and its role in star formation and galaxy evolution, which will be publicly available on completion of the quality assessment.
Fil: Bolatto, Alberto. University of Maryland; Estados Unidos
Fil: Wong, Tony. University of Illinois at Urbana; Estados Unidos
Fil: Utomo, Dyas. University of California at Berkeley; Estados Unidos
Fil: Blitz, Leo. University of California at Berkeley; Estados Unidos
Fil: Vogel, Stuart N.. University of Maryland; Estados Unidos
Fil: Sánchez, Sebastián F.. Universidad Nacional Autónoma de México; México
Fil: Barrera-Ballesteros, Jorge. University Johns Hopkins; Estados Unidos
Fil: Cao, Yixian. University of Illinois; Estados Unidos
Fil: Colombo, Dario. Max Planck Institut Fur Radioastronomie; Alemania
Fil: Dannerbauer, Helmut. Universidad de La Laguna; España
Fil: García-Benito, Rubén. Instituto de Astrofísica de Andalucía; España
Fil: Herrera-Camus, Rodrigo. Max Planck Institute für Extraterrestrische Physik; Alemania
Fil: Husemann, Bernd. Max-Planck-Institut für Astronomie; Alemania
Fil: Kalinova, Veselina. Max Planck Institut für Radioastronomie; Alemania
Fil: Leroy, Adam K.. Ohio State University; Estados Unidos
Fil: Leung, Gigi. Max-Planck-Institut für Astronomie; Alemania
Fil: Levy, Rebecca C.. University of Maryland; Estados Unidos
Fil: Mast, Damian. Observatorio Astronomico de la Universidad Nacional de Cordoba; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba; Argentina
Fil: Ostriker, Eve. University of Princeton; Estados Unidos
Fil: Rosolowsky, Erik. University of Alberta; Canadá
Fil: Sandstrom, Karin M.. University of California at San Diego; Estados Unidos
Fil: Teuben, Peter. University of Maryland; Estados Unidos
Fil: Van De Ven, Glenn. Max-Planck-Institut für Astronomie; Alemania
Fil: Walter, Fabian. Max-Planck-Institut für Astronomie; Alemania - Materia
-
GALAXIES: EVOLUTION
GALAXIES: ISM
ISM: MOLECULES - 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:11336/79461
Ver los metadatos del registro completo
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The EDGE-CALIFA Survey: Interferometric Observations of 126 Galaxies with CARMABolatto, AlbertoWong, TonyUtomo, DyasBlitz, LeoVogel, Stuart N.Sánchez, Sebastián F.Barrera-Ballesteros, JorgeCao, YixianColombo, DarioDannerbauer, HelmutGarcía-Benito, RubénHerrera-Camus, RodrigoHusemann, BerndKalinova, VeselinaLeroy, Adam K.Leung, GigiLevy, Rebecca C.Mast, DamianOstriker, EveRosolowsky, ErikSandstrom, Karin M.Teuben, PeterVan De Ven, GlennWalter, FabianGALAXIES: EVOLUTIONGALAXIES: ISMISM: MOLECULEShttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1We present interferometric CO observations, made with the Combined Array for Millimeter-wave Astronomy (CARMA) interferometer, of galaxies from the Extragalactic Database for Galaxy Evolution survey (EDGE). These galaxies are selected from the Calar Alto Legacy Integral Field Area (CALIFA) sample, mapped with optical integral field spectroscopy. EDGE provides good-quality CO data (3σ sensitivity before inclination correction, resolution ∼1.4 kpc) for 126 galaxies, constituting the largest interferometric CO survey of galaxies in the nearby universe. We describe the survey and data characteristics and products, then present initial science results. We find that the exponential scale lengths of the molecular, stellar, and star-forming disks are approximately equal, and galaxies that are more compact in molecular gas than in stars tend to show signs of interaction. We characterize the molecular-to-stellar ratio as a function of Hubble type and stellar mass and present preliminary results on the resolved relations between the molecular gas, stars, and star-formation rate. We then discuss the dependence of the resolved molecular depletion time on stellar surface density, nebular extinction, and gas metallicity. EDGE provides a key data set to address outstanding topics regarding gas and its role in star formation and galaxy evolution, which will be publicly available on completion of the quality assessment.Fil: Bolatto, Alberto. University of Maryland; Estados UnidosFil: Wong, Tony. University of Illinois at Urbana; Estados UnidosFil: Utomo, Dyas. University of California at Berkeley; Estados UnidosFil: Blitz, Leo. University of California at Berkeley; Estados UnidosFil: Vogel, Stuart N.. University of Maryland; Estados UnidosFil: Sánchez, Sebastián F.. Universidad Nacional Autónoma de México; MéxicoFil: Barrera-Ballesteros, Jorge. University Johns Hopkins; Estados UnidosFil: Cao, Yixian. University of Illinois; Estados UnidosFil: Colombo, Dario. Max Planck Institut Fur Radioastronomie; AlemaniaFil: Dannerbauer, Helmut. Universidad de La Laguna; EspañaFil: García-Benito, Rubén. Instituto de Astrofísica de Andalucía; EspañaFil: Herrera-Camus, Rodrigo. Max Planck Institute für Extraterrestrische Physik; AlemaniaFil: Husemann, Bernd. Max-Planck-Institut für Astronomie; AlemaniaFil: Kalinova, Veselina. Max Planck Institut für Radioastronomie; AlemaniaFil: Leroy, Adam K.. Ohio State University; Estados UnidosFil: Leung, Gigi. Max-Planck-Institut für Astronomie; AlemaniaFil: Levy, Rebecca C.. University of Maryland; Estados UnidosFil: Mast, Damian. Observatorio Astronomico de la Universidad Nacional de Cordoba; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba; ArgentinaFil: Ostriker, Eve. University of Princeton; Estados UnidosFil: Rosolowsky, Erik. University of Alberta; CanadáFil: Sandstrom, Karin M.. University of California at San Diego; Estados UnidosFil: Teuben, Peter. University of Maryland; Estados UnidosFil: Van De Ven, Glenn. Max-Planck-Institut für Astronomie; AlemaniaFil: Walter, Fabian. Max-Planck-Institut für Astronomie; AlemaniaIOP Publishing2017-09info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/79461Bolatto, Alberto; Wong, Tony; Utomo, Dyas; Blitz, Leo; Vogel, Stuart N.; et al.; The EDGE-CALIFA Survey: Interferometric Observations of 126 Galaxies with CARMA; IOP Publishing; Astrophysical Journal; 846; 2; 9-20170004-637X1538-4357CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/doi/10.3847/1538-4357/aa86aainfo:eu-repo/semantics/altIdentifier/url/https://iopscience.iop.org/article/10.3847/1538-4357/aa86aainfo:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T10:29:10Zoai:ri.conicet.gov.ar:11336/79461instacron: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 10:29:11.088CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
| dc.title.none.fl_str_mv |
The EDGE-CALIFA Survey: Interferometric Observations of 126 Galaxies with CARMA |
| title |
The EDGE-CALIFA Survey: Interferometric Observations of 126 Galaxies with CARMA |
| spellingShingle |
The EDGE-CALIFA Survey: Interferometric Observations of 126 Galaxies with CARMA Bolatto, Alberto GALAXIES: EVOLUTION GALAXIES: ISM ISM: MOLECULES |
| title_short |
The EDGE-CALIFA Survey: Interferometric Observations of 126 Galaxies with CARMA |
| title_full |
The EDGE-CALIFA Survey: Interferometric Observations of 126 Galaxies with CARMA |
| title_fullStr |
The EDGE-CALIFA Survey: Interferometric Observations of 126 Galaxies with CARMA |
| title_full_unstemmed |
The EDGE-CALIFA Survey: Interferometric Observations of 126 Galaxies with CARMA |
| title_sort |
The EDGE-CALIFA Survey: Interferometric Observations of 126 Galaxies with CARMA |
| dc.creator.none.fl_str_mv |
Bolatto, Alberto Wong, Tony Utomo, Dyas Blitz, Leo Vogel, Stuart N. Sánchez, Sebastián F. Barrera-Ballesteros, Jorge Cao, Yixian Colombo, Dario Dannerbauer, Helmut García-Benito, Rubén Herrera-Camus, Rodrigo Husemann, Bernd Kalinova, Veselina Leroy, Adam K. Leung, Gigi Levy, Rebecca C. Mast, Damian Ostriker, Eve Rosolowsky, Erik Sandstrom, Karin M. Teuben, Peter Van De Ven, Glenn Walter, Fabian |
| author |
Bolatto, Alberto |
| author_facet |
Bolatto, Alberto Wong, Tony Utomo, Dyas Blitz, Leo Vogel, Stuart N. Sánchez, Sebastián F. Barrera-Ballesteros, Jorge Cao, Yixian Colombo, Dario Dannerbauer, Helmut García-Benito, Rubén Herrera-Camus, Rodrigo Husemann, Bernd Kalinova, Veselina Leroy, Adam K. Leung, Gigi Levy, Rebecca C. Mast, Damian Ostriker, Eve Rosolowsky, Erik Sandstrom, Karin M. Teuben, Peter Van De Ven, Glenn Walter, Fabian |
| author_role |
author |
| author2 |
Wong, Tony Utomo, Dyas Blitz, Leo Vogel, Stuart N. Sánchez, Sebastián F. Barrera-Ballesteros, Jorge Cao, Yixian Colombo, Dario Dannerbauer, Helmut García-Benito, Rubén Herrera-Camus, Rodrigo Husemann, Bernd Kalinova, Veselina Leroy, Adam K. Leung, Gigi Levy, Rebecca C. Mast, Damian Ostriker, Eve Rosolowsky, Erik Sandstrom, Karin M. Teuben, Peter Van De Ven, Glenn Walter, Fabian |
| 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 |
| dc.subject.none.fl_str_mv |
GALAXIES: EVOLUTION GALAXIES: ISM ISM: MOLECULES |
| topic |
GALAXIES: EVOLUTION GALAXIES: ISM ISM: MOLECULES |
| 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 interferometric CO observations, made with the Combined Array for Millimeter-wave Astronomy (CARMA) interferometer, of galaxies from the Extragalactic Database for Galaxy Evolution survey (EDGE). These galaxies are selected from the Calar Alto Legacy Integral Field Area (CALIFA) sample, mapped with optical integral field spectroscopy. EDGE provides good-quality CO data (3σ sensitivity before inclination correction, resolution ∼1.4 kpc) for 126 galaxies, constituting the largest interferometric CO survey of galaxies in the nearby universe. We describe the survey and data characteristics and products, then present initial science results. We find that the exponential scale lengths of the molecular, stellar, and star-forming disks are approximately equal, and galaxies that are more compact in molecular gas than in stars tend to show signs of interaction. We characterize the molecular-to-stellar ratio as a function of Hubble type and stellar mass and present preliminary results on the resolved relations between the molecular gas, stars, and star-formation rate. We then discuss the dependence of the resolved molecular depletion time on stellar surface density, nebular extinction, and gas metallicity. EDGE provides a key data set to address outstanding topics regarding gas and its role in star formation and galaxy evolution, which will be publicly available on completion of the quality assessment. Fil: Bolatto, Alberto. University of Maryland; Estados Unidos Fil: Wong, Tony. University of Illinois at Urbana; Estados Unidos Fil: Utomo, Dyas. University of California at Berkeley; Estados Unidos Fil: Blitz, Leo. University of California at Berkeley; Estados Unidos Fil: Vogel, Stuart N.. University of Maryland; Estados Unidos Fil: Sánchez, Sebastián F.. Universidad Nacional Autónoma de México; México Fil: Barrera-Ballesteros, Jorge. University Johns Hopkins; Estados Unidos Fil: Cao, Yixian. University of Illinois; Estados Unidos Fil: Colombo, Dario. Max Planck Institut Fur Radioastronomie; Alemania Fil: Dannerbauer, Helmut. Universidad de La Laguna; España Fil: García-Benito, Rubén. Instituto de Astrofísica de Andalucía; España Fil: Herrera-Camus, Rodrigo. Max Planck Institute für Extraterrestrische Physik; Alemania Fil: Husemann, Bernd. Max-Planck-Institut für Astronomie; Alemania Fil: Kalinova, Veselina. Max Planck Institut für Radioastronomie; Alemania Fil: Leroy, Adam K.. Ohio State University; Estados Unidos Fil: Leung, Gigi. Max-Planck-Institut für Astronomie; Alemania Fil: Levy, Rebecca C.. University of Maryland; Estados Unidos Fil: Mast, Damian. Observatorio Astronomico de la Universidad Nacional de Cordoba; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba; Argentina Fil: Ostriker, Eve. University of Princeton; Estados Unidos Fil: Rosolowsky, Erik. University of Alberta; Canadá Fil: Sandstrom, Karin M.. University of California at San Diego; Estados Unidos Fil: Teuben, Peter. University of Maryland; Estados Unidos Fil: Van De Ven, Glenn. Max-Planck-Institut für Astronomie; Alemania Fil: Walter, Fabian. Max-Planck-Institut für Astronomie; Alemania |
| description |
We present interferometric CO observations, made with the Combined Array for Millimeter-wave Astronomy (CARMA) interferometer, of galaxies from the Extragalactic Database for Galaxy Evolution survey (EDGE). These galaxies are selected from the Calar Alto Legacy Integral Field Area (CALIFA) sample, mapped with optical integral field spectroscopy. EDGE provides good-quality CO data (3σ sensitivity before inclination correction, resolution ∼1.4 kpc) for 126 galaxies, constituting the largest interferometric CO survey of galaxies in the nearby universe. We describe the survey and data characteristics and products, then present initial science results. We find that the exponential scale lengths of the molecular, stellar, and star-forming disks are approximately equal, and galaxies that are more compact in molecular gas than in stars tend to show signs of interaction. We characterize the molecular-to-stellar ratio as a function of Hubble type and stellar mass and present preliminary results on the resolved relations between the molecular gas, stars, and star-formation rate. We then discuss the dependence of the resolved molecular depletion time on stellar surface density, nebular extinction, and gas metallicity. EDGE provides a key data set to address outstanding topics regarding gas and its role in star formation and galaxy evolution, which will be publicly available on completion of the quality assessment. |
| publishDate |
2017 |
| dc.date.none.fl_str_mv |
2017-09 |
| 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/11336/79461 Bolatto, Alberto; Wong, Tony; Utomo, Dyas; Blitz, Leo; Vogel, Stuart N.; et al.; The EDGE-CALIFA Survey: Interferometric Observations of 126 Galaxies with CARMA; IOP Publishing; Astrophysical Journal; 846; 2; 9-2017 0004-637X 1538-4357 CONICET Digital CONICET |
| url |
http://hdl.handle.net/11336/79461 |
| identifier_str_mv |
Bolatto, Alberto; Wong, Tony; Utomo, Dyas; Blitz, Leo; Vogel, Stuart N.; et al.; The EDGE-CALIFA Survey: Interferometric Observations of 126 Galaxies with CARMA; IOP Publishing; Astrophysical Journal; 846; 2; 9-2017 0004-637X 1538-4357 CONICET Digital CONICET |
| dc.language.none.fl_str_mv |
eng |
| language |
eng |
| dc.relation.none.fl_str_mv |
info:eu-repo/semantics/altIdentifier/doi/10.3847/1538-4357/aa86aa info:eu-repo/semantics/altIdentifier/url/https://iopscience.iop.org/article/10.3847/1538-4357/aa86aa |
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openAccess |
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https://creativecommons.org/licenses/by-nc-sa/2.5/ar/ |
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application/pdf application/pdf |
| dc.publisher.none.fl_str_mv |
IOP Publishing |
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IOP Publishing |
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reponame:CONICET Digital (CONICET) instname:Consejo Nacional de Investigaciones Científicas y Técnicas |
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Consejo Nacional de Investigaciones Científicas y Técnicas |
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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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