Dataciencia

Colección SciELO Chile

VALES - III. The calibration between the dust continuum and interstellar gas content of star-forming galaxies

Indexado

WoS	WOS:000410066800022
Scopus	SCOPUS_ID:85030477474

DOI

10.1093/MNRASL/SLX033

Año

2017

Tipo

artículo de investigación

Citas Totales

Autores Afiliación Chile

Instituciones Chile

% Participación
Internacional

Autores
Afiliación Extranjera

Instituciones
Extranjeras

Abstract

We present the calibration between the dust continuum luminosity and interstellar gas content obtained from the Valparaiso ALMA Line Emission Survey (VALES) sample of 67 main-sequence star-forming galaxies at 0.02 < z < 0.35. We use CO(1-0) observations from the Atacama Large Millimetre/submillimetre Array to trace the molecular gas mass, M-H2, and estimate the rest-frame monochromatic luminosity at 850 mu m, L-nu 850, by extrapolating the dust continuum from MAGPHYS modelling of the far-ultraviolet to submillimetre spectral energy distribution sampled by the Galaxy And Mass Assembly survey. Adopting alpha(CO) = 6.5 (K km s(-1) pc(2))(-1), the average ratio of L-nu 850/M-H2 = (6.4 +/- 1.4) x 10(19) erg s(-1) Hz(-1) M-circle dot(-1), in excellent agreement with literature values. We obtain a linear fit of log(10) (M-H2/M-circle dot) = (0.92 +/- 0.02) log(10)(L-nu 850/erg s(-1) Hz(-1)) - (17.31 +/- 0.59). We provide relations between L-nu 850, M-H2 and M-ISM when combining the VALES and literature samples, and adopting a Galactic alpha(CO) value.

Revista

Revista	ISSN
Monthly Notices Of The Royal Astronomical Society: Letters	1745-3925

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Disciplinas de Investigación

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Scopus
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SciELO
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Publicaciones WoS (Ediciones: ISSHP, ISTP, AHCI, SSCI, SCI), Scopus, SciELO Chile.

Colaboración Institucional

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Autores - Afiliación

Ord.	Autor	Género	Institución - País
1	Hughes, Thomas M.	Hombre	Universidad de Valparaíso - Chile
2	IBAR-PLASSER, EDUARDO	Hombre	Universidad de Valparaíso - Chile
3	Villanueva, Vicente	Hombre	Universidad de Valparaíso - Chile
4	ARAVENA-PASTEN, MONICA	Hombre	Universidad Diego Portales - Chile
5	Baes, Maarten	Hombre	Univ Ghent - Bélgica Universiteit Gent - Bélgica
6	Bourne, N.	Hombre	UNIV EDINBURGH - Reino Unido University of Edinburgh, Institute for Astronomy - Reino Unido Cardiff University - Reino Unido
7	Cooray, A.	-	Univ Calif Irvine - Estados Unidos University of California, Irvine - Estados Unidos
8	Davies, L.	Hombre	Univ Western Australia - Australia University of Western Australia - Australia The University of Western Australia - Australia
9	Driver, S.	Hombre	Univ Western Australia - Australia Univ St Andrews - Reino Unido University of Western Australia - Australia University of St Andrews - Reino Unido The University of Western Australia - Australia
10	Bourne, N.	Hombre	UNIV EDINBURGH - Reino Unido University of Edinburgh, Institute for Astronomy - Reino Unido Cardiff University - Reino Unido
10	Dunne, L.	Mujer	UNIV EDINBURGH - Reino Unido Cardiff Univ - Reino Unido University of Edinburgh, Institute for Astronomy - Reino Unido Cardiff University - Reino Unido
11	Dye, Simon	Hombre	Univ Nottingham - Reino Unido University of Nottingham - Reino Unido
12	Eales, Stephen A.	Hombre	Cardiff Univ - Reino Unido Cardiff University - Reino Unido
13	Furlanetto, Cristina	Mujer	Univ Nottingham - Reino Unido Minist Educ Brazil - Brasil University of Nottingham - Reino Unido Ministry of Education Brazil - Brasil Coordenação de Aperfeiçoamento de Pessoal de Nível Superior, Brazil - Brasil
14	Herrera-Camus, Rodrigo	Hombre	Max Planck Inst Extraterr Phys - Alemania Max Planck Institute for Extraterrestrial Physics - Alemania
15	Ivison, R. J.	Hombre	UNIV EDINBURGH - Reino Unido ESO - Alemania University of Edinburgh, Institute for Astronomy - Reino Unido Observatorio Europeo Austral - Alemania
16	van Kampen, Eelco	Hombre	ESO - Alemania Observatorio Europeo Austral - Alemania
17	LARA-LOPEZ, MARITZA ARLENE	Mujer	Univ Nacl Autonoma Mexico - México Universidad Nacional Autónoma de México - México
18	Maddox, S. J.	Hombre	UNIV EDINBURGH - Reino Unido Cardiff Univ - Reino Unido University of Edinburgh, Institute for Astronomy - Reino Unido Cardiff University - Reino Unido
19	Michalowski, Michal J.	Hombre	UNIV EDINBURGH - Reino Unido University of Edinburgh, Institute for Astronomy - Reino Unido
20	Oteo, Ivan	Hombre	UNIV EDINBURGH - Reino Unido ESO - Alemania University of Edinburgh, Institute for Astronomy - Reino Unido Observatorio Europeo Austral - Alemania
21	Smith, D.	-	UNIV EDINBURGH - Reino Unido Univ Hertfordshire - Reino Unido University of Hertfordshire - Reino Unido
21	Smith, Daniel J. B.	Hombre	University of Hertfordshire - Reino Unido
22	Smith, Matthew	Hombre	Cardiff Univ - Reino Unido Cardiff University - Reino Unido
23	Valiante, E.	Mujer	Cardiff Univ - Reino Unido Cardiff University - Reino Unido
24	van der Werf, Paul P.	Hombre	Leiden Univ - Países Bajos Leiden Observatory Research Institute - Países Bajos Sterrewacht Leiden - Países Bajos
25	Viaene, Sebastien	Hombre	Univ Ghent - Bélgica Univ Hertfordshire - Reino Unido Universiteit Gent - Bélgica University of Hertfordshire - Reino Unido
26	Xue, Yongquan	-	Univ Sci & Technol China - China University of Science and Technology of China - China

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Citas identificadas: Las citas provienen de documentos incluidos en la base de datos de DATACIENCIA

Citas Identificadas: 12.12 %
Citas No-identificadas: 87.88 %

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Citas identificadas: Las citas provienen de documentos incluidos en la base de datos de DATACIENCIA

Citas Identificadas: 12.12 %
Citas No-identificadas: 87.88 %

Financiamiento

Fuente
FONDECYT
National Natural Science Foundation of China
National Science Foundation
European Research Council
Seventh Framework Programme
STFC (UK)
AAO
ARC (Australia)
European Research Council Consolidator Grant COSMICDUST
European Research Council Advanced Investigator Grant COSMICISM
CONICYT/ALMA

Muestra la fuente de financiamiento declarada en la publicación.

Agradecimientos

Agradecimiento
TMH and EI acknowledge CONICYT/ALMA funding Program in Astronomy/PCI Project No: 31140020. MA acknowledges partial support from FONDECYT through grant 1140099. DR acknowledges support from the National Science Foundation under grant number AST-1614213 to the Cornell University. LD, SJM and RJI acknowledge support from European Research Council Advanced Investigator Grant COSMICISM, 321302; SJM and LD are also supported by the European Research Council Consolidator Grant COSMICDUST (ERC-2014-CoG-647939). YQX acknowledges support from grants NSFC-11473026 and NSFC-11421303. This paper uses the following ALMA data: ADS/JAO.ALMA #2012.1.01080.S andjk #2013.1.00530.S. ALMA is a partnership of ESO (representing its member states), NSF (USA) and NINS (Japan), together with NRC (Canada), NSC and ASIAA (Taiwan), and KASI (Republic of Korea), in cooperation with the Republic of Chile. The Joint ALMA Observatory is operated by ESO, AUI/NRAO and NAOJ.
GAMA is a joint European-Australasian project based around a spectroscopic campaign using the Anglo-Australian Telescope. The GAMA input catalogue is based on data taken from the Sloan Digital Sky Survey and the UKIRT Infrared Deep Sky Survey. Complementary imaging of the GAMA regions is being obtained by a number of independent survey programmes includingGALEXMIS, VST KiDS, VISTA VIKING, WISE, Herschel-ATLAS, GMRT and ASKAP providing UV to radio coverage. GAMA is funded by the STFC (UK), the ARC (Australia), the AAO, and the participating institutions. The GAMA website is http://www.gama-survey.org/. TMH and EI acknowledge CONICYT/ALMA funding Program in Astronomy/PCI Project No:31140020. MA acknowledges partial support from FONDECYT through grant 1140099. DR acknowledges support from the National Science Foundation under grant number AST-1614213 to the Cornell University. LD, SJM and RJI acknowledge support from European Research Council Advanced Investigator Grant COSMICISM, 321302; SJM and LD are also supported by the European Research Council Consolidator Grant COSMICDUST (ERC-2014-CoG-647939). YQX acknowledges support from grants NSFC-11473026 and NSFC-11421303. This paper uses the followingALMAdata: ADS/JAO.ALMA #2012.1.01080.S andjk #2013.1.00530.S. ALMA is a partnership of ESO (representing its member states), NSF (USA) and NINS (Japan), together with NRC (Canada), NSC and ASIAA (Taiwan), and KASI (Republic of Korea), in cooperation with the Republic of Chile. The Joint ALMA Observatory is operated by ESO, AUI/NRAO and NAOJ.

Agradecimiento

TMH and EI acknowledge CONICYT/ALMA funding Program in Astronomy/PCI Project No: 31140020. MA acknowledges partial support from FONDECYT through grant 1140099. DR acknowledges support from the National Science Foundation under grant number AST-1614213 to the Cornell University. LD, SJM and RJI acknowledge support from European Research Council Advanced Investigator Grant COSMICISM, 321302; SJM and LD are also supported by the European Research Council Consolidator Grant COSMICDUST (ERC-2014-CoG-647939). YQX acknowledges support from grants NSFC-11473026 and NSFC-11421303. This paper uses the following ALMA data: ADS/JAO.ALMA #2012.1.01080.S andjk #2013.1.00530.S. ALMA is a partnership of ESO (representing its member states), NSF (USA) and NINS (Japan), together with NRC (Canada), NSC and ASIAA (Taiwan), and KASI (Republic of Korea), in cooperation with the Republic of Chile. The Joint ALMA Observatory is operated by ESO, AUI/NRAO and NAOJ.

GAMA is a joint European-Australasian project based around a spectroscopic campaign using the Anglo-Australian Telescope. The GAMA input catalogue is based on data taken from the Sloan Digital Sky Survey and the UKIRT Infrared Deep Sky Survey. Complementary imaging of the GAMA regions is being obtained by a number of independent survey programmes includingGALEXMIS, VST KiDS, VISTA VIKING, WISE, Herschel-ATLAS, GMRT and ASKAP providing UV to radio coverage. GAMA is funded by the STFC (UK), the ARC (Australia), the AAO, and the participating institutions. The GAMA website is http://www.gama-survey.org/. TMH and EI acknowledge CONICYT/ALMA funding Program in Astronomy/PCI Project No:31140020. MA acknowledges partial support from FONDECYT through grant 1140099. DR acknowledges support from the National Science Foundation under grant number AST-1614213 to the Cornell University. LD, SJM and RJI acknowledge support from European Research Council Advanced Investigator Grant COSMICISM, 321302; SJM and LD are also supported by the European Research Council Consolidator Grant COSMICDUST (ERC-2014-CoG-647939). YQX acknowledges support from grants NSFC-11473026 and NSFC-11421303. This paper uses the followingALMAdata: ADS/JAO.ALMA #2012.1.01080.S andjk #2013.1.00530.S. ALMA is a partnership of ESO (representing its member states), NSF (USA) and NINS (Japan), together with NRC (Canada), NSC and ASIAA (Taiwan), and KASI (Republic of Korea), in cooperation with the Republic of Chile. The Joint ALMA Observatory is operated by ESO, AUI/NRAO and NAOJ.

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Abstract

Revista

Métricas Externas

Disciplinas de Investigación

Colaboración Institucional

Autores - Afiliación

Origen de Citas Identificadas

Financiamiento

Agradecimientos

Departamento Gestión de Conocimiento, Monitoreo y Prospección