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| DOI | 10.1051/0004-6361/201526023 | ||||
| Año | 2015 | ||||
| Tipo | artículo de investigación |
Citas Totales
Autores Afiliación Chile
Instituciones Chile
% Participación
Internacional
Autores
Afiliación Extranjera
Instituciones
Extranjeras
Conclusions. In the local Universe, the H alpha luminosity derived from IFS observations can be used to measure SFR, at least in statistically-significant, optically-selected galaxy samples, once stellar continuum absorption and dust attenuation effects are accounted for. The analysis of the SFR calibrations by galaxies properties could potentially be used by other works to study the impact of different selection criteria in the SFR values derived, and to disentangle selection effects from other physically motivated differences, such as environmental or evolutionary effects.
| Ord. | Autor | Género | Institución - País |
|---|---|---|---|
| 1 | Catalan-Torrecilla, C. | - |
UNIV COMPLUTENSE MADRID - España
Universidad Complutense de Madrid - España |
| 2 | Gil de Paz, A. | Hombre |
UNIV COMPLUTENSE MADRID - España
Universidad Complutense de Madrid - España |
| 3 | CASTILLO-MORALES, MARIA AFRICA | Mujer |
UNIV COMPLUTENSE MADRID - España
Universidad Complutense de Madrid - España |
| 4 | Iglesias-Paramo, J. | Hombre |
CSIC - España
Instituto de Astrofísica de Andalucía - CSIC - España CSIC - Estación Experimental de Zonas Áridas (EEZA) - España CSIC - Estación Experimental de Zonas Áridas (EEZA) - España |
| 5 | SANCHEZ-SANCHEZ, SEBASTIAN FRANCISCO | Hombre |
Univ Nacl Autonoma Mexico - México
Universidad Nacional Autónoma de México - México |
| 6 | Kennicutt, R. C. | Hombre |
UNIV CAMBRIDGE - Reino Unido
Institute of Astronomy - Reino Unido |
| 7 | GONZALEZ-VILLARROEL, PABLO EMILIO | Hombre |
UNIV COMPLUTENSE MADRID - España
Universidad Complutense de Madrid - España |
| 8 | Marino, R. A. | Mujer |
UNIV COMPLUTENSE MADRID - España
Universidad Complutense de Madrid - España |
| 9 | Walcher, C. J. | - |
Leibniz Inst Astrophys Potsdam AIP - Alemania
Leibniz Institute for Astrophysics Potsdam - Alemania |
| 10 | Husemann, Bernd | Hombre |
ESO - Alemania
Observatorio Europeo Austral - Alemania |
| 11 | Garciá-Benito, R. | Hombre |
CSIC - España
Instituto de Astrofísica de Andalucía - CSIC - España |
| 12 | Mast, D. | Hombre |
Ctr Brasileiro Pesquisas Fis - Brasil
Centro Brasileiro de Pesquisas Físicas - Brasil |
| 13 | Gonzalez Delgado, R. | - |
CSIC - España
Instituto de Astrofísica de Andalucía - CSIC - España |
| 14 | Muñoz-Mateos, Juan Carlos | Hombre |
ESO - Chile
European Southern Observatory Santiago - Chile Observatorio Europeo Austral - Chile |
| 15 | Bryant, Julia J. | Mujer |
UNIV SYDNEY - Australia
The University of Sydney - Australia |
| 16 | Bomans, D. | - |
Ruhr Univ Bochum - Alemania
Ruhr-Universität Bochum - Alemania |
| 17 | del Olmo, A. | Mujer |
CSIC - España
Instituto de Astrofísica de Andalucía - CSIC - España |
| 18 | Frohmaier, C. | Hombre |
Universidad de Chile - Chile
|
| 19 | Gomes, J. M. | - |
Univ Porto - Portugal
Universidade do Porto, Centro de Astrofísica - Portugal Centro de Astrofísica da Universidade do Porto - Portugal |
| 20 | Kehrig, C. | Mujer |
CSIC - España
Instituto de Astrofísica de Andalucía - CSIC - España |
| 21 | Lopez-Sanchez, Angel R. | Hombre |
Australian Astron Observ - Australia
Macquarie Univ - Australia Australian Astronomical Observatory - Australia Macquarie University - Australia |
| 22 | Mendoza, M. A. | - |
CSIC - España
Instituto de Astrofísica de Andalucía - CSIC - España |
| 23 | Monreal-Ibero, A. | - |
Univ Paris Diderot - Francia
GEPI - Galaxies, Etoiles, Physique, Instrumentation - Francia |
| 24 | PEREZ-TORRES, MIGUEL ANGEL | Hombre |
CSIC - España
CEFCA - España Instituto de Astrofísica de Andalucía - CSIC - España Centro de Estudios de Física Del Cosmos de Aragón - España |
| 25 | SANCHEZ-BLAZQUEZ, PATRICIA | Mujer |
UNIV AUTONOMA MADRID - España
Universidad Autónoma de Madrid - España |
| 26 | VILCHEZ-MEDINA, JOSE MANUEL | Hombre |
CSIC - España
Instituto de Astrofísica de Andalucía - CSIC - España |
| 27 | CALIFA Collaboration | Corporación |
| Fuente |
|---|
| National Science Foundation |
| Ministerio de Economía, Fomento y Turismo |
| Fundação para a Ciência e a Tecnologia |
| FCT |
| Ministerio de Economía y Competitividad |
| Fondo Nacional de Desarrollo Científico y Tecnológico |
| Comisión Nacional de Investigación Científica y Tecnológica |
| Ministerio de Educación, Cultura y Deporte |
| U.S. Department of Energy |
| Science and Technology Facilities Council |
| National Aeronautics and Space Administration |
| Spanish MINECO |
| Alfred P. Sloan Foundation |
| Max-Planck-Gesellschaft |
| Spanish grant |
| Ministry of Economy, Development, and Tourism's Millennium Science Initiative |
| Conicyt through Fondecyt |
| Higher Education Funding Council for England |
| FPU |
| Spanish Ministerio de Economia y Competitividad (MINECO) |
| Programa Operacional Temático Factores de Competitividade |
| Junta de Andalucia Excellence Project |
| FCT-MEC (PIDDAC) |
| FEDER (COMPETE) |
| Millennium Institute of Astrophysics, MAS |
| FCT-MEC |
| Plan Nacional de Investigación y Desarrollo |
| Spanish program of International Campus of Excellence Moncloa |
| POPH/FSE by FEDER through program Programa Operacional de Factores de Competitividade (COMPETE) |
| Plan Nacional de Investigacion y Desarrollo funding programs |
| Fundacao para a Ciencia e a Tecnologia (FCT) from FCT (Portugal) |
| Junta de Andalucia Excellence |
| Fundació Catalana de Trasplantament |
| Agradecimiento |
|---|
| The Participating Institutions are the American Museum of Natural History, Astrophysical Institute Potsdam, University of Basel, University of Cambridge, Case Western Reserve University, University of Chicago, Drexel University, Fermilab, the Institute for Advanced Study, the Japan Participation Group, Johns Hopkins University, the Joint Institute for Nuclear Astrophysics, the Kavli Institute for Particle Astrophysics and Cosmology, the Korean Scientist Group, the Chinese Academy of Sciences (LAMOST), Los Alamos National Laboratory, the Max-Planck-Institute for Astronomy (MPIA), the Max-Planck-Institute for Astrophysics (MPA), New Mexico State University, Ohio State University, University of Pittsburgh, University of Portsmouth, Princeton University, the US Naval Observatory, and the University of Washington. GALEX (Galaxy Evolution Explorer) is a NASA Small Explorer, launched in April 2003. We gratefully acknowledge NASA's support for construction, operation, and science analysis for the GALEX mission, developed in cooperation with the Centre National d'Etudes Spatiales (CNES) of France and the Korean Ministry of Science and Technology. |
| This study makes uses of the data provided by the Calar Alto Legacy Integral Field Area (CALIFA) survey ( http://califa.caha.es ). CALIFA is the first legacy survey being performed at Calar Alto. The CALIFA collaboration would like to thank the IAA-CSIC and MPIA-MPG as major partners of the observatory, and CAHA itself, for the unique access to telescope time and support in manpower and infrastructures. The CALIFA collaboration also thanks the CAHA staff for the dedication to this project. C.C.-T. thanks the support of the Spanish Ministerio de Educación, Cultura y Deporte by means of the FPU fellowship program. The authors also thank the support from the Plan Nacional de Investigación y Desarrollo funding programs, AYA2012-30717 and AyA2013-46724P, of Spanish Ministerio de Economía y Competitividad (MINECO). P.G.P.-G. acknowledges support from the AYA2012-30717 and AYA2012-31277. J.I.P. acknowledges financial support from the Spanish MINECO under grant AYA2010-21887-C04-01 and from Junta de Andalucía Excellence Project PEX2011-FQM7058. R.A.M. is funded by the Spanish program of International Campus of Excellence Moncloa (CEI). M.A.P.T. acknowledges support from the Spanish MINECO through grant AYA2012-38491-C02-02. A.d.O. acknowledge financial support from the Spanish grant AYA2013-42227-P. Support for L.G. is provided by the Ministry of Economy, Development, and Tourism’s Millennium Science Initiative through grant IC120009, awarded to The Millennium Institute of Astrophysics, MAS. L.G. acknowledges support by CONICYT through FONDECYT grant 3140566. J.M.G. acknowledges support from the Fundação para a Ciência e a Tecnologia (FCT) through the Fellowship SFRH/BPD/66958/2009 from FCT (Portugal) and POPH/FSE (EC) by FEDER funding through the program Programa Operacional de Factores de Competitividade (COMPETE). J.M.G. also acknowledges support by FCT under project FCOMP-01-0124-FEDER-029170 (Reference FCT PTDC/FIS-AST/3214/2012), funded by FCT-MEC (PIDDAC) and FEDER (COMPETE). This research has made use of the NASA/IPAC Extragalactic Database (NED) which is operated by the Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space Administration. This publication makes use of data products from the Wide-field Infrared Survey Explorer, which is a joint project of the University of California, Los Angeles, and the Jet Propulsion Laboratory/California Institute of Technology, funded by the National Aeronautics and Space Administration. This research has made use of the NASA/ IPAC Infrared Science Archive, which is operated by the Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space Administration. Funding for the SDSS, and SDSS-II has been provided by the Alfred P. Sloan Foundation, the Participating Institutions, the National Science Foundation, the US Department of Energy, the National Aeronautics and Space Administration, the Japanese Monbukagakusho, the Max Planck Society, and the Higher Education Funding Council for England. The SDSS Web Site is http://www.sdss.org/ . The SDSS is managed by the Astrophysical Research Consortium for the Participating Institutions. The Participating Institutions are the American Museum of Natural History, Astrophysical Institute Potsdam, University of Basel, University of Cambridge, Case Western Reserve University, University of Chicago, Drexel University, Fermilab, the Institute for Advanced Study, the Japan Participation Group, Johns Hopkins University, the Joint Institute for Nuclear Astrophysics, the Kavli Institute for Particle Astrophysics and Cosmology, the Korean Scientist Group, the Chinese Academy of Sciences (LAMOST), Los Alamos National Laboratory, the Max-Planck-Institute for Astronomy (MPIA), the Max-Planck-Institute for Astrophysics (MPA), New Mexico State University, Ohio State University, University of Pittsburgh, University of Portsmouth, Princeton University, the US Naval Observatory, and the University of Washington. GALEX (Galaxy Evolution Explorer) is a NASA Small Explorer, launched in April 2003. We gratefully acknowledge NASA’s support forconstruction, operation, and science analysis for the GALEX mission, developed in cooperation with the Centre National d’Etudes Spatiales (CNES) of France and the Korean Ministry of Science and Technology. |