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The environmental dependence of the stellar mass function at z similar to 1 Comparing cluster and field between the GCLASS and UltraVISTA surveys
| Indexado |
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| DOI | 10.1051/0004-6361/201321237 | ||||
| Año | 2013 | ||||
| Tipo | artículo de investigación |
Citas Totales
Autores Afiliación Chile
Instituciones Chile
% Participación
Internacional
Autores
Afiliación Extranjera
Instituciones
Extranjeras
Abstract
Conclusions. If galaxies in clusters and the field quench their star formation via different mechanisms, these processes have to conspire in such a way that the shapes of the quiescent and star-forming SMF remain similar in these different environments.
| Ord. | Autor | Género | Institución - País |
|---|---|---|---|
| 1 | van der Burg, Remco | Hombre |
Leiden Univ - Países Bajos
Leiden Observatory Research Institute - Países Bajos Sterrewacht Leiden - Países Bajos |
| 2 | Muzzin, A. | Hombre |
Leiden Univ - Países Bajos
Leiden Observatory Research Institute - Países Bajos Sterrewacht Leiden - Países Bajos |
| 3 | Hoekstra, H. | Hombre |
Leiden Univ - Países Bajos
Leiden Observatory Research Institute - Países Bajos Sterrewacht Leiden - Países Bajos |
| 4 | Lidman, Chris | Hombre |
Australian Astron Observ - Australia
Australian Astronomical Observatory - Australia |
| 5 | Rettura, Alessando | Hombre |
CALTECH - Estados Unidos
California Institute of Technology - Estados Unidos |
| 6 | Wilson, G. | Mujer |
Univ Calif Riverside - Estados Unidos
University of California, Riverside - Estados Unidos |
| 7 | Yee, Howard K. C. | Hombre |
UNIV TORONTO - Canadá
University of Toronto - Canadá |
| 8 | Hildebrandt, Hendrik | Hombre |
UNIV BRITISH COLUMBIA - Canadá
Argelander Inst Astron - Alemania The University of British Columbia - Canadá Universität Bonn - Alemania |
| 9 | Marchesini, Danilo | Hombre |
Tufts Univ - Estados Unidos
Tufts University - Estados Unidos |
| 10 | Stefanon, Mauro | Hombre |
Univ Missouri - Estados Unidos
University of Missouri - Estados Unidos |
| 11 | DEMARCO-BULL, RODRIGO ANDRES | Hombre |
Universidad de Concepción - Chile
|
| 12 | Kuijken, K. | Hombre |
Leiden Univ - Países Bajos
Leiden Observatory Research Institute - Países Bajos Sterrewacht Leiden - Países Bajos |
| Fuente |
|---|
| FONDECYT |
| National Science Foundation |
| Comisión Nacional de Investigación Científica y Tecnológica |
| Australian Research Council |
| Deutsche Forschungsgemeinschaft |
| Ministerio de Ciencia, Tecnología e Innovación Productiva |
| DFG |
| NASA |
| National Research Council |
| Comisión Nacional de Investigación CientÃfica y Tecnológica |
| National Aeronautics and Space Administration |
| Fondo Nacional de Desarrollo Científico, Tecnológico y de Innovación Tecnológica |
| BASAL Center for Astrophysics and Associated Technologies (CATA) |
| Ministerio da Ciencia, Tecnologia e Inovacao |
| National Rehabilitation Center |
| Fondo Nacional de Desarrollo CientÃfico, Tecnológico y de Innovación Tecnológica |
| CFHT |
| Marie Curie |
| University of Hawai'i |
| JPL/Caltech |
| Ministerio de Ciencia, TecnologÃa e Innovación Productiva |
| Ministério da Ciência, Tecnologia e Inovação |
| Institut National des Sciences de l'Univers, Centre National de la Recherche Scientifique |
| Netherlands Organisation for Scientic Research |
| CITA National Fellowship |
| La Silla Paranal Observatories under ESO |
| Centre Eau Terre Environnement, Institut National de la Recherche Scientifique |
| Agradecimiento |
|---|
| We thank Gregory Rudnick, Marijn Franx and Simone Weinmann for discussions and helpful suggestions for this study. Further we thank Jean-Charles Cuillandre for providing information on the MegaCam amplifier drift problem, and Michael Balogh for general feedback on the paper draft. R. F. J. van der Burg and H. Hoekstra acknowledge support from the Netherlands Organisation for Scientic Research grant number 639.042.814. C. Lidman is the recipient of an Australian Research Council Future Fellowship (programme number FT0992259). H. Hildebrandt is supported by the Marie Curie IOF 252760, a CITA National Fellowship, and the DFG grant Hi 1495/2-1. R. D. gratefully acknowledges the support provided by the BASAL Center for Astrophysics and Associated Technologies (CATA), and by FONDECYT grant N. 1130528. Based on observations obtained at the Gemini Observatory, which is operated by the Association of Universities for Research in Astronomy, Inc., under a cooperative agreement with the NSF on behalf of the Gemini partnership: the National Science Foundation (United States), the National Research Council (Canada), CONICYT (Chile), the Australian Research Council (Australia), Ministerio da Ciencia, Tecnologia e Inovacao (Brazil) and Ministerio de Ciencia, Tecnologia e Innovacion Productiva (Argentina). Based on observations obtained with MegaPrime/MegaCam, a joint project of CFHT and CEA/DAPNIA, at the Canada-France-Hawaii Telescope (CFHT) which is operated by the National Research Council (NRC) of Canada, the Institute National des Sciences de l'Univers of the Centre National de la Recherche Scientifique of France, and the University of Hawaii. Based on observations obtained with WIRCam, a joint project of CFHT, Taiwan, Korea, Canada, France, and the Canada-FranceHawaii Telescope (CFHT) which is operated by the National Research Council (NRC) of Canada, the Institute National des Sciences de l'Univers of the Centre National de la Recherche Scientifique of France, and the University of Hawaii. This work is based in part on observations made with the Spitzer Space Telescope, which is operated by the Jet Propulsion Laboratory, California Institute of Technology under a contract with NASA. Support for this work was provided by NASA through an award issued by JPL/Caltech. This paper includes data gathered with the 6.5 m Magellan Telescopes located at Las Campanas Observatory, Chile. This work is based on observations obtained at the CTIO Blanco 4-m telescopes, which are operated by the Association of Universities for Research in Astronomy Inc. (AURA), under a cooperative agreement with the NSF as part of the National Optical Astronomy Observatories (NOAO). Based on observations that were carried out using the Very Large Telescope at the ESO Paranal Observatory. Based on data products from observations made with ESO Telescopes at the La Silla Paranal Observatories under ESO programme ID 179.A-2005 and on data products produced by TERAPIX and the Cambridge Astronomy Survey Unit on behalf of the UltraVISTA consortium. |
| We thank Gregory Rudnick, Marijn Franx and Simone Weinmann for discussions and helpful suggestions for this study. Further we thank Jean-Charles Cuillandre for providing information on the MegaCam amplifier drift problem, and Michael Balogh for general feedback on the paper draft. R. F. J. van der Burg and H. Hoekstra acknowledge support from the Netherlands Organisation for Scientic Research grant number 639.042.814. C. Lidman is the recipient of an Australian Research Council Future Fellowship (programme number FT0992259). H. Hildebrandt is supported by the Marie Curie IOF 252760, a CITA National Fellowship, and the DFG grant Hi 1495/2-1. R.D. gratefully acknowledges the support provided by the BASAL Center for Astrophysics and Associated Technologies (CATA), and by FONDECYT grant N. 1130528. Based on observations obtained at the Gemini Observatory, which is operated by the Association of Universities for Research in Astronomy, Inc., under a cooperative agreement with the NSF on behalf of the Gemini partnership: the National Science Foundation (United States), the National Research Council (Canada), CONICYT (Chile), the Australian Research Council (Australia), Ministério da Ciência, Tecnologia e Inovação (Brazil) and Ministerio de Ciencia, Tecnología e Innovación Productiva (Argentina). Based on observations obtained with MegaPrime/MegaCam, a joint project of CFHT and CEA/DAPNIA, at the Canada-France-Hawaii Telescope (CFHT) which is operated by the National Research Council (NRC) of Canada, the Institute National des Sciences de l’Univers of the Centre National de la Recherche Scientifique of France, and the University of Hawaii. Based on observations obtained with WIRCam, a joint project of CFHT, Taiwan, Korea, Canada, France, and the Canada-France-Hawaii Telescope (CFHT) which is operated by the National Research Council (NRC) of Canada, the Institute National des Sciences de l’Univers of the Centre National de la Recherche Scientifique of France, and the University of Hawaii. This work is based in part on observations made with the Spitzer Space Telescope, which is operated by the Jet Propulsion Laboratory, California Institute of Technology under a contract with NASA. Support for this work was provided by NASA through an award issued by JPL/Caltech. This paper includes data gathered with the 6.5 m Magellan Telescopes located at Las Campanas Observatory, Chile. This work is based on observations obtained at the CTIO Blanco 4-m telescopes, which are operated by the Association of Universities for Research in Astronomy Inc. (AURA), under a cooperative agreement with the NSF as part of the National Optical Astronomy Observatories (NOAO). Based on observations that were carried out using the Very Large Telescope at the ESO Paranal Observatory. Based on data products from observations made with ESO Telescopes at the La Silla Paranal Observatories under ESO programme ID 179.A-2005 and on data products produced by TERAPIX and the Cambridge Astronomy Survey Unit on behalf of the UltraVISTA consortium. |
