Muestra métricas de impacto externas asociadas a la publicación. Para mayor detalle:
Departamento Gestión de Conocimiento, Monitoreo y Prospección
Consultas o comentarios: productividad@anid.cl
Consultas o comentarios: productividad@anid.cl
CLASH-VLT: The stellar mass function and stellar mass density profile of the z=0.44 cluster of galaxies MACS J1206.2-0847
| Indexado |
|
||||
| DOI | 10.1051/0004-6361/201424102 | ||||
| Año | 2014 | ||||
| Tipo | artículo de investigación |
Citas Totales
Autores Afiliación Chile
Instituciones Chile
% Participación
Internacional
Autores
Afiliación Extranjera
Instituciones
Extranjeras
Abstract
Conclusions. Our results appear consistent with a scenario in which SF galaxies evolve into passive galaxies due to density-dependent environmental processes and eventually get destroyed very near the cluster center to become part of a diffuse intracluster medium. Dynamical friction, on the other hand, does not seem to play an important role. Future investigations of other clusters of the CLASH-VLT sample will allow us to confirm our interpretation.
| Ord. | Autor | Género | Institución - País |
|---|---|---|---|
| 1 | Annunziatella, M. | Mujer |
UNIV TRIESTE - Italia
Osserv Astron Trieste - Italia Università degli Studi di Trieste - Italia Osservatorio Astronomico di Trieste - Italia |
| 2 | Biviano, A. | Mujer |
Osserv Astron Trieste - Italia
Osservatorio Astronomico di Trieste - Italia |
| 3 | Mercurio, A. | Mujer |
Osserv Astron Capodimonte - Italia
Osservatorio Astronomico di Capodimonte - Italia |
| 4 | Nonino, M. | Hombre |
Osserv Astron Trieste - Italia
Osservatorio Astronomico di Trieste - Italia |
| 5 | Rosati, P. | Hombre |
Univ Ferrara - Italia
University of Ferrara - Italia |
| 6 | Balestra, I. | Hombre |
Osserv Astron Trieste - Italia
Osservatorio Astronomico di Trieste - Italia |
| 7 | Presotto, V. | - |
UNIV TRIESTE - Italia
Osserv Astron Trieste - Italia Università degli Studi di Trieste - Italia Osservatorio Astronomico di Trieste - Italia |
| 8 | Girardi, M. | - |
UNIV TRIESTE - Italia
Osserv Astron Trieste - Italia Università degli Studi di Trieste - Italia Osservatorio Astronomico di Trieste - Italia |
| 9 | Gobat, Raphael A. S. | Hombre |
Univ Paris Diderot - Francia
Astrophysique, Instrumentation et Modélisation de Paris-Saclay - Francia |
| 10 | Grillo, C. | Hombre |
Univ Copenhagen - Dinamarca
Niels Bohr Institute - Dinamarca Niels Bohr Institutet - Dinamarca |
| 11 | Kelson, Daniel D. | Hombre |
Observatorio Las Campanas - Estados Unidos
|
| 12 | Medezinski, Elinor | Mujer |
Johns Hopkins Univ - Estados Unidos
Johns Hopkins University - Estados Unidos |
| 13 | Postman, M. | Hombre |
Space Telescope Sci Inst - Estados Unidos
STScI - Estados Unidos Space Telescope Science Institute - Estados Unidos |
| 14 | Scodeggio, M. | - |
INAF IAS Milano - Italia
|
| 15 | Brescia, Massimo | Hombre |
Osservatorio Astronomico di Capodimonte - Italia
|
| 16 | DEMARCO-BULL, RODRIGO ANDRES | Hombre |
Universidad de Concepción - Chile
Centro de Excelencia en Astrofísica y Tecnologías Afines - Chile |
| 17 | Fritz, A. | - |
INAF Istituto di Astrofisica Spaziale e Fisica Cosmica, Milan - Italia
INAF Istituto di Astrofisica Spaziale e Fisica Cosmica, Bologna - Italia |
| 18 | Koekemoer, Anton | Hombre |
STScI - Estados Unidos
Space Telescope Science Institute - Estados Unidos |
| 19 | Lemze, Dorom | Hombre |
Johns Hopkins University - Estados Unidos
Johns Hopkins Univ - Estados Unidos |
| 20 | Lombardi, M. | Hombre |
Univ Milan - Italia
Università degli Studi di Milano - Italia |
| 21 | Sartoris, B. | - |
UNIV TRIESTE - Italia
Osserv Astron Trieste - Italia Ist Nazl Fis Nucl - Italia Università degli Studi di Trieste - Italia Osservatorio Astronomico di Trieste - Italia Istituto Nazionale di Fisica Nucleare, Sezione di Trieste - Italia |
| 22 | Umetsu, Keiichi | Hombre |
Acad Sinica - Taiwán
Academia Sinica, Institute of Astronomy and Astrophysics - Taiwán |
| 23 | Vanzella, E. | Hombre |
Osservatorio Astron Bologna - Italia
INAF Istituto di Astrofisica Spaziale e Fisica Cosmica, Bologna - Italia |
| 24 | Bradley, L. D. | Hombre |
STScI - Estados Unidos
Space Telescope Science Institute - Estados Unidos |
| 25 | Coe, D. | - |
STScI - Estados Unidos
Space Telescope Science Institute - Estados Unidos |
| 26 | Donahue, M. | Mujer |
Michigan State Univ - Estados Unidos
Michigan State University - Estados Unidos |
| 27 | INFANTE-LIRA, LEOPOLDO | Hombre |
Pontificia Universidad Católica de Chile - Chile
Centro de Excelencia en Astrofísica y Tecnologías Afines - Chile |
| 28 | Kuchner, U. | Mujer |
Univ Vienna - Austria
Universität Wien - Austria |
| 29 | Maier, C. | - |
Univ Vienna - Austria
Universität Wien - Austria |
| 30 | Regos, E. | - |
European Lab Particle Phys - Suiza
European Organization for Nuclear Research - Suiza |
| 31 | Verdugo, M. | - |
Univ Vienna - Austria
Universität Wien - Austria |
| 32 | Ziegler, Bodo | Hombre |
Univ Vienna - Austria
Universität Wien - Austria |
| Fuente |
|---|
| FONDECYT |
| MIUR |
| Ministero dell’Istruzione, dell’Università e della Ricerca |
| BASAL Center for Astrophysics and Associated Technologies (CATA) |
| Ministero dell’Istruzione, dell’Università e della Ricerca |
| Agradecimiento |
|---|
| We thank the referee for providing useful and constructive comments that helped to improve the quality of this paper, and Elisabete da Cunha and Adam Muzzin for useful discussions. We also thank Elisabete da Cunha for providing us with a non public library of models for the MAGPHYS SED fitting procedure. We acknowledge financial support from MIUR PRIN2010-2011 (J91J12000450001). R.D. gratefully acknowledges the support provided by the BASAL Center for Astrophysics and Associated Technologies (CATA), and by FONDECYT grant N. 1130528. Based (in part) on data collected at Subaru Telescope and obtained from the SMOKA, which is operated by the Astronomy Data Center, National Astronomical Observatory of Japan. |
| We thank the referee for providing useful and constructive comments that helped to improve the quality of this paper, and Elisabete da Cunha and Adam Muzzin for useful discussions. We also thank Elisabete da Cunha for providing us with a non public library of models for the MAGPHYS SED fitting procedure. We acknowledge financial support from MIUR PRIN2010-2011 (J91J12000450001). R.D. gratefully acknowledges the support provided by the BASAL Center for Astrophysics and Associated Technologies (CATA), and by FONDECYT grant N. 1130528. Based (in part) on data collected at Subaru Telescope and obtained from the SMOKA, which is operated by the Astronomy Data Center, National Astronomical Observatory of Japan. |
