Dataciencia

Revista	ISSN
Astronomy & Astrophysics	0004-6361

Revista

ISSN

Astronomy & Astrophysics

0004-6361

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WOS
Astronomy & Astrophysics

WOS

Astronomy & Astrophysics

Scopus
Sin Disciplinas

Scopus

Sin Disciplinas

SciELO
Sin Disciplinas

SciELO

Sin Disciplinas

Muestra la distribución de disciplinas para esta publicación.

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

Ord.	Autor	Género	Institución - País
1	GONZALEZ, ELIZABETH JOHANA	Mujer	Comision Nacional de Investigacion Cientifica y Tecnologica - Argentina UNIV NACL CORDOBA - Argentina Instituto de Astronomia Teorica y Experimental - Argentina Observatorio Astronomico de la Universidad Nacional de Cordoba - Argentina Consejo Nacional de Investigaciones Científicas y Técnicas (CONICET) - Argentina
2	de los Rios, M.	Hombre	Comision Nacional de Investigacion Cientifica y Tecnologica - Argentina UNIV NACL CORDOBA - Argentina Instituto de Astronomia Teorica y Experimental - Argentina Observatorio Astronomico de la Universidad Nacional de Cordoba - Argentina Consejo Nacional de Investigaciones Científicas y Técnicas (CONICET) - Argentina
3	Oio, Gabriel A.	Hombre	Comision Nacional de Investigacion Cientifica y Tecnologica - Argentina UNIV NACL CORDOBA - Argentina Instituto de Astronomia Teorica y Experimental - Argentina Observatorio Astronomico de la Universidad Nacional de Cordoba - Argentina Consejo Nacional de Investigaciones Científicas y Técnicas (CONICET) - Argentina
4	Hernandez Lang, Daniel	Hombre	Universidad de la Serena - Chile
4	Lang, Daniel Hernández	Hombre	Universidad de la Serena - Chile
5	Aguirre Tagliaferro, Tania	Mujer	Comision Nacional de Investigacion Cientifica y Tecnologica - Argentina UNIV NACL CORDOBA - Argentina Consejo Nacional de Investigaciones Científicas y Técnicas (CONICET) - Argentina
5	Tagliaferro, Tania Aguirre	Mujer	Instituto de Astronomia Teorica y Experimental - Argentina Observatorio Astronomico de la Universidad Nacional de Cordoba - Argentina Consejo Nacional de Investigaciones Científicas y Técnicas (CONICET) - Argentina UNIV NACL CORDOBA - Argentina
6	Dominguez, Mariano J. R.	Hombre	Comision Nacional de Investigacion Cientifica y Tecnologica - Argentina UNIV NACL CORDOBA - Argentina Instituto de Astronomia Teorica y Experimental - Argentina Observatorio Astronomico de la Universidad Nacional de Cordoba - Argentina Consejo Nacional de Investigaciones Científicas y Técnicas (CONICET) - Argentina
7	NILO-CASTELLON, JOSE LUIS	Hombre	Universidad de la Serena - Chile
8	Hector Cuevas, L.	-	Universidad de la Serena - Chile
8	Cuevas, H.	Hombre	Universidad de la Serena - Chile
9	Valotto, Carlos	Hombre	Comision Nacional de Investigacion Cientifica y Tecnologica - Argentina UNIV NACL CORDOBA - Argentina Instituto de Astronomia Teorica y Experimental - Argentina Observatorio Astronomico de la Universidad Nacional de Cordoba - Argentina Consejo Nacional de Investigaciones Científicas y Técnicas (CONICET) - Argentina

Ord.

Autor

Género

Institución - País

GONZALEZ, ELIZABETH JOHANA

Mujer

Comision Nacional de Investigacion Cientifica y Tecnologica - Argentina
UNIV NACL CORDOBA - Argentina
Instituto de Astronomia Teorica y Experimental - Argentina
Observatorio Astronomico de la Universidad Nacional de Cordoba - Argentina
Consejo Nacional de Investigaciones Científicas y Técnicas (CONICET) - Argentina

de los Rios, M.

Hombre

Oio, Gabriel A.

Hombre

Hernandez Lang, Daniel

Hombre

Universidad de la Serena - Chile

Lang, Daniel Hernández

Hombre

Universidad de la Serena - Chile

Aguirre Tagliaferro, Tania

Mujer

Comision Nacional de Investigacion Cientifica y Tecnologica - Argentina
UNIV NACL CORDOBA - Argentina
Consejo Nacional de Investigaciones Científicas y Técnicas (CONICET) - Argentina

Tagliaferro, Tania Aguirre

Mujer

Instituto de Astronomia Teorica y Experimental - Argentina
Observatorio Astronomico de la Universidad Nacional de Cordoba - Argentina
Consejo Nacional de Investigaciones Científicas y Técnicas (CONICET) - Argentina
UNIV NACL CORDOBA - Argentina

Dominguez, Mariano J. R.

Hombre

NILO-CASTELLON, JOSE LUIS

Hombre

Universidad de la Serena - Chile

Hector Cuevas, L.

Universidad de la Serena - Chile

Cuevas, H.

Hombre

Universidad de la Serena - Chile

Valotto, Carlos

Hombre

Fuente
Consejo Nacional de Investigaciones Científicas y Técnicas
National Science Foundation
Air Force Office of Scientific Research
Ohio State University
Vanderbilt University
University of Tokyo
Yale University
National Research Council
Alfred P. Sloan Foundation
U.S. Department of Energy Office of Science
University of Arizona
Brazilian Participation Group
Brookhaven National Laboratory
Carnegie Mellon University
University of Florida
French Participation Group
German Participation Group
Harvard University
Instituto de Astrofisica de Canarias
Michigan State/Notre Dame/JINA Participation Group
Johns Hopkins University
Lawrence Berkeley National Laboratory
Max Planck Institute for Astrophysics
Max Planck Institute for Extraterrestrial Physics
New Mexico State University
New York University
Pennsylvania State University
University of Portsmouth
Princeton University
Spanish Participation Group
University of Utah
University of Virginia
University of Washington
National Rehabilitation Center
Centre National de la Recherche Scientifique
Consejo Nacional de Investigaciones Cientificas y Tecnicas (CONICET, Argentina)
Consejo Nacional de Investigaciones CientÃficas y TÃ©cnicas
CFHT
Secretaria de Ciencia y Tecnologia de la Universidad Nacional de Cordoba (SeCyT-UNC, Argentina)
AFOSR/IO
Secretaria de Ciencia y Tecnología - Universidad Nacional de Córdoba
Southern Office of Aerospace Research and development
Southern Office of Aerospace Research and development (SOARD), a branch of the Air Force Office of the Scientific Researchs International Office of the United States (AFOSR/IO)
University of Hawai'i
Secretaria de Ciencia y TecnologÃa - Universidad Nacional de CÃ³rdoba
Institut National des Sciences de l'Univers, Centre National de la Recherche Scientifique
Direccion de Investigacion de la Universidad de La Serena through the Programa de Incentivo a la Investigacion Academica (PIA-DIULS)
DirecciÃ³n de la Industria del Software
SOARD
CEA/IRFU
Centre Eau Terre Environnement, Institut National de la Recherche Scientifique
Dirección de la Industria del Software

Fuente

Consejo Nacional de Investigaciones Científicas y Técnicas

National Science Foundation

Air Force Office of Scientific Research

Ohio State University

Vanderbilt University

University of Tokyo

Yale University

National Research Council

Alfred P. Sloan Foundation

U.S. Department of Energy Office of Science

University of Arizona

Brazilian Participation Group

Brookhaven National Laboratory

Carnegie Mellon University

University of Florida

French Participation Group

German Participation Group

Harvard University

Instituto de Astrofisica de Canarias

Michigan State/Notre Dame/JINA Participation Group

Johns Hopkins University

Lawrence Berkeley National Laboratory

Max Planck Institute for Astrophysics

Max Planck Institute for Extraterrestrial Physics

New Mexico State University

New York University

Pennsylvania State University

University of Portsmouth

Princeton University

Spanish Participation Group

University of Utah

University of Virginia

University of Washington

National Rehabilitation Center

Centre National de la Recherche Scientifique

Consejo Nacional de Investigaciones Cientificas y Tecnicas (CONICET, Argentina)

CFHT

Secretaria de Ciencia y Tecnologia de la Universidad Nacional de Cordoba (SeCyT-UNC, Argentina)

AFOSR/IO

Secretaria de Ciencia y Tecnología - Universidad Nacional de Córdoba

Southern Office of Aerospace Research and development

Southern Office of Aerospace Research and development (SOARD), a branch of the Air Force Office of the Scientific Researchs International Office of the United States (AFOSR/IO)

University of Hawai'i

Secretaria de Ciencia y TecnologÃa - Universidad Nacional de CÃ³rdoba

Institut National des Sciences de l'Univers, Centre National de la Recherche Scientifique

Direccion de Investigacion de la Universidad de La Serena through the Programa de Incentivo a la Investigacion Academica (PIA-DIULS)

DirecciÃ³n de la Industria del Software

SOARD

CEA/IRFU

Centre Eau Terre Environnement, Institut National de la Recherche Scientifique

Dirección de la Industria del Software

Agradecimiento
We thank the anonymous referee for the useful comments and suggestions which helped to improve the manuscript. This research is based on data collected at Subaru Telescope, which is operated by the National Astronomical Observatory of Japan and on observations obtained with MegaPrime/MegaCam, a joint project of CFHT and CEA/IRFU, at the Canada-France-Hawaii Telescope (CFHT) which is operated by the National Research Council (NRC) of Canada, the Institut National des Science de l'Univers of the Centre National de la Recherche Scientifique (CNRS) of France, and the University of Hawaii. This work is based in part on data products produced at Terapix available at the Canadian Astronomy Data Centre as part of the Canada-France-Hawaii Telescope Legacy Survey, a collaborative project of NRC and CNRS. Ww have made use of data and/or software provided by the High Energy Astrophysics Science Archive Research Center (HEASARC), which is a service of the Astrophysics Science Division at NASA/GSFC and the High Energy Astrophysics Division of the Smithsonian Astrophysical Observatory. We have made use of the ROSAT Data Archive of the Max-Planck-Institut fur extraterrestrische Physik (MPE) at Garching, Germany. We have also use SDSS-III data. Funding for SDSS-III has been provided by the Alfred P. Sloan Foundation, the Participating Institutions, the National Science Foundation, and the U.S. Department of Energy Office of Science. The SDSS-III web site is http://www.sdss3.org/. SDSS-III is managed by the Astrophysical Research Consortium for the Participating Institutions of the SDSS-III Collaboration including the University of Arizona, the Brazilian Participation Group, Brookhaven National Laboratory, Carnegie Mellon University, University of Florida, the French Participation Group, the German Participation Group, Harvard University, the Instituto de Astrofisica de Canarias, the Michigan State/Notre Dame/JINA Participation Group, Johns Hopkins University, Lawrence Berkeley National Laboratory, Max Planck Institute for Astrophysics, Max Planck Institute for Extraterrestrial Physics, New Mexico State University, New York University, Ohio State University, Pennsylvania State University, University of Portsmouth, Princeton University, the Spanish Participation Group, University of Tokyo, University of Utah, Vanderbilt University, University of Virginia, University of Washington, and Yale University. We made an extensive use of the following python libraries:http://www.numpy.org/, http://www.scipy.org/, http://roban.github.com/CosmoloPy/and http://www.matplotlib.org/. This work was partially supported by the Consejo Nacional de Investigaciones Cientificas y Tecnicas (CONICET, Argentina) and the Secretaria de Ciencia y Tecnologia de la Universidad Nacional de Cordoba (SeCyT-UNC, Argentina). J.L.N.C. is grateful of the Southern Office of Aerospace Research and Development (SOARD), a branch of the Air Force Office of the Scientific Researchs International Office of the United States (AFOSR/IO), for the financial support obtained through grant FA9550-15-1-0167. J.L.N.C. also acknowledges financial support from the Direccion de Investigacion de la Universidad de La Serena through the Programa de Incentivo a la Investigacion Academica (PIA-DIULS).
cA knowledgements. We thank the anonymous referee for the useful comments and suggestions which helped to improve the manuscript. This research is based on data collected at Subaru Telescope, which is operated by the National Astronomical Observatory of Japan and on observations obtained with MegaPrime/MegaCam, a joint project of CFHT and CEA/IRFU, at the Canada-France-Hawaii Telescope (CFHT) which is operated by the National Research Council (NRC) of Canada, the Institut National des Science de l’Univers of the Centre National de la Recherche Scientifique (CNRS) of France, and the University of Hawaii. This work is based in part on data products produced at Terapix available at the Canadian Astronomy Data Centre as part of the Canada-France-Hawaii Telescope Legacy Survey, a collaborative project of NRC and CNRS. Ww have made use of data and/or software provided by the High Energy Astrophysics Science Archive Research Center (HEASARC), which is a service of the Astrophysics Science Division at NASA/GSFC and the High Energy Astrophysics Division of the Smithsonian Astrophysical Observatory. We have made use of the ROSAT Data Archive of the Max-Planck-Institut für extraterrestrische Physik (MPE) at Garching, Germany. We have also use SDSS-III data. Funding for SDSS-III has been provided by the Alfred P. Sloan Foundation, the Participating Institutions, the National Science Foundation, and the U.S. Department of Energy Office of Science. The SDSS-III web site is http://www.sdss3.org/. SDSS-III is managed by the Astrophysical Research Consortium for the Participating Institutions of the SDSS-III Collaboration including the University of Arizona, the Brazilian Participation Group, Brookhaven National Laboratory, Carnegie Mellon University, University of Florida, the French Participation Group, the German Participation Group, Harvard University, the Instituto de Astrofísica de Canarias, the Michigan State/Notre Dame/JINA Participation Group, Johns Hopkins University, Lawrence Berkeley National Laboratory, Max Planck Institute for Astrophysics, Max Planck Institute for Extraterrestrial Physics, New Mexico State University, New York University, Ohio State University, Pennsylvania State University, University of Portsmouth, Princeton University, the Spanish Participation Group, University of Tokyo, University of Utah, Vanderbilt University, University of Virginia, University of Washington, and Yale University. We made an extensive use of the following python libraries: http://www.numpy.org/,http: //www.scipy.org/, http://roban.github.com/CosmoloPy/ and http://www.matplotlib.org/. This work was partially supported by the Consejo Nacional de Investigaciones Científicas y Técnicas (CONICET, Argentina) and the Secretaría de Ciencia y Tecnología de la Universidad Nacional de Córdoba (SeCyT-UNC, Argentina). J.L.N.C. is grateful of the Southern Office of Aerospace Research and Development (SOARD), a branch of the Air Force Office of the Scientific Researchs International Office of the United States (AFOSR/IO), for the financial support obtained through grant FA9550-15-1-0167. J.L.N.C. also acknowledges financial support from the Dirección de Investigación de la Universidad de La Serena through the Programa de Incentivo a la Investigación Académica (PIA-DIULS).

Agradecimiento

We thank the anonymous referee for the useful comments and suggestions which helped to improve the manuscript. This research is based on data collected at Subaru Telescope, which is operated by the National Astronomical Observatory of Japan and on observations obtained with MegaPrime/MegaCam, a joint project of CFHT and CEA/IRFU, at the Canada-France-Hawaii Telescope (CFHT) which is operated by the National Research Council (NRC) of Canada, the Institut National des Science de l'Univers of the Centre National de la Recherche Scientifique (CNRS) of France, and the University of Hawaii. This work is based in part on data products produced at Terapix available at the Canadian Astronomy Data Centre as part of the Canada-France-Hawaii Telescope Legacy Survey, a collaborative project of NRC and CNRS. Ww have made use of data and/or software provided by the High Energy Astrophysics Science Archive Research Center (HEASARC), which is a service of the Astrophysics Science Division at NASA/GSFC and the High Energy Astrophysics Division of the Smithsonian Astrophysical Observatory. We have made use of the ROSAT Data Archive of the Max-Planck-Institut fur extraterrestrische Physik (MPE) at Garching, Germany. We have also use SDSS-III data. Funding for SDSS-III has been provided by the Alfred P. Sloan Foundation, the Participating Institutions, the National Science Foundation, and the U.S. Department of Energy Office of Science. The SDSS-III web site is http://www.sdss3.org/. SDSS-III is managed by the Astrophysical Research Consortium for the Participating Institutions of the SDSS-III Collaboration including the University of Arizona, the Brazilian Participation Group, Brookhaven National Laboratory, Carnegie Mellon University, University of Florida, the French Participation Group, the German Participation Group, Harvard University, the Instituto de Astrofisica de Canarias, the Michigan State/Notre Dame/JINA Participation Group, Johns Hopkins University, Lawrence Berkeley National Laboratory, Max Planck Institute for Astrophysics, Max Planck Institute for Extraterrestrial Physics, New Mexico State University, New York University, Ohio State University, Pennsylvania State University, University of Portsmouth, Princeton University, the Spanish Participation Group, University of Tokyo, University of Utah, Vanderbilt University, University of Virginia, University of Washington, and Yale University. We made an extensive use of the following python libraries:http://www.numpy.org/, http://www.scipy.org/, http://roban.github.com/CosmoloPy/and http://www.matplotlib.org/. This work was partially supported by the Consejo Nacional de Investigaciones Cientificas y Tecnicas (CONICET, Argentina) and the Secretaria de Ciencia y Tecnologia de la Universidad Nacional de Cordoba (SeCyT-UNC, Argentina). J.L.N.C. is grateful of the Southern Office of Aerospace Research and Development (SOARD), a branch of the Air Force Office of the Scientific Researchs International Office of the United States (AFOSR/IO), for the financial support obtained through grant FA9550-15-1-0167. J.L.N.C. also acknowledges financial support from the Direccion de Investigacion de la Universidad de La Serena through the Programa de Incentivo a la Investigacion Academica (PIA-DIULS).

cA knowledgements. We thank the anonymous referee for the useful comments and suggestions which helped to improve the manuscript. This research is based on data collected at Subaru Telescope, which is operated by the National Astronomical Observatory of Japan and on observations obtained with MegaPrime/MegaCam, a joint project of CFHT and CEA/IRFU, at the Canada-France-Hawaii Telescope (CFHT) which is operated by the National Research Council (NRC) of Canada, the Institut National des Science de l’Univers of the Centre National de la Recherche Scientifique (CNRS) of France, and the University of Hawaii. This work is based in part on data products produced at Terapix available at the Canadian Astronomy Data Centre as part of the Canada-France-Hawaii Telescope Legacy Survey, a collaborative project of NRC and CNRS. Ww have made use of data and/or software provided by the High Energy Astrophysics Science Archive Research Center (HEASARC), which is a service of the Astrophysics Science Division at NASA/GSFC and the High Energy Astrophysics Division of the Smithsonian Astrophysical Observatory. We have made use of the ROSAT Data Archive of the Max-Planck-Institut für extraterrestrische Physik (MPE) at Garching, Germany. We have also use SDSS-III data. Funding for SDSS-III has been provided by the Alfred P. Sloan Foundation, the Participating Institutions, the National Science Foundation, and the U.S. Department of Energy Office of Science. The SDSS-III web site is http://www.sdss3.org/. SDSS-III is managed by the Astrophysical Research Consortium for the Participating Institutions of the SDSS-III Collaboration including the University of Arizona, the Brazilian Participation Group, Brookhaven National Laboratory, Carnegie Mellon University, University of Florida, the French Participation Group, the German Participation Group, Harvard University, the Instituto de Astrofísica de Canarias, the Michigan State/Notre Dame/JINA Participation Group, Johns Hopkins University, Lawrence Berkeley National Laboratory, Max Planck Institute for Astrophysics, Max Planck Institute for Extraterrestrial Physics, New Mexico State University, New York University, Ohio State University, Pennsylvania State University, University of Portsmouth, Princeton University, the Spanish Participation Group, University of Tokyo, University of Utah, Vanderbilt University, University of Virginia, University of Washington, and Yale University. We made an extensive use of the following python libraries: http://www.numpy.org/,http: //www.scipy.org/, http://roban.github.com/CosmoloPy/ and http://www.matplotlib.org/. This work was partially supported by the Consejo Nacional de Investigaciones Científicas y Técnicas (CONICET, Argentina) and the Secretaría de Ciencia y Tecnología de la Universidad Nacional de Córdoba (SeCyT-UNC, Argentina). J.L.N.C. is grateful of the Southern Office of Aerospace Research and Development (SOARD), a branch of the Air Force Office of the Scientific Researchs International Office of the United States (AFOSR/IO), for the financial support obtained through grant FA9550-15-1-0167. J.L.N.C. also acknowledges financial support from the Dirección de Investigación de la Universidad de La Serena through the Programa de Incentivo a la Investigación Académica (PIA-DIULS).

Abstract

Revista

Métricas Externas

Disciplinas de Investigación

Colaboración Institucional

Autores - Afiliación

Financiamiento

Agradecimientos

Departamento Gestión de Conocimiento, Monitoreo y Prospección