Colección SciELO Chile

Departamento Gestión de Conocimiento, Monitoreo y Prospección
Consultas o comentarios: productividad@anid.cl
Búsqueda Publicación
Búsqueda por Tema Título, Abstract y Keywords



Discovery of two neighbouring satellites in the Carina constellation with MagLiteS
Indexado
WoS WOS:000428835700054
Scopus SCOPUS_ID:85045890270
DOI 10.1093/MNRAS/STY170
Año 2018
Tipo artículo de investigación

Citas Totales

Autores Afiliación Chile

Instituciones Chile

% Participación
Internacional

Autores
Afiliación Extranjera

Instituciones
Extranjeras


Abstract



We report the discovery of two ultra-faint satellites in the vicinity of the Large Magellanic Cloud (LMC) in data from the Magellanic Satellites Survey (MagLiteS). Situated 18 deg (similar to 20 kpc) from the LMC and separated from each other by only 18 arcmin, Carina II and III form an intriguing pair. By simultaneously modelling the spatial and the colour-magnitude stellar distributions, we find that both Carina II and Carina III are likely dwarf galaxies, although this is less clear for Carina III. There are in fact several obvious differences between the two satellites. While both are well described by an old and metal poor population, Carina II is located at similar to 36 kpc from the Sun, with M-V similar to -4.5 and r(h) similar to 90 pc, and it is further confirmed by the discovery of 3 RR Lyrae at the right distance. In contrast, Carina III is much more elongated, measured to be fainter (M-V similar to -2.4), significantly more compact (r(h) similar to 30 pc), and closer to the Sun, at similar to 28 kpc, placing it only 8 kpc away from Car II. Together with several other systems detected by the Dark Energy Camera, Carina II and III form a strongly anisotropic cloud of satellites in the vicinity of the Magellanic Clouds.

Métricas Externas



PlumX Altmetric Dimensions

Muestra métricas de impacto externas asociadas a la publicación. Para mayor detalle:

Disciplinas de Investigación



WOS
Astronomy & Astrophysics
Scopus
Sin Disciplinas
SciELO
Sin Disciplinas

Muestra la distribución de disciplinas para esta publicación.

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

Colaboración Institucional



Muestra la distribución de colaboración, tanto nacional como extranjera, generada en esta publicación.


Autores - Afiliación



Ord. Autor Género Institución - País
1 Torrealba, G. - UNIV CAMBRIDGE - Reino Unido
Acad Sinica - Taiwán
Institute of Astronomy - Reino Unido
Academia Sinica, Institute of Astronomy and Astrophysics - Taiwán
2 Belokurov, Vasily Hombre UNIV CAMBRIDGE - Reino Unido
Flatiron Inst - Estados Unidos
Institute of Astronomy - Reino Unido
Flatiron Institute - Estados Unidos
Simons Foundation - Estados Unidos
3 Koposov, S. Hombre UNIV CAMBRIDGE - Reino Unido
Carnegie Mellon Univ - Estados Unidos
Institute of Astronomy - Reino Unido
Carnegie Mellon University - Estados Unidos
4 Bechtol, K. Hombre Large Synopt Survey Telescope - Estados Unidos
Large Synoptic Survey Telescope - Estados Unidos
5 Drlica-Wagner, A. Hombre Fermilab Natl Accelerator Lab - Estados Unidos
Fermi National Accelerator Laboratory - Estados Unidos
6 Olsen, Knut A. G. Hombre Natl Opt Astron Observ - Estados Unidos
National Optical Astronomy Observatory - Estados Unidos
7 Vivas, A. Katherina Mujer Natl Opt Astron Observ - Chile
Cerro Tololo Inter American Observatory - Chile
National Optical Astronomy Observatory - Chile
8 Yanny, B. Hombre Fermilab Natl Accelerator Lab - Estados Unidos
Fermi National Accelerator Laboratory - Estados Unidos
9 Jethwa, Prashin - UNIV CAMBRIDGE - Reino Unido
Institute of Astronomy - Reino Unido
10 WALKER, ALISTAIR Hombre Natl Opt Astron Observ - Chile
Cerro Tololo Inter American Observatory - Chile
National Optical Astronomy Observatory - Chile
11 Bulik, T. Hombre Fermilab Natl Accelerator Lab - Estados Unidos
Fermi National Accelerator Laboratory - Estados Unidos
12 Allam, S. Mujer Fermilab Natl Accelerator Lab - Estados Unidos
Fermi National Accelerator Laboratory - Estados Unidos
13 Conn, Blair C. - Mt Stromlo & Siding Spring Observ - Australia
Australian National University, Mount Stromlo Observatory - Australia
14 Gallart, C. Mujer Inst Astrofis Canarias - España
UNIV LA LAGUNA - España
Instituto Astrofisico de Canarias - España
Universidad de La Laguna - España
15 Gruen, D. Hombre UNIV ILLINOIS - Estados Unidos
Natl Ctr Supercomp Applicat - Estados Unidos
University of Illinois at Urbana-Champaign - Estados Unidos
University of Illinois Urbana-Champaign - Estados Unidos
16 James, David J. Hombre Harvard Smithsonian Ctr Astrophys - Estados Unidos
Harvard-Smithsonian Center for Astrophysics - Estados Unidos
17 Johnson, Margaret W. G. Mujer Natl Ctr Supercomp Applicat - Estados Unidos
University of Illinois at Urbana-Champaign - Estados Unidos
University of Illinois Urbana-Champaign - Estados Unidos
18 Kuehn, K. Hombre Australian Astron Observ - Australia
Australian Astronomical Observatory - Australia
19 Kuropatkin, N. Hombre Fermilab Natl Accelerator Lab - Estados Unidos
Fermi National Accelerator Laboratory - Estados Unidos
20 Martin, N. F. Hombre Univ Strasbourg - Francia
Max Planck Inst Astron - Alemania
Université de Strasbourg - Francia
Max Planck Institute for Astronomy - Alemania
21 Martinez-Delgado, D. Hombre Heidelberg Univ - Alemania
Astronomisches Rechen-Institut Heidelberg - Alemania
Astronomisches Rechen-Institut - Alemania
22 Ségransan, Damien Hombre Natl Opt Astron Observ - Estados Unidos
National Optical Astronomy Observatory - Estados Unidos
23 Noël, N. E.D. Mujer Univ Surrey - Reino Unido
University of Surrey - Reino Unido
24 Simon, Joshua D. Hombre Observ Carnegie Inst Sci - Estados Unidos
Observatorio Las Campanas - Estados Unidos
25 Stringfellow, Guy Hombre UNIV COLORADO - Estados Unidos
University of Colorado Boulder - Estados Unidos
26 Tucker, D. L. Hombre Fermilab Natl Accelerator Lab - Estados Unidos
Fermi National Accelerator Laboratory - Estados Unidos

Muestra la afiliación y género (detectado) para los co-autores de la publicación.

Origen de Citas Identificadas



Muestra la distribución de países cuyos autores citan a la publicación consultada.

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

Citas Identificadas: 14.29 %
Citas No-identificadas: 85.71000000000001 %

Muestra la distribución de instituciones nacionales o extranjeras cuyos autores citan a la publicación consultada.

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

Citas Identificadas: 14.29 %
Citas No-identificadas: 85.71000000000001 %

Financiamiento



Fuente
National Science Foundation
Fundação Carlos Chagas Filho de Amparo à Pesquisa do Estado do Rio de Janeiro
Conselho Nacional de Desenvolvimento Científico e Tecnológico
Ministerio de Economía y Competitividad
Comisión Nacional de Investigación Científica y Tecnológica
Spanish Ministry of Economy and Competitiveness
University of Illinois at Urbana-Champaign
Australian Research Council
Deutsche Forschungsgemeinschaft
Ministry of Science and Technology
Financiadora de Estudos e Projetos
European Research Council
Conicyt Chile
U.S. Department of Energy
U.S. National Science Foundation
Ohio State University
Comisión Nacional de Investigación Científica y Tecnológica
Science and Technology Facilities Council
Robert Martin Ayers Sciences Fund
Seventh Framework Programme
Lawrence Berkeley National Laboratory
University of Portsmouth
Ministerio de Economía y Competitividad
University of Chicago
Science and Technology Facilities Council of the United Kingdom
Spanish Ministry of Economy and Competitiveness (MINECO)
University of Cambridge
Office of Science
University of Michigan
Academia Sinica
Ministry of Science and Education of Spain
Higher Education Funding Council for England
National Center for Supercomputing Applications at the University of Illinois at Urbana-Champaign
Kavli Institute of Cosmological Physics at the University of Chicago
Center for Cosmology and Astro-Particle Physics at the Ohio State University
Mitchell Institute for Fundamental Physics and Astronomy at Texas AM University
Ministerio da Ciencia, Tecnologia e Inovacao
Argonne National Laboratory
University College London
University of Edinburgh
Eidgenossische Technische Hochschule (ETH) Zurich
Fermi National Accelerator Laboratory
Institut de Ciencies de l'Espai (IEEC/CSIC)
Institut de Fisica d'Altes Energies
Ludwig-Maximilians Universitat Munchen
National Optical Astronomy Observatory
University of Nottingham
University of Pennsylvania
SLAC National Accelerator Laboratory
University of Sussex
Texas AM University
University of California at Santa Cruz
Centro de Investigaciones Energeticas, Medioambientales y Tecnologicas-Madrid
Stanford University
DES-Brazil Consortium
European Research Council under the European Union
U.S. Department of Energy, Office of Science, Office of High Energy Physics
Horizon 2020 Framework Programme
Ministry of Science and Technology, Taiwan
SLAC National Accelerator Laboratory, Stanford University
Fermilab
NationalCenter for Supercomputing Applications at the University of Illinois at Urbana-Champaign
Excellence Cluster Universe
Collaborating Institutions in the Dark Energy Survey
Fermi Research Alliance, LLC
Texas A and M University
Center for Cosmology and Astroparticle Physics, Ohio State University
Mitchell Institute for Fundamental Physics and Astronomy at Texas A&M University
Ministerio de Ciencia y Tecnología
High Energy Physics
United States Government
University of California, Santa Cruz
Eidgenössische Technische Hochschule Zürich
Conselho Nacional de Desenvolvimento Cient?fico e Tecnol?gico
Universidade do Estado do Rio de Janeiro
Pesquisa do Estado do Rio de Janeiro
Minist?rio da Ci?ncia
Collaborating Institutions are Argonne National Laboratory
Institut de Ci?ncies de l'Espai
Institut de F?sica d'Altes Energies
Ludwig-Maximilians Universit ?
Science and Technology FacilitiesCouncil
Eidgen?ssische Technische Hochschule

Muestra la fuente de financiamiento declarada en la publicación.

Agradecimientos



Agradecimiento
GT acknowledges support from the Ministry of Science and Technology grant MOST 105-2112-M-001-028-MY3, and a Career Development Award (to YTL) from Academia Sinica.
Support for GT is provided by CONICYT Chile. We are grateful for Director's Discretionary time on the Blanco 4 m with DECam. CG acknowledges support by the Spanish Ministry of Economy and Competitiveness (MINECO) under grant AYA2014-56795-P. The research leading to these results has received funding from the European Research Council under the European Union's Seventh Framework Programme (FP/2007-2013)/ERC grant agreement no. 308024. BCC acknowledges the support of the Australian Research Council through Discovery project DP150100862. Funding for the DES Projects has been provided by the U.S. Department of Energy, the U.S. National Science Foundation, theMinistry of Science and Education of Spain, the Science and Technology FacilitiesCouncil of theUnitedKingdom, theHigher Education Funding Council for England, the NationalCenter for Supercomputing Applications at the University of Illinois at Urbana-Champaign, the Kavli Institute of Cosmological Physics at the University of Chicago, the Center for Cosmology and Astro-Particle Physics at the Ohio State University, the Mitchell Institute for Fundamental Physics and Astronomy at Texas A&M University, Financiadora de Estudos e Projetos, Funda??o Carlos Chagas Filho de Amparo ? Pesquisa do Estado do Rio de Janeiro, Conselho Nacional de Desenvolvimento Cient?fico e Tecnol?gico and the Minist?rio da Ci?ncia, Tecnologia e Inovac?o, the Deutsche Forschungsgemeinschaft, and the Collaborating Institutions in the Dark Energy Survey. The Collaborating Institutions are Argonne National Laboratory, the University of California at Santa Cruz, the University of Cambridge, Centro de Investigaciones En?rgeticas, Medioambientales y Tecnol?gicas-Madrid, the University of Chicago, University College London, the DES-Brazil Consortium, the University of Edinburgh, the Eidgen?ssische Technische Hochschule (ETH) Z?rich, Fermi National Accelerator Laboratory, the University of Illinois at Urbana-Champaign, the Institut de Ci?ncies de l'Espai (IEEC/CSIC), the Institut de F?sica d'Altes Energies, Lawrence Berkeley National Laboratory, the Ludwig-Maximilians Universit ?t M?nchen and the associated Excellence Cluster Universe, the University of Michigan, the National Optical Astronomy Observatory, the University of Nottingham, the Ohio State University, the University of Pennsylvania, the University of Portsmouth, SLAC National Accelerator Laboratory, Stanford University, the University of Sussex, and Texas A&M University. This manuscript has been authored by Fermi Research Alliance, LLC under Contract No. DE-AC02-07CH11359 with the U.S. Department of Energy, Office of Science, Office of High Energy Physics. TheUnited StatesGovernment retains and the publisher, by accepting the article for publication, acknowledges that the United States Government retains a non-exclusive, paid-up, irrevocable, world-wide license to publish or reproduce the published form of this manuscript, or allow others to do so, for United States Government purposes. This research has made use of the APASS data base, located at the AAVSO web site. Funding for APASS has been provided by the Robert Martin Ayers Sciences Fund. BCC acknowledges the support of the Australian Research Council through Discovery project DP150100862. GTacknowledges support from the Ministry of Science and Technology grant MOST 105-2112-M-001-028-MY3, and a Career Development Award (to YTL) from Academia Sinica.

Muestra la fuente de financiamiento declarada en la publicación.