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Young Galaxy Candidates in the Hubble Frontier Fields. IV. MACS J1149.5+2223
Indexado
WoS WOS:000395870900003
Scopus SCOPUS_ID:85014345394
DOI 10.3847/1538-4357/AA5D55
Año 2017
Tipo artículo de investigación

Citas Totales

Autores Afiliación Chile

Instituciones Chile

% Participación
Internacional

Autores
Afiliación Extranjera

Instituciones
Extranjeras


Abstract



We search for high-redshift dropout galaxies behind the Hubble Frontier Fields (HFF) galaxy cluster MACS J1149.5+2223, a powerful cosmic lens that has revealed a number of unique objects in its field. Using the deep images from the Hubble and Spitzer space telescopes, we find 11 galaxies at z > 7 in the MACS J1149.5+2223 cluster field, and 11 in its parallel field. The high-redshift nature of the bright z similar or equal to 9.6 galaxy MACS1149-JD, previously reported by Zheng et al., is further supported by non-detection in the extremely deep optical images from the HFF campaign. With the new photometry, the best photometric redshift solution for MACS1149-JD reduces slightly to z = 9.44 +/- 0.12. The young galaxy has an estimated stellar mass of (7 +/- 2) x 10(8) M-circle dot, and was formed at z = 13.2(-1.6)(+1.9) when the universe was approximate to 300 Myr old. Data available for the first four HFF clusters have already enabled us to find faint galaxies to an intrinsic magnitude of M-UV similar or equal to -15.5, approximately a factor of 10 deeper than the parallel fields.

Revista



Revista ISSN
Astrophysical Journal 0004-637X

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Disciplinas de Investigación



WOS
Astronomy & Astrophysics
Scopus
Sin Disciplinas
SciELO
Sin Disciplinas

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

Colaboración Institucional



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Autores - Afiliación



Ord. Autor Género Institución - País
1 Zheng, Wei - Johns Hopkins Univ - Estados Unidos
Johns Hopkins University - Estados Unidos
2 Zitrin, A. - CALTECH - Estados Unidos
BEN GURION UNIV NEGEV - Israel
California Institute of Technology - Estados Unidos
Ben-Gurion University of the Negev - Israel
3 INFANTE-LIRA, LEOPOLDO Hombre Pontificia Universidad Católica de Chile - Chile
Centro de Excelencia en Astrofísica y Tecnologías Afines - Chile
4 Laporte, Nicolas Hombre UCL - Reino Unido
University College London - Reino Unido
5 Huang, Xingxing - Univ Sci & Technol China - China
University of Science and Technology of China - China
6 Moustakas, John Hombre Siena Coll - Estados Unidos
Siena College - Estados Unidos
7 Ford, Holland C. - Johns Hopkins Univ - Estados Unidos
Johns Hopkins University - Estados Unidos
8 Shu, X. - Univ Sci & Technol China - China
Anhui Normal Univ - China
University of Science and Technology of China - China
Anhui Normal University - China
9 Wang, Jun-Xian Hombre Univ Sci & Technol China - China
University of Science and Technology of China - China
10 Diego, Jose M. Hombre UC CSIC - España
CSIC-UC - Instituto de Física de Cantabria (IFCA) - España
11 BAUER, FRANZ ERIK Hombre Pontificia Universidad Católica de Chile - Chile
Instituto Milenio de Astrofísica - Chile
Space Sci Inst - Estados Unidos
Space Science Institute - Estados Unidos
Centro de Excelencia en Astrofísica y Tecnologías Afines - Chile
12 TRONCOSO-IRIBARREN, PAULINA ALEJANDRA Mujer Pontificia Universidad Católica de Chile - Chile
13 Broadhurst, Thomas Hombre Univ Basque Country UPV EHU - España
Basque Fdn Sci - España
Universidad del País Vasco - España
Ikerbasque, the Basque Foundation for Science - España
Ikerbasque, Basque Foundation for Science - España
14 Molino, Alberto Hombre UNIV SAO PAULO - Brasil
CSIC - España
Universidade de Sao Paulo - USP - Brasil
Instituto de Astrofísica de Andalucía - CSIC - España
Universidade de São Paulo - Brasil

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Origen de Citas Identificadas



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

Citas Identificadas: 9.09 %
Citas No-identificadas: 90.91 %

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

Citas Identificadas: 9.09 %
Citas No-identificadas: 90.91 %

Financiamiento



Fuente
CONICYT
CONICYT-Chile
National Natural Science Foundation of China
National science foundation of China
Fundação de Amparo à Pesquisa do Estado de São Paulo
MINECO/FEDER
NASA
Fundação de Amparo à Pesquisa do Estado de São Paulo
Ministry of Economy, Development, and Tourism's Millennium Science Initiative
CAS Frontier Science Key Research Program
Horizon 2020 Framework Programme
NASA through Hubble Fellowship - STScI
European Research Council Advanced Grant
Brazilian funding agency FAPESP

Muestra la fuente de financiamiento declarada en la publicación.

Agradecimientos



Agradecimiento
The work presented in this paper is based on observations made with the NASA/ESA Hubble Space Telescope, obtained from the Data Archive at the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS 5-26555. It is also based on data obtained with the Spitzer Space Telescope, which is operated by the Jet Propulsion Laboratory, California Institute of Technology under a contract with NASA. This work utilizes gravitational lensing models produced by the teams led by Bradac, Ishigaki, Kneib & Natarajan, Sharon, Williams, Merten & Zitrin, respectively. Support for A.Z. is provided by NASA through Hubble Fellowship grant HST-HF-51334.01-A awarded by STScI. N.L. acknowledges support from a European Research Council Advanced Grant FP7/669253. L.I., N.L., F.E.B. and P.T.I. are in part supported by CONICYT-Chile grants Basal-CATA PFB-06/2007, 3140542 and Conicyt-PIA-ACT 1417. F.E.B. also thanks CONICYT-Chile grant FONDECYT Regular 1141218 and the Ministry of Economy, Development, and Tourism's Millennium Science Initiative through grant IC120009, awarded to The Millennium Institute of Astrophysics, MAS. J.M.D. acknowledges support of the consolider projects CSD2010-00064, AYA2012-39475-C02-01 and AYA2015-64508-P (MINECO/FEDER, UE). A.M. acknowledges the financial support of the Brazilian funding agency FAPESP (Post-doc fellowship 2014/11806-9). X.X.H. and J.X.W. acknowledge support from the National Science Foundation of China (grants 11233002,11421303) and the CAS Frontier Science Key Research Program (QYZDJ-SSWSLH006).
A.M. acknowledges the financial support of the Brazilian funding agency FAPESP (Post-doc fellowship 2014/11806-9). X.X.H. and J.X.W. acknowledge support from the National Science Foundation of China (grants 11233002,11421303) and the CAS Frontier Science Key Research Program (QYZDJSSWSLH006).

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