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| 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
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.
| 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
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| 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 |
| 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 |
| 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). |