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A Highly Magnified Supernova at z = 1.703 behind the Massive Galaxy Cluster A1689

Authors :
A. Goobar
Edvard Mörtsell
S. Fabbro
C. Lidman
K. Paech
H. Dahle
B. Milvang-Jensen
Teresa Riehm
Dan M. Watson
J. Nordin
B. Clement
Vallery Stanishev
J. Richard
Rahman Amanullah
J. P. Kneib
Jakob Jonsson
M. Limousin
Jens Hjorth
J. G. Cuby
Tomas Dahlen
Department of Astronomy
Stockholm University
Department of Physics
Laboratoire d'Astrophysique de Marseille (LAM)
Aix Marseille Université (AMU)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)
University of Oslo (UiO)
Niels Bohr Institute [Copenhagen] (NBI)
Faculty of Science [Copenhagen]
University of Copenhagen = Københavns Universitet (UCPH)-University of Copenhagen = Københavns Universitet (UCPH)
University of Victoria [Canada] (UVIC)
European Southern Observatory (ESO)
Centre de Recherche Astrophysique de Lyon (CRAL)
École normale supérieure de Lyon (ENS de Lyon)-Université Claude Bernard Lyon 1 (UCBL)
Université de Lyon-Université de Lyon-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)
Instituto Superior Técnico, Universidade Técnica de Lisboa (IST)
Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Aix Marseille Université (AMU)-Centre National d'Études Spatiales [Toulouse] (CNES)
University of Copenhagen = Københavns Universitet (KU)-University of Copenhagen = Københavns Universitet (KU)
École normale supérieure - Lyon (ENS Lyon)-Université Claude Bernard Lyon 1 (UCBL)
Université de Lyon-Université de Lyon-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)
Source :
The Astrophysical journal letters, The Astrophysical journal letters, 2011, 742, pp.L7. ⟨10.1088/2041-8205/742/1/L7⟩, The Astrophysical journal letters, Bristol : IOP Publishing, 2011, 742, pp.L7. ⟨10.1088/2041-8205/742/1/L7⟩
Publication Year :
2011
Publisher :
HAL CCSD, 2011.

Abstract

Our ability to study the most remote supernova explosions, crucial for the understanding of the evolution of the high-redshift universe and its expansion rate, is limited by the light collection capabilities of telescopes. However, nature offers unique opportunities to look beyond the range within reach of our unaided instruments thanks to the light-focusing power of massive galaxy clusters. Here we report on the discovery of one of the most distant supernovae ever found, at redshift, z=1.703. Due to a lensing magnification factor of 4.3\pm0.3, we are able to measure a lightcurve of the supernova, as well as spectroscopic features of the host galaxy with a precision comparable to what will otherwise only be possible with future generation telescopes.<br />Comment: 19 pages, 4 figures, 1 table, accepted to ApJL

Details

Language :
English
ISSN :
20418205 and 20418213
Database :
OpenAIRE
Journal :
The Astrophysical journal letters, The Astrophysical journal letters, 2011, 742, pp.L7. ⟨10.1088/2041-8205/742/1/L7⟩, The Astrophysical journal letters, Bristol : IOP Publishing, 2011, 742, pp.L7. ⟨10.1088/2041-8205/742/1/L7⟩
Accession number :
edsair.doi.dedup.....ff9fb8ac2b54d71ada3a7ab8e44a953d
Full Text :
https://doi.org/10.1088/2041-8205/742/1/L7⟩