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Journal articles
Spectroscopic confirmation of high-redshift supernovae with the ESO VLT
C. Lidman
D.A. Howell
G. Folatelli
G. Garavini
1
S. Nobili
1
G. Aldering
R. Amanullah
P. Antilogus
1
P. Astier
1
G. Blanc
M. S. Burns
A. Conley
S. E. Deustua
M. Doi
R. Ellis
S. Fabbro
V. Fadeyev
R. Gibbons
G. Goldhaber
A. Goobar
D. E. Groom
I. Hook
N. Kashikawa
A. G. Kim
R.A. Knop
B. C. Lee
J. Mendez
T. Morokuma
K. Motohara
P. E. Nugent
R. Pain
1
S. Perlmutter
V. Prasad
R. Quimby
J. Raux
1
N. Regnault
1
P. Ruiz-Lapuente
G. Sainton
1
B. E. Schaefer
K. Schahmaneche
1
E. Smith
A. L. Spadafora
V. Stanishev
N.A. Walton
L. Wang
W. M. Wood-Vasey
N. Yasuda
S. Nobili 1
Author
G. Aldering
Author
R. Amanullah
Author
P. Antilogus 1
Author IdHAL : pierre-antilogus arXiv : https://arxiv.org/a/PierreAntilogus ORCID : https://orcid.org/0000-0002-0389-5706
K. Motohara
Author
P. E. Nugent
Author
R. Pain 1
Author IdHAL : reynald-pain ORCID : https://orcid.org/0000-0003-4016-6067
S. Perlmutter
Author
1
LPNHE - Laboratoire de Physique Nucléaire et de Hautes Énergies (Barre 12-22, 1er étage 4 Place Jussieu 75252 Paris Cedex 05 - France)
- CNRS - Centre National de la Recherche Scientifique : UMR7585 (France)
- UPD7 - Université Paris Diderot - Paris 7 (5 rue Thomas-Mann - 75205 Paris cedex 13 - France)
- IN2P3 - Institut National de Physique Nucléaire et de Physique des Particules du CNRS (France)
- UPMC - Université Pierre et Marie Curie - Paris 6 (4 place Jussieu - 75005 Paris - France)
Abstract : We present VLT FORS1 and FORS2 spectra of 39 candidate high-redshift supernovae that were discovered as part of a cosmological study using Type Ia supernovae (SNe Ia) over a wide range of redshifts. From the spectra alone, 20 candidates are spectrally classified as SNe Ia with redshifts ranging from z=0.212 to z=1.181. Of the remaining 19 candidates, 1 might be a Type II supernova and 11 exhibit broad supernova-like spectral features and/or have supernova-like light curves. The candidates were discovered in 8 separate ground-based searches. In those searches in which SNe Ia at z ~ 0.5 were targeted, over 80% of the observed candidates were spectrally classified as SNe Ia. In those searches in which SNe Ia with z > 1 were targeted, 4 candidates with z > 1 were spectrally classified as SNe Ia and later followed with ground and space based observatories. We present the spectra of all candidates, including those that could not be spectrally classified as supernova.
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Journal articles
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http://hal.in2p3.fr/in2p3-00023320
Contributor : Sylvie Flores Connect in order to contact the contributor
Submitted on : Tuesday, November 21, 2006 - 10:57:31 AM
Last modification on : Monday, January 4, 2021 - 2:44:02 PM
Contributor : Sylvie Flores Connect in order to contact the contributor
Submitted on : Tuesday, November 21, 2006 - 10:57:31 AM
Last modification on : Monday, January 4, 2021 - 2:44:02 PM
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- HAL Id : in2p3-00023320, version 1
- ARXIV : astro-ph/0410506
- DOI : 10.1051/0004-6361:20041504
Collections
LPNHE | CNRS | UNIV-PARIS7 | IN2P3 | UPMC | USPC | SORBONNE-UNIVERSITE | SU-SCIENCES | UNIV-PARIS | UP-SCIENCES | SU-TI
Citation
C. Lidman, D.A. Howell, G. Folatelli, G. Garavini, S. Nobili, et al.. Spectroscopic confirmation of high-redshift supernovae with the ESO VLT. Astronomy and Astrophysics - A&A, EDP Sciences, 2005, 430, pp.843-851. ⟨10.1051/0004-6361:20041504⟩. ⟨in2p3-00023320⟩
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