| HAL: in2p3-00455299, version 1 |
| arXiv: 0907.4524 |
| ADS Bibliographic id: 2009ApJ...704.1036F |
| DOI: 10.1088/0004-637X/704/2/1036 |
| Detailed view | Export this paper |
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| The Astrophysical Journal 704 (2009) 1036-1058 |
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| The Carnegie Supernova Project: First Near-Infrared Hubble Diagram to z ~ 0.7 |
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| W. L. FreedmanC. R. Burns |
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| For the SUPERNOVAE collaboration(s) |
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| (2009-10) |
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| The Carnegie Supernova Project (CSP) is designed to measure the luminosity distance for Type Ia supernovae (SNe Ia) as a function of redshift, and to set observational constraints on the dark energy contribution to the total energy content of the universe. The CSP differs from other projects to date in its goal of providing an I-band rest-frame Hubble diagram. Here, we present the first results from near-infrared observations obtained using the Magellan Baade telescope for SNe Ia with 0.1 |
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| 1: | Laboratoire d'Astrophysique de Marseille (LAM) |
| CNRS : UMR6110 – INSU – Université de Provence - Aix-Marseille I | |
| 2: | Observatories of the Carnegie Institution of Washington (OCIW) |
| Carnegie Institution of Washington | |
| 3: | Laboratoire de Physique Nucléaire et de Hautes Énergies (LPNHE) |
| CNRS : UMR7585 – IN2P3 – Université Pierre et Marie Curie [UPMC] - Paris VI – Université Paris VII - Paris Diderot | |
| 4: | Department of Astronomy and Astrophysics |
| University of Toronto | |
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| Subject(s) | : | Physics/Astrophysics/Cosmology and Extra-Galactic Astrophysics Sciences of the Universe/Astrophysics/Cosmology and Extra-Galactic Astrophysics |
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| cosmology: observations – distance scale – supernovae: general |
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| Fulltext link: |
| in2p3-00455299, version 1 | |
| http://hal.in2p3.fr/in2p3-00455299 | |
| oai:hal.in2p3.fr:in2p3-00455299 | |
| From: Julien Guy | |
| Submitted on: Wednesday, 10 February 2010 13:44:31 | |
| Updated on: Wednesday, 10 February 2010 13:45:01 | |