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The Astrophysical Journal 704 (2009) 1036-1058
The Carnegie Supernova Project: First Near-Infrared Hubble Diagram to z ~ 0.7
W. L. Freedman, C. R. Burns, M. M. Phillips, P. Wyatt, S. E. Persson, B. F. Madore 1, 2, C. Contreras, G. Folatelli, E. Sergio Gonzalez, M. Hamuy, E. Hsiao, D. D. Kelson, N. Morrell, D. C. Murphy, M. Roth, M. Stritzinger, L. Sturch, N. B. Suntzeff, P. Astier 3, C. Balland 3, B. Bassett, L. Boldt, R. G. Carlberg 4, A. J. Conley, J. A. Frieman, P. M. Garnavich, J. Guy 3, D. Hardin 3, D. A. Howell, R. Kessler, H. Lampeitl, J. Marriner, R. Pain 3, K. Perrett, N. Regnault 3, A. G. Riess, M. Sako, D. P. Schneider, M. Sullivan, M. Wood-Vasey
For the SUPERNOVAE collaboration(s)
(2009-10)

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
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
Physics/Astrophysics/Cosmology and Extra-Galactic Astrophysics

Sciences of the Universe/Astrophysics/Cosmology and Extra-Galactic Astrophysics
cosmology: observations – distance scale – supernovae: general
Fulltext link: 
http://fr.arXiv.org/abs/0907.4524