Abstract
We present a novel technique for fitting restframe I-band light curves on a data set of 42 type Ia supernovae (SNe Ia). Using the result of the fit, we construct a Hubble diagram with 26 SNe from the subset at 0.01< z
Original language | English |
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Pages (from-to) | 789-804 |
Number of pages | 16 |
Journal | Astronomy and Astrophysics |
Volume | 437 |
DOIs | |
Publication status | Published - 1 Jul 2005 |