Quantitative comparison between type Ia supernova spectra at low and high redshifts: a case study

Quantitative comparison between type Ia supernova spectra at low and high redshifts: a case study

We develop a method to measure the strength of the absorption features in type la supernova (SN la) spectra and use it to make a quantitative comparisons between the spectra of type la supernovae at low and high redshifts. In this case study, we apply the method to 12 high-redshift (0.212 ≤ z ≤ 0.91...

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מידע ביבליוגרפי
Main Authors: Garavini, G, Folatelli, G, Nobili, S, Aldering, G, Amanullah, R, Antilogus, P, Astier, P, Blanc, G, Bronder, T, Burns, MS, Conley, A, Deustua, SE, Doi, M, Fabbro, S, Fadeyev, V, Gibbons, R, Goldhaber, G, Goobar, A, Groom, D, Hook, I, Howell, D, Kashikawa, N, Kim, A, Kowalski, M, Kuznetsova, N
פורמט: Journal article
שפה:English
יצא לאור: 2007

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