Do spectra improve distance measurements of Type Ia supernovae?

Astronomy and Astrophysics

Volumn 526, Issue 10, 2011, Pages

  Blondin, S ^a   Mandel, K S ^b   Kirshner, R P ^b  

^a CENTRE DE CALCUL DE L INSTITUT NATIONAL DE PHYSIQUE NUCLEAIRE ET DE PHYSIQUE DES PARTICULES   (France)

^b HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

Author keywords

cosmology: observations; supernovae: general

Indexed keywords

COLOR PARAMETER; COLOR VARIATIONS; COSMOLOGY: OBSERVATION; CROSS VALIDATION; DARK ENERGY; EQUIVALENT WIDTH; EXPLOSION MODELS; FLUX RATIO; HOST GALAXIES; HUBBLE DIAGRAMS; LINEAR MODEL; RED SHIFT; SPECTRAL FLUX; SPECTROSCOPIC MEASUREMENTS; STATISTICAL SIGNIFICANCE; SUPERNOVAE: GENERAL; SYNTHETIC SPECTRA; WEIGHTED RMS;

ABSORPTION; ABSORPTION SPECTROSCOPY; ASTRONOMY; COLOR; STANDARDS;

ATMOSPHERIC OPTICS;

EID: 78650906727     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201015792     Document Type: Article

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