Using spectral flux ratios to standardize SN Ia luminosities

Astronomy and Astrophysics

Volumn 500, Issue 2, 2009, Pages

  Bailey, S ^a   Aldering, G ^b   Antilogus, P ^a   Aragon, C ^b   Baltay, C ^c   Bongard, S ^a   Buton, C ^d,e,f   Childress, M ^b,g   Chotard, N ^d,e,f   Copin, Y ^d,e,f   Gangler, E ^d,e,f   Loken, S ^b   Nugent, P ^b   Pain, R ^a   Pecontal, E ^d,e,h,i   Pereira, R ^d,e,f   Perlmutter, S ^b,g   Rabinowitz, D ^c   Rigaudier, G ^d,e,h,i   Runge, K ^b   Scalzo, R ^c   Smadja, G ^d,e,f   Swift, H ^b,g   Tao, C ^j   Thomas, R C ^b   Wu, C ^a   more..

^a UNIVERSITÉ PARIS DIDEROT   (France)

^b LAWRENCE BERKELEY NATIONAL LABORATORY   (United States)

^c Yale University   (United States)

^d UNIVERSITÉ DE LYON   (France)

^e UNIVERSITÉ LYON 1   (France)

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

^g UNIVERSITY OF CALIFORNIA   (United States)

^h CENTRE DE RECHERCHE ASTROPHYSIQUE DE LYON   (France)

ⁱ UNIVERSITÉ DE LYON   (France)

^j AIX MARSEILLE UNIVERSITÉ   (France)

more..

Author keywords

Cosmology: observations; Stars: supernovae: general

Indexed keywords

BROAD BANDS; COLOR MEASUREMENTS; COLOR PARAMETER; CORRECTION FACTORS; COSMOLOGY: OBSERVATIONS; EQUIVALENT WIDTH; FLUX RATIO; HUBBLE DIAGRAMS; LIGHT CURVES; NORMALIZATION METHODS; SPECTRAL FEATURE; SPECTRAL FLUX; STANDARD DEVIATION; STARS: SUPERNOVAE: GENERAL; TRAINING SAMPLE;

COLOR; COSMOLOGY; STARS;

LUMINANCE;

EID: 67649560507     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/200911973     Document Type: Article

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