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Monthly Notices of the Royal Astronomical Society 415 (2011) 1935-1942
Cosmic flows: University of Hawaii 2.2-m I-band photometry
H.M. Courtois1, R. Brent Tully, P. Héraudeau
(08/2011)

Within the 'Cosmic Flows' project, I-band photometry of 524 relatively nearby galaxies has been carried out over the course of several years with the University of Hawaii 2.2-m telescope and a camera with a 7.5-arcmin field of view. The primary scientific goal was to provide global magnitudes and inclinations for galaxies for the purpose of measuring distances through the correlation between galaxy luminosities and rotation rates. The 1σ accuracy on a total magnitude is 0.08 mag. The observations typically extend to 7-8 exponential disc scalelengths, so the data are useful for studies of the structural properties of galaxies.
1 :  IPNL - Institut de Physique Nucléaire de Lyon
Cosmologie Observationnelle
Physique/Astrophysique/Astrophysique galactique

Planète et Univers/Astrophysique/Astrophysique galactique

Physique/Astrophysique/Cosmologie et astrophysique extra-galactique

Planète et Univers/Astrophysique/Cosmologie et astrophysique extra-galactique
astronomical data bases: miscellaneous – catalogues – galaxies: distances and redshifts – galaxies: photometry
Lien vers le texte intégral : 
http://fr.arXiv.org/abs/1103.5106