Journal Article

Cosmic flows: University of Hawaii 2.2-m <i>I</i>-band photometry

Hélène M. Courtois, R. Brent Tully and Philippe Héraudeau

in Monthly Notices of the Royal Astronomical Society

Published on behalf of The Royal Astronomical Society

Volume 415, issue 2, pages 1935-1942
Published in print August 2011 | ISSN: 0035-8711
Published online July 2011 | e-ISSN: 1365-2966 | DOI:
Cosmic flows: University of Hawaii 2.2-m I-band photometry

Show Summary Details


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.

Keywords: astronomical data bases: miscellaneous; catalogues; galaxies: distances and redshifts; galaxies: photometry

Journal Article.  4592 words.  Illustrated.

Subjects: Astronomy and Astrophysics

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