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The Hubble Space Telescope Extragalactic Distance Scale Key Project. X. The Cepheid Distance to NGC 7331The distance to NGC 7331 has been derived from Cepheid variables observed with HST/WFPC2, as part of the Extragalactic Distance Scale Key Project. Multi-epoch exposures in F555W(~V) and F814W (~1), with photometry derived independently from DoPHOT and DAOPHOT/ALLFRAME programs, which were used to detect a total of 14 reliable Cepheids, with periods between 11 and 42 days.
Document ID
20060036734
Acquisition Source
Jet Propulsion Laboratory
Document Type
Preprint (Draft being sent to journal)
External Source(s)
Authors
Hughes, S. M. G.
Han, M.
Hoessel, J.
Saha, A.
Silbermann, N.
Stetson, P. B.
Freedman, W. L.
Harding, P.
Kennicutt, R. C., Jr.
Madore, B. F.
Mould, J. R.
Ferrarese, L.
Ford, H.
Graham, J. A.
Hill, R.
Huchra, J.
Illingworth, G. D.
Phelps, R.
Sakai, S.
Date Acquired
August 23, 2013
Publication Date
January 1, 1996
Subject Category
Astronomy
Distribution Limits
Public
Copyright
Other
Keywords
Cepheids galaxies distances redshifts NGC 7331 early type stars stars luminosity
photometric techniques

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