A Cepheid Distance to NGC 4603 in Centaurus:

A WWW Supplement

Jeffrey A. Newman, Stephen E. Zepf, Marc Davis, Wendy L. Freedman, Barry F. Madore, Peter B. Stetson, N. Silbermann, and Randy Phelps

e-mail addresses: jnewman@astro.berkeley.edu, zepf@astro.yale.edu, marc@astro.berkeley.edu, wendy@ociw.edu, barry@ipac.caltech.edu, Peter.Stetson@hia.nrc.ca, nancys@ipac.caltech.edu, rphelps@physics.oberlin.edu

A preprint of our paper (gzipped Postscript) (PDF)

Color (Combined VI) image of Planetary Camera Field (gzipped Postscript) (JPEG)

Color (Combined VI) image of central portions of NGC 4603 (gzipped Postscript) (JPEG)

Light curves for all candidate Cepheids (gzipped Postscript) A more complete version of Figure 10 from the paper.

Captions for all figures (Postscript)

Complete Postscript figures (gzipped tar file)

Complete tables, including epochal photometry for all candidate Cepheids (Postscript)

Machine-Readable (space delimited) text tables of Epochal Photometry for candidate Cepheids:

Format: <Star ID Number> <Magnitude> <Error> <Magnitude> <Error> <Magnitude> <Error> . . .

V photometry
I photometry

All epochal photometry provided is based on robustly averaged ALLFRAME magnitudes using zero points and aperture and averaging bias corrections as described in the paper.