HST photometry of M51 cluster (Bik+, 2003)

Details HST photometry of M51 cluster (Bik+, 2003) HST photometry of M51 cluster (Bik+, 2003)

Mar 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003ycat..33970473b&link_type=abstract

VizieR On-line Data Catalog: J/A+A/397/473. Originally published in: 2003A&A...397..473B

Physics

Galaxies: Photometry, Associations: Stellar

Scientific paper

M 51 was observed with HST-WFPC2 as part of the HST Supernova INtensive Study (SINS) program (Millard et al., 1999ApJ...527..746M). For this study we use the images taken in the broad band filters F336W (U), F439W (B), F555W (V), F675W (R) and F814W (I) from the SINS program and in the narrow band filters F502N ([OIII]) and F656N (Hα) from the GO-program of H. C. Ford. The image in U was taken on 1994 May 12, the BVRI images were taken on Jan. 15 1995 and the [OIII] and Hα images on Jan. 25 1995. The U and B images were split into three and two exposures of 400s and 700s respectively. The [OIII] and Hα images are split into two exposures of 1200s and 500s ([OIII]) and 1400s and 400s (Hα). In the remaining bands one single exposure of 600s was taken. The data was processed through the PODPS (Post Observing Data Processing System) for bias removal, flat fielding and dark frame correction.
(2 data files).

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