BVRI photometry in NGC 2419, Pal 4, and Pal 14 (Saha+, 2005)

Details BVRI photometry in NGC 2419, Pal 4, and Pal 14 (Saha+, 2005) BVRI photometry in NGC 2419, Pal 4, and Pal 14 (Saha+, 2005)

Feb 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006ycat..71170037s&link_type=abstract

VizieR On-line Data Catalog: J/PASP/117/37. Originally published in: 2005PASP..117...37S

Physics

Photometry: Ubvri, Clusters: Globular, Photometry: Cousins

Scientific paper

Observations were made primarily with the WIYN 3.5m telescope at the Kitt Peak National Observatory. In addition, our target fields and standard stars were also observed at the WIYN 0.9m telescope at Kitt Peak. Observations of NGC 2419, Pal 4, and Pal 14, all of which are distant globular clusters in our galaxy and have the additional virtue of having been observed repeatedly with the WFPC2 camera of the HST, were made on nights that appeared to be cloudless.
(3 data files).

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