VizieR Online Data Catalog: BVRI photometry in NGC 2419, Pal 4, and Pal 14 (Saha+, 2005)

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).