J/AJ/103/131 J/AJ/103/131 Photometric Study of Globular Palomar 14 S Holland W E Harris Astrophys. Journ. 103, No. 1 131 1992 1992AJ....103..131H Clusters, globular Colors Photometry, UBV This catalog contains relative coordinates and deep B and V CCD photometry for 327 stars in a field of the second-parameter outermost-halo globular cluster Palomar 14. It corresponds to Table 3 in the published source reference. It is based on six V and four B frames obtained with the RCA4 CCD camera at the prime focus of the 3.6m CFHT on May 16-17 1988. The resultant limiting V magnitude is approximately 24.5. The scale factor is 0.206 arcsec/pixel. Positions are given in the table as "x" and "y" in pixel units, where x increases Eastward and y increases Southward. The star identification numbers given by the authors are arbitrary and were assigned in order of increasing y. The V magnitudes and the (B-V) colors are tabulated. The data reduction was done using DAOPHOT . Palomar 14 is located at R.A.=16h08.8m and Dec=+15deg,05.2min (1950). The field observed is centered approximately 1.14' West and 2.32' South of the cluster center.

Ident Star identification --- x x coordinate (+x=E; 1 pixel= 0.206") pixel y y coordinate (+y=S; 1 pixel= 0.206") pixel V V magnitude mag (B-V) (B-V) color mag J.E. Gass Hughes STX/NASA 1995Sep08 UNKNOWN UNKNOWN Machine-readable version records were sorted in order of ascending star identifier as submitted by author. The published table was printed in order of decreasing V magnitude. ReadMe by J. E. Gass (Hughes STX) Sep. 1995. J_AJ_103_131.xml