J/AJ/109/218 J/AJ/109/218 Catalogue of globular cluster profiles S C Trager I R King S Djorgovski Astron. J. 109 218 1995 1995AJ....109..218T II/117 : Catalog of UBVRI Photometry of Globular Clusters (Peterson 1986) VII/151 : Structure Parameters of Galactic Globular Clusters (Webbink 1985) Clusters, globular Photometry, surface The data for individual objects are in tables file. The header information, which provides the Chebyshev and power-of-x coefficients, for each cluster are in tables.hdr file We present a catalogue of surface-brightness profiles (SBPs) of 125 Galactic globular clusters, the largest such collection ever gathered. The SBPs are constructed from generally inhomogeneous data, but are based heavily on the Berkeley Globular Cluster Survey of Djorgovski & King. All but four of the SBPs have photometric zero points. We derive central surface brightnesses, King-model concentrations, core radii, half-light, and other fraction-of-light radii where data permit, and we briefly discuss their use.

Name Cluster name --- logRad Log of radius of surface brightness meas. arcsec muV Meas. surface brightness at r, in V mags. mag/arcsec2 muVf Fitted surface brightness at r, from Chebyshev fit mag/arcsec2 Resid Residual of Chebyshev fit at r, muV-muVf mag/arcsec2 Weight Weight of data point in Chebyshev fit --- DataSet Data set name The CCD data follow a naming convention: "C" stands for data taken at CTIO; e.g. "CRB1" stands for the first "B" image from the CTIO 1.5m reflector with the RCA chip. "L" stands for the Lick 1 m Nickel reflector: these datasets are labeled as, e.g. "LTR-B", the second frame from the Lick Nickel reflector, taken with the T1 chip through the Spinrad "R" filter. See Sec. 2.1 of printed paper for details of chips and filters. "DJB2" stands for the second "B" image taken by Djorgovski. For Terzan 5, "I" refers to an I-band image from CTIO kindly provided by Dr. T. Armandroff. "UPGA.4" means the first ("A") ultraviolet ("U") plate used for photographic photometry ("PG") of the cluster in question. "SCAN" data are scanning photoelectric photometry. "ANN" data are centered-aperture photoelectric photometry. Photographic star counts are referenced by plate number; see caption to Figure 2 in printed paper for references. --- CDS 1995Jul10AAS CD-ROM series, Vol. 4, 1995 Lee Brotzman [ADS] 26-Apr-1995 J_AJ_109_218.xml