J/ApJ/628/729       CCD BVIc photometry of M10 stars          (Pollard+, 2005)

The unusual luminosity function of the globular cluster M10. Pollard D.L., Sandquist E.L., Hargis J.R., Bolte M. <Astrophys. J., 628, 729-737 (2005)> =2005ApJ...628..729P 2005ApJ...628..729P
ADC_Keywords: Clusters, globular ; Photometry, CCD ; Photometry, UBVRI Keywords: diffusion - globular clusters: individual (M10) - stars: evolution - stars: luminosity function, mass function Description: Observations of the globular cluster M10 were taken at the Kitt Peak National Observatory (KPNO) 0.9 m telescope on the nights of UT dates 1995 May 6 and 9 using BVI filters. All frames were taken using a 2048x2048 pixel CCD with pixels covering 0.68 arcseconds on a side, for a total field of approximately 23.2 arcminutes on a side. The data were calibrated against Stetson (2000PASP..112..925S 2000PASP..112..925S) standard stars. Additional high-resolution images were taken at the 3.6 m Canada-France-Hawaii Telescope (CFHT) on the night of UT date 1993 April 13 in BI filters. These observations used a 1200x1200 pixel CCD with pixels covering 0.11 arcseconds on a side, for a total field 2.2 arcminutes on a side, roughly centered on the cluster core. These data were calibrated against the KPNO data. Objects: ---------------------------------------------------------- RA (2000) DE Designation(s) ---------------------------------------------------------- 16 57 08.9 -04 05 58 M 10 = NGC 6254 = C 1654-040 ---------------------------------------------------------- File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file kpno.dat 77 21313 BVI Photometry for M10 stars cfht.dat 58 8448 BI Photometry for M10 stars -------------------------------------------------------------------------------- Byte-by-byte Description of file: kpno.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 5 I5 --- Seq Sequential number 7- 14 F8.3 pix Xpos X coordinate in pixels (1) 16- 23 F8.3 pix Ypos Y coordinate in pixels (1) 26- 32 F7.4 mag Bmag ?=0.0 Johnson B magnitude (2) 35- 41 F7.4 mag e_Bmag ?=0.0 Johnson B magnitude error 44- 50 F7.4 mag Vmag ?=0.0 Johnson V magnitude (2) 53- 59 F7.4 mag e_Vmag ?=0.0 Johnson V magnitude error 62- 68 F7.4 mag Icmag ?=0.0 Cousins I magnitude (2) 71- 77 F7.4 mag e_Icmag ?=0.0 Cousins I magnitude error -------------------------------------------------------------------------------- Note (1): Cluster center : (999, 1016). 1 pix = 0.68" North is approximately in the decreasing x direction in pixel coord., and east is in the decreasing y direction, although there is a small rotation. Note (2): These data have not been dereddened. -------------------------------------------------------------------------------- Byte-by-byte Description of file: cfht.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 4 I4 --- Seq Sequential number 6- 13 F8.3 pix Xpos X coordinate in pixels (1) 15- 22 F8.3 pix Ypos Y coordinate in pixels (1) 25- 31 F7.4 mag Bmag Johnson B magnitude (2) 34- 40 F7.4 mag e_Bmag Johnson B magnitude error 43- 49 F7.4 mag Icmag Cousins I magnitude (2) 52- 58 F7.4 mag e_Icmag Cousins I magnitude error -------------------------------------------------------------------------------- Note (1): The coordinates of the cfht.dat file can be approximately converted into kpno.dat coordinates using the transformation x(KPNO) = 900.819 - 0.01274 * x(CFHT) + 0.15936 * y(CFHT) y(KPNO) =1099.063 - 0.16071 * x(CFHT) - 0.00963 * y(CFHT) 1 pix = 0.11" Note (2): These data have not been dereddened. -------------------------------------------------------------------------------- Acknowledgements: Eric Sandquist, erics(at)sciences.sdsu.edu
(End) Eric Sandquist [San Diego State Univ.], Patricia Vannier [CDS] 08-Sep-2005
The document above follows the rules of the Standard Description for Astronomical Catalogues; from this documentation it is possible to generate f77 program to load files into arrays or line by line