J/A+A/390/961       VI photometry in NGC 188                 (Andreuzzi+, 2002)

The white dwarf cooling sequence in the old open cluster NGC 188. Andreuzzi G., Richer H.B., Limongi M., Bolte M. <Astron. Astrophys. 390, 961 (2002)> =2002A&A...390..961A 2002A&A...390..961A
ADC_Keywords: Clusters, open ; Photometry, UBVRI Keywords: open clusters and associations: individual: NGC 188 - stars: white dwarfs - stars: luminosity function Abstract: We used HST-WFPC2 to study the white dwarf luminosity function of the old open cluster NGC 188 in order to determine a lower limit to the age of the cluster (∼5Gyr) by looking at the faint end of the cooling sequence (down to V∼26.5). Description: HST-WFCs photometry in the F555W-F814W filters, is presented for 223 objects belonging to 4 different fields located on the center of the cluster. By applying selection criteria to the catalog (stellarity index, c≥0.8), we identified 157 candidate stars of which 28 white dwarfs. Objects: ---------------------------------------------------------- RA (2000) DE Designation(s) ---------------------------------------------------------- 00 48 26 +85 15 21 NGC 188 cluster center 00 48 00 +85 13 30 Field f1 00 48 00 +85 16 00 Field f2 00 46 00 +85 16 00 Field f3 00 46 00 +85 13 30 Field f4 ---------------------------------------------------------- File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file catalog.dat 70 223 V, V-I photometry for stars in NGC 188 -------------------------------------------------------------------------------- See also: J/AJ/124/601 : Absolute positions & proper motions in NGC 188 (Platais+, 2002) Byte-by-byte Description of file: catalog.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 3- 9 F7.3 pix xpos x coordinate (1) 12- 18 F7.3 pix ypos y coordinate (1) 22- 27 F6.3 mag Imag Johnson I magnitude (from F814W filter) 32- 36 F5.3 mag e_Imag I photometric error 40- 45 F6.3 mag Vmag Johnson V magnitude (from F555W filter) 50- 54 F5.3 mag e_Vmag V photometric error 59- 63 F5.3 --- c Stellarity index (2) 65- 70 I6 --- ID Identification number (3) -------------------------------------------------------------------------------- Note (1): The observations consisted of four fields, f1, f2, f3 and f4, in such a way that WF4 of the field f4 overlaps WF2 of the field f1 and WF4 of the field f3 overlaps WF2 of the field f2. 1 pix = 0.1arcsec (HST-WFC). The coordinates in the catalogue are computed respect to different median images, obtained considering the single field and camera: 4 x WF2 4 x WF3 4 x WF4 Note (2): The catalog includes only the objects for which stellarity index c is ≥0.2 Note (3): IDs in the catalog have been created to indicates the camera and the field in which each object has been identified: the first number in the ID indicate the field (f1, f2, f3, f4); the second one indicate the camera: WF2: ID<f30000; WF3: f30000≤ID<f40000; WF4: f40000≤ID<f50000 -------------------------------------------------------------------------------- Acknowledgements: Gloria Andreuzzi History: * 14-Apr-2004: the original catalog contained a decimal fraction ".000" attached to each ID number (last column of catalog), which has been removed.
(End) Patricia Bauer [CDS] 30-Aug-2002
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