III/151     UBV K Stars South Galactic Pole (Kuijken+ 1989)

Catalogue of K Stars Towards the South Galactic Pole Kuijken K., Gilmore G. <Mon. Not. R. Astron. Soc., 239, 605, (1989)> =1989MNRAS.239..605K 1989MNRAS.239..605K
ADC_Keywords: Galactic pole, south ; Stars, K-type Description: B and V photographic photometry is collected for approximately 2000 stars near the south galactic pole with 0.8<B-V<1.20; v<19.0, and B<20.06. Velocities with respect to the local standard of rest are provided for approximately 500 K dwarfs and K giants. table8.dat contains photometry in 11.5 square degrees towards the South Galactic Pole, derived from UK Schmidt data, and table9.dat contains photometric data over 0.72 square degrees, derived from 4 B and 3 V plates from Las Campanas Observatory. table10.dat, table11.dat and table12.dat contain velocities for dwarf stars. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table8.dat 60 1846 UK Schmidt photometric data in SGP table9.dat 60 170 Las Campanas Plates photometric data table10.dat 52 472 Spectral data for K dwarfs, 8-plate photometry table11.dat 52 39 Spectral data for K dwarfs, 4-plate photometry table12.dat 52 69 Spectral data for K giants -------------------------------------------------------------------------------- Table 8: Byte-by-byte Description of file: table[89].dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 4 I4 --- ID Star number 5 A1 --- Obs [L] 'L' for Las Campanas (table9) data 6- 7 I2 h RAh Right ascension hours (1950) 9- 10 I2 min RAm Right ascension minutes (1950) 12- 16 F5.2 s RAs Right ascension seconds (1950) 18 A1 --- DE- Sign of declination 19- 20 I2 deg DEd Declination degree (1950) 22- 23 I2 arcmin DEm Declination minute (1950) 25- 28 F4.1 arcsec DEs Declination second (1950) 30- 34 F5.2 mag Vmag V magnitude 36- 39 F4.2 mag e_Vmag *Mean error of Vmag 41- 45 F5.2 mag Bmag B magnitude 47- 50 F4.2 mag e_Bmag *Mean error of Bmag 52- 55 F4.2 mag B-V *B-V color 57- 60 F4.2 mag e_B-V *Mean error of B-V color -------------------------------------------------------------------------------- Note on e_Vmag, e_Bmag, e_B-V: e_V and e_B refer to the rms scatter of the different plates' measurements, not the errors in the mean e_B-V refers to the error on the mean Note on B-V: table8: all stars with 0.80<B-V<1.20, Vmag<19.0, Bmag<20.06 are listed. table9: all stars with 0.80<B-V<1.20, Vmag<20 are listed -------------------------------------------------------------------------------- Byte-by-byte Description of file: table1[012].dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 4 I4 --- ID *?Star number 5 A1 --- Obs [i] in table11.dat 7- 8 I2 h RAh Right ascension hours (1950) 10- 11 I2 min RAm Right ascension minutes (1950) 13- 17 F5.2 s RAs Right ascension seconds (1950) 19 A1 --- DE- Sign of declination 20- 21 I2 deg DEd Declination degree (1950) 23- 24 I2 arcmin DEm Declination minute (1950) 26- 29 F4.1 arcsec DEs Declination second (1950) 31- 35 F5.2 mag Vmag V magnitude 37- 40 F4.2 mag B-V B-V color 42- 46 F5.0 km/s Vlsr Velocity w/respect to local std of rest 48- 52 F5.3 km/s e_Vlsr *?Uncertainty of Vlsr -------------------------------------------------------------------------------- Note on ID: Where given, ID refers to ID in table8.dat. Note on e_Vlsr: e_Vlsr refers to the rms scatter of the different plates' measurements, not the errors in the mean -------------------------------------------------------------------------------- History: * 21-Sep-1995: (Nancy G. Roman, ADC): * 10-Apr-1996:
(End) Julie Anne Watko [SSDOO/ADC] 10-Apr-1996
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