III/133         Michigan Catalogue of HD stars, Vol.4  (Houk+, 1988)

Catalogue of two-dimensional spectral types for the HD stars. Vol.4 Houk N., Smith-Moore M. <Ann Arbor, Dept. of Astronomy, Univ. of Michigan (1988)>
ADC_Keywords: MK spectral classification Description: Please refer to the "adc.txt" file by Wayne H. Warren Jr. See also: III/31 : Michigan Catalogue, Vol.1 (-90/-53deg, Houk N., 1975) III/51 : Michigan Catalogue, Vol.2 (-53/-40deg, Houk N., 1978) III/80 : Michigan Catalogue, Vol.3 (-40/-26deg, Houk N., 1982) File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file adc.txt 79 961 Documentation by Wayne H. Warren Jr. vol4.dat 127 33301 The Catalogue (vol.4) rem4.dat 375 5143 Notes (to vol.4) plates4.dat 32 505 Summary of Plates -------------------------------------------------------------------------------- Byte-per-byte Description of file: vol4.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 6 I6 --- HD Henry Draper Catalog (HD) number 7 A1 --- Case [*] if sp. type has lower case in printed ver. 8 A1 --- n_SpType [+] if spectral type is from HD Catalog 9- 26 A18 --- SpType Spectral type 27 A1 --- Ave_Flag [A] if classification used is an average. 28 I1 --- q_SpType [1/4]? Quality of the classification, see adc.txt 29- 33 A5 --- Remark Remark (see adc.txt Appendix A for description) 35- 40 A6 mag Ptg Photographic magnitude from HD catalog 41 A1 --- Var_Flag 'V' if star is known or suspected variable 43- 44 I2 h RAh Hours RA, 1900.0 46- 47 I2 min RAm Minutes RA, 1900.0 49- 52 F4.1 s RAs Seconds RA, 1900.0 54 A1 --- DE- Sign Dec, 1900.0 55- 56 I2 deg DEd Degrees Dec, 1900.0 58- 59 I2 arcmin DEm Minutes Dec, 1900.0 61- 62 I2 arcsec DEs Seconds Dec, 1900.0 64- 67 I4 0.01min/yr precRAm Centennial precession in RA, minutes 69- 72 F4.1 0.01s/yr precRAs Centennial precession in RA, seconds 74 A1 0.01arcmin/yr precDE- Centennial precession in Dec, sign 75- 76 I2 0.01arcmin/yr precDEm Centennial precession in Dec, minutes 78- 79 I2 0.01arcsec/yr precDEs Centennial precession in Dec, seconds 81- 85 F5.1 deg GLON Galactic longitude 87- 91 F5.1 deg GLAT Galactic latitude 93-102 A10 --- DM Durchmusterung identification ('BD', 'CD', or 'CP' in bytes 93-94; -ZZNNNNN in bytes 95-102) 106-111 I6 --- SAO [1/258997]? SAO Catalog number 112-115 A4 --- Plate1 Plate code #1 (see file plates4) 116-119 A4 --- Plate2 Plate code #2 (see file plates4) 120-123 A4 --- Plate3 Plate code #3 (see file plates4) 124-127 A4 --- Plate4 Plate code #4 (see file plates4) -------------------------------------------------------------------------------- Byte-per-byte Description of file: rem4.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 6 I6 --- HD Henry Draper Catalog (HD) number 8-375 A368 --- Remark Remarks in free form text -------------------------------------------------------------------------------- Byte-per-byte Description of file: plates4.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 4 A4 --- Code Plate code 7- 11 I5 --- Number Plate Number 15- 32 A18 --- Date Exposure date -------------------------------------------------------------------------------- Historical Notes: * 22-Nov-1993: list of plates added at CDS * 08-Dec-1994: list of plates provided by Shiro Nishimura [ADAC/NAOJ]
(End) Francois Ochsenbein [CDS] 08-Dec-1994
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