II/41       420nm CN and G bands in G8-K5 spectra          (Griffin+ 1960)

Photoelectric Measurements of the 4200-A CN Band and the G Band in G8-K5 Spectra Griffin R.E., Redman R.O. <Mon. Not. R. Astron. Soc., 120, 287 (1960)> =1960MNRAS.120..287G 1960MNRAS.120..287G
ADC_Keywords: Photometry, CN band; Photometry, G band; Stars, late-type Description: Measurements of the λ4200Å CN band are presented for 712 late-type stars. G band data are also included for 212 of these stars. Mean errors of absolute magnitudes derived from CN intensities are at least 1.5 mag. Spectral type determined by G band intensity has a mean deviation of 0.15 class from the MK type for G to K1 stars. The file photom.dat contains 712 data records in the form of CN ratios and G-band ratios, with annotations. The CN ratio is the ratio of the sum of the intensities in the 4097-4149Å and 4230-4283Å wavelength ranges to the intensity in the 4164-4214Å range. The latter contains the CN absorption band, and the first two ranges serve as nearby continuum references. The ratio is a measure of the depth of the absorption in the CN band. Values greater than 2 indicate absorption in the band. The G-band ratio is similarly the ratio of the sum of the intensities in the 4230-4270Å and 4342-4380Å wavelength ranges to the intensity in the 4285-4315Å range. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file photom.dat 20 712 Catalog Data (table 1 of paper) -------------------------------------------------------------------------------- Byte-by-byte Description of file: photom.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 6 I6 --- HD ? Number of star in the Henry Draper Catalog (1) 9- 11 I3 % CN CN-band ratio (x100) 14- 16 I3 % Gband ? G-band ratio (x100) 19- 20 A2 --- Notes Notes to the entries (2) -------------------------------------------------------------------------------- Note (1): In three instances, the star observed has no HD number and this column is left blank. The star is identified in the fourth column. Note (2): Meaning of the characters in these columns: A = Dynamical space velocity greater than 80km/s B = "4150" C = "Weak-CN" D = "Strong-line" E = "Weak-line" F = BD+42 939 G = Composite spectrum, early-type companion H = Double, companion star only partly excluded by slit I = Star name: 49 Ser B J = Star name: 70 Oph B In the cases of all double stars not indicated with 'H', where the angular separation is less than 2 arcsec, the two stars have been measured together, and where the separation is more than 2 arcsec, the brighter component alone has been observed.
(End) Julie Anne Watko [SSDOO/ADC], Seth W. Digel [SSDOO] 25-Aug-1997
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