V/24             Catalogue of Geneva Photometric Boxes     (Nicolet, 1982)

Catalogue of Geneva Photometric Boxes Nicolet B. <Astron. Astrophys. Suppl. Ser. 48, 485 (1982)> =1982A&AS...48..485N 1982A&AS...48..485N =2013yCat.5024....0N 2013yCat.5024....0N
ADC_Keywords: Photometry, Geneva Keywords: Geneva photometric system ; Star boxes ; Catalogues Abstract: The catalogue of the Geneva photometric boxes (or Golay's boxes) is announced. Introduction: The Geneva photometric boxes, or Golay's boxes, are based on the Geneva 7-colour photometry contained in Rufener's 3rd Catalogue (Cat. II/72). For a given star S measured in the Geneva photometry, the strict [0.01] box is the set of stars S' whose colours are all equal to those of S within 0.01mag; S is called the central star, and the S' are the member stars of the [0.01] box of S. Only the boxes containing at least 2 elements (including S) are considered. Other definitions of the photometric boxes are used. For instance, the "0.01" box of S contains the stars S' having |dU|=|U(S)-U(S')≤0.02, and all other colours |dV|, |dB1|, |dB2|, |dV1| and |dG| all ≤0.01. Photometric boxes can also be defined from other colour indices (reddening-free), or with elliptical shapes. See the definitions used here in the "Note (G2)" section below. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file cstar.dat 35 13457 List of central stars (stars defining boxes) member.dat 35 221730 Photometric associations (members of photometric boxes) catalog.txt 126 79732 Ready-to-print photometric boxes (1286 pages) -------------------------------------------------------------------------------- See also: II/72 : 3rd Catalogue of Stars Measured in the Geneva Photometric System (Rufener, 1981) Byte-by-byte Description of file: cstar.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 2- 10 I09 --- ID Coded identifier of star defining the box (G1) 11- 12 A2 --- n_ID Remarks on central star (component, variable) 13- 21 A9 --- Name Star name (HD or Durchmusterung) 22- 23 I2 h RAh Right Ascension B1900 (hours) 25- 28 F4.1 min RAm Right Ascension B1900 (minutes) 30 A1 --- DE- Declination B1900 (sign) 31- 32 I2 deg DEd Declination B1900 (degrees) 34- 35 I2 arcmin DEm Declination B1900 (minutes) -------------------------------------------------------------------------------- Byte-by-byte Description of file: member.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 2- 10 I09 --- ID Coded identifier of star defining the box (G1) 11- 12 A2 --- n_ID Remarks on central star (component, variable) 14- 22 I9 --- Name LID code of the member star (in the same box) 24- 27 A4 --- Btype [ABIJKLDE ] Type of box (G2) 29- 30 I2 h RAh Right Ascension B1900 (hours) 32- 35 F4.1 min RAm Right Ascension B1900 (minutes) -------------------------------------------------------------------------------- Gloval Notes: Note (G1): the "Geneva Identifier" is made from star designation in a hierarchy of catalogs (HD, Durchmusterungen, etc), see details in the Table I of the paper Note (G2): the "belonging code" contains 4 characters expressing in which definition the member star is associated to the star defining the photometric box: A = strict [0.01] box, i.e. the member star has all 6 colors U-B B1-B B2-B V-B V1-B G-B differing by at most 0.01mag (|dC|≤0.01) B = "0.01" box, i.e. the member star has |d(U-B)|≤0.02 and the 5 other colors differing by at most 0.01mag I = 0.012-0.009 4-colour boxes: |d(U-B1)|≤0.012, and the 3 other color indices |d(B1-B2)|, |d(B2-V1)| and |d(V1-G)| differ by ≤0.009 J = 0.016-0.012 4-colour boxes: |d(U-B1)|≤0.016, and the 3 other color indices |d(B1-B2)|, |d(B2-V1)| and |d(V1-G)| differ by ≤0.012 K = 0.010 elliptical 4-colour indices U-B1, B1-B2, B2-V1, V1-G L = 0.015 elliptical 4-colour indices U-B1, B1-B2, B2-V1, V1-G D = 0.008 elliptical (d Δ g) reddening-free indices: d=(U-B1)-1.430(B1-B2), Δ=(U-B2)-0.832(B2-G), g=(B1-B2)-1.357(V1-G) E = 0.012 elliptical (d Δ g) reddening-free indices History: * Prepared by B. Nicolet in Sptember 1981, and mailed to CDS on magnetic tape and microfiche. * 29-Mar-2013: Catalog standardized, documentation added.
(End) Francois Ochsenbein [CDS] 29-Mar-2013
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