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J/AJ/114/222        Cross identifications in NGC 1502 (Weitenbeck 1997)

Cross identifications in the region of cluster NGC 1502 Weitenbeck A.J. <Astron. J. 114, 222 (1997)> =1997AJ....114..222W
ADC_Keywords: Clusters, open ; Cross identifications Description: In studying this region Purgathofer (1964AnWie..26...37P) [the SIMBAD numbering], Hoag et al.(1961PUSNO..17..343H), and Dombrovskii and Hagen-Thorn (1964TrLen..20...75D) each set up their own numbering system; subsequent authors used one or another of those or variants or combinations. The region covered is 2 degrees in diameter, centered at: (2000) RA 04 04 53.28 dec +62 19 20.7. This is about 15' west of the cluster, the position of HD 25290. Objects: ----------------------------------------- RA (2000) DE Designation(s) ----------------------------------------- 04 07.8 +62 20 NGC 1502 = C 0403+622 ----------------------------------------- File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table1.dat 85 281 Cross Identifications near NGC 1502 by GSC number table2.dat 25 76 Cross Identifications near NGC 1502 by cluster member number
See also: I/220 : The HST Guide Star Catalog (Lasker+ 1992) Byte-by-byte Description of file: table1.dat
Bytes Format Units Label Explanations
1- 9 A9 --- GSC GSC designation (Cat. I/220) 11- 15 F5.2 mag mag Magnitude 17- 18 I2 h RAh Right ascension (J2000.0) 20- 21 I2 min RAm Right ascension (J2000.0) 23- 27 F5.2 s RAs Right ascension (J2000.0) 29 A1 --- DE- Declination sign 30- 31 I2 deg DEd Declination (J2000.0) 33- 34 I2 arcmin DEm Declination (J2000.0) 36- 39 F4.1 arcsec DEs Declination (J2000.0) 41- 54 A14 ---- Name Other name (1) 56- 67 A12 --- Name2 Other name (1) 69- 78 A10 ---- Name3 Other name (1) 79- 83 A5 --- Name4 Other name (1) 85 A1 --- Note [*] Note (2)
Note (1): Designations of the form NGC 1502 NN are from Purgathofer (1964AnWie..26...37P), those of the form HoagNN and DHNN are from Hoag et al. (1961PUSNO..17..343H) and Dombrovskii and Hagen-Thorn (1964TrLen..20...75D). Hoag et al. (1961PUSNO..17..343H) give a table of 26 numbered stars with photoelectric photometry, and a second, longer, unnumbered table of stars with photographic photometry, which includes the stars in the other table. Reiman and Pfau (1987AN....308..111R) numbered the stars in the second table by continuing the numbering from the first table, calling the first star in the second table 27; this system is used here. Note (2): 4067-862 and 4067-873: The 1855 coordinates for BD +61 649 lies almost exactly halfway between these two GSC stars. Additionally, 4067-414 10.8mag, is about 2.6' from the position 4068-347: This is evidently DH97, though DH do not give a BD number. There are no other stars of similar brightness in the vicinity in the GSC or on the Palomar Sky Survey.
Byte-by-byte Description of file: table2.dat
Bytes Format Units Label Explanations
1- 2 I2 --- NGC1502 NGC 1502 (1964AnWie..26...37P) identification number (1) 3 A1 --- m_NGC1502 Multiplicity index on NGC1502 5- 6 I2 --- Hoag ? Hoag (1961PUSNO..17..343H) number (2) 8- 9 I2 --- Tapia ? Tapia (1991MNRAS.253..649T) number 11- 12 I2 --- DH ? DH (1964TrLen..20...75D) number 14- 17 I4 --- GSC ? GSC 4068- (Cat. I/220) number
Note (1): NGC 1502 1 and 2: There is some confusion in the literature over identification of these two similar stars. In SIMBAD the lower HD number HD25638 = 1 is east of HD25639 = 2, and all the other identifications given there are consistent with this. PPM and DH are two of the places with the reverse of SIMBAD. Note (2): These Hoag et al. stars are not in the GSC: 24, 45, 58, 59, 63, 67, 69, 71, 80, 83, 85, 87, 88, 89, 92, 93, 94.
Acknowledgements: It is a pleasure to thank Anthony J. Weitenbeck (ajw(at)sal.wisc.edu) who kindly supplied a copy of this table. History: * 18-Nov-1997: Original version * 28-Mar-2008: One bad BD number in table1: GSC 218-4068 is BD+62 643 (originally written as BD+61 643)
(End) Patricia Bauer [CDS] 28-Mar-2008
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

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