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J/other/AISAO/32.31      BVr photometry in SA68, SA 5 and M 82 (Afanasiev+ 1990)

Spectral and photometrical investigation of objects in selected fields with the 6-m telescope Afanasiev V.L., Vlasyuk V.V., Dodonov J.N., Lorens H., Terebbizh V.Y. <Astrofizik. Issledovanija, 32, 31 (1990)> =1990AISAO..32...31A (SIMBAD/NED BibCode)
ADC_Keywords: Photometry, CCD ; MK spectral classification Abstract: A description of the photometry and spectroscopy of the objects of the fields SA 68 (00h14m51.03s +15deg36'19.1"), M 82 (9h53m28.33s +69deg52'12.7") and SA 57 (13h06m03.69s +29deg36'31.8") is given. Photometric samples of the objects are complete to B=21.75m for the field SA 68, to B=22.25m for the field M 82. and to B=23m for the field SA 57. Spectroscopy is completed up to 64 % for the field SA 68, to 63% for the field M 82, and to 56% for the field SA 57. Photometric and spectroscopic data are gathered into catalogues. Objects: ---------------------------------------------------------- RA (2000) DE Designation(s) ---------------------------------------------------------- 00 17 28 +15 53 12 SA 68 13 08 26 +29 24 SA 57 09 55 51 +69 41 45 M 82 ---------------------------------------------------------- File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file tab3-5 60 518 Photometric catalog tab6-8 40 186 Spectroscopic catalog
Byte-by-byte Description of file: tab3-5
Bytes Format Units Label Explanations
1- 6 A6 --- Field Field name 8- 10 I3 --- N Sequential number 12- 14 I3 --- Nf Photometric catalogue sequential number 16- 17 I2 h RAh Right ascension (1950) 19- 20 I2 min RAm Right ascension (1950) 22- 26 F5.2 s RAs Right ascension (1950) 28 A1 --- DE- Declination sign 29- 30 I2 deg DEd Declination (1950) 32- 33 I2 arcmin DEm Declination (1950) 35- 39 F5.2 arcsec DEs Declination (1950) 40- 44 F5.2 mag Bmag ? B magnitude 46- 50 F5.2 mag Vmag ? V magnitude 52- 56 F5.2 mag rmag ? r magnitude 58 I1 --- MType [0/3]? Morphological type (1) 60 A1 --- Com [N] Comments (2)
Note (1): 0: Star 1: Star ? 2: Star ? (the B curve is not a stellar one) 3: Diffuse source Note (2): N: Magnitude contaminated by a close object
Byte-by-byte Description of file: tab6-8
Bytes Format Units Label Explanations
1- 5 A5 --- Field Field name 7- 9 I3 --- Nf Photometric catalogue sequential number 11- 15 F5.2 mag Bmag B magnitude 17 I1 --- MType [0/3] Morphological type (1) 19- 23 A5 --- Class Spectral classification 25- 29 F5.3 --- z ? Redshift when extragalactic object 31 I1 ---- Q [2/5] Quality of the spectrum (2) 33- 38 A6 --- Com Comments
Note (1): 0: Star 1: Star ? 2: Star ? (the B curve is not a stellar one) 3: Diffuse source Note (2): 5: very good 4: good spectrum 3: medium 2: bad 1: superposition of spectra
History: Prepared via OCR at CDS.
(End) Marie-Jose Wagner, Patricia Bauer [CDS] 29-Apr-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

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