J/other/Ap/52.369   Blue stellar objects in strip DE=47°    (Erastova, 2009)

Byurakan spectral sky surveys. Blue stellar objects in the strip at δ=+47°. Erastova L.K. <Astrophysics, 52, 369-376 (2009)> =2009Ap.....52..369E 2009Ap.....52..369E
ADC_Keywords: Surveys ; Blue objects ; Photometry ; Redshifts Keywords: extragalactic surveys: Second Byurakan Survey: blue stellar objects Abstract: This is a list of 111 blue stellar objects and individual active galaxies with excess ultraviolet continuum lying within 08h-17h in α and +45° +49° in δ (1950.0). The surveyed objects are classified in terms of activity type. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table1.dat 99 111 List of observed objects notes.dat 80 26 Individual notes -------------------------------------------------------------------------------- Byte-by-byte Description of file: table1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 9 A9 --- Name Byurakan source name (HHMM+DDDA, B1950) 11 A1 --- S/G [sg] stellar or galaxy classification 13- 14 I2 h RAh Right ascension (J2000) 16- 17 I2 min RAm Right ascension (J2000) 19- 23 F5.2 s RAs Right ascension (J2000) 25 A1 --- DE- Declination sign (J2000) 26- 27 I2 deg DEd Declination (J2000) 29- 30 I2 arcmin DEm Declination (J2000) 32- 35 F4.1 arcsec DEs Declination (J2000) 37- 40 A4 --- Surv Survey type 42- 43 I2 arcsec size1 ? Angular dimension for diffuse objects (max) 44 A1 --- --- [*] 45- 46 I2 arcsec size2 ? Angular dimension for diffuse objects (min) 48- 51 F4.1 mag Bmag Visuble blue magnitude 53- 57 F5.2 mag BmagA ? B magnitude according to APM 59- 64 F6.4 --- z ? Redshift 66- 71 A6 --- Type Physical type according to the form of its slit spectrum 73- 81 A9 --- r_z Source of the redshift (1) 83- 92 A10 --- OName Other name 93- 99 A7 --- r_OName Reference for OName (2) -------------------------------------------------------------------------------- Note (1): Source of redshift as follows: HS = Hamburg Survey SBS = Second Byurakan Survey SDSS = Sloan Digital Sky Survey Note (2): References as follows: 4 = 1987ApJS...63..809S 1987ApJS...63..809S Sanduleak et al. 5 = 1989ApJS...70..173S 1989ApJS...70..173S Sanduleak & Pesch 6 = 1989PASP..101.1081S 1989PASP..101.1081S Sanduleak & Pesch 7 = 1989A&A...223L...1G 1989A&A...223L...1G Groote et al. 9 = 2003A&A...400..939E 2003A&A...400..939E Edelmann et al., Cat. J/A+A/400/939 10 = 1995ApJS...98...41P 1995ApJS...98...41P Pesch et al. 11 = 2004ApJS..153..119M 2004ApJS..153..119M Mitchell & Usher, Cat. J/ApJS/153/119 12 = 1999A&AS..139....1T 1999A&AS..139....1T Thuan et al., Cat. J/A+AS/139/1 13 = 1993BSAO...36....5S 1993BSAO...36....5S Stepanian et al. 14 = 1999PASP..111.1099S 1999PASP..111.1099S Stepanian et al. 15 = 1990Afz....33...89S 1990Afz....33...89S Stepanian et al. 16 = 2000BSAO...49...32S 2000BSAO...49...32S Stepanian et al. 17 = 1999ApJS..121....1M 1999ApJS..121....1M McCook & Sion, Cat. III/210, III/235 18 = 1995A&A...293L..21R 1995A&A...293L..21R Reimers et al. 19 = 1995A&AS..110..469B 1995A&AS..110..469B Bade et al., Cat. J/A+AS/110/469 -------------------------------------------------------------------------------- Byte-by-byte Description of file: notes.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 9 A9 --- Name Byurakan source name (HHMM+DDDA, B1950) 11- 80 A70 --- Note Text of the note -------------------------------------------------------------------------------- History: From electronic version of the journal
(End) Patricia Vannier [CDS] 03-Feb-2011
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