J/A+AS/113/51/table1Association between IRAS sources and S starsrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintGCGSS[1/1347] GCGSS or Stephenson (1990) number (1)meta.noteintprimaryn_GCGSS[S] If S flag is present, star belongs to Stephenson's (1990) supplementary list (1)meta.notecharRA1950GCGSS right ascension (1950)pos.eq.ra;meta.mainn_RA1950[*] When '*' the seconds were indicated as tenths of minutes in the original tablemeta.notecharDE1950GCGSS declination (1950)pos.eq.dec;meta.mainn_DE1950[*] When '*' the arcseconds were indicated as tenths of arcminutes in the original tablemeta.notecharGCGSSmag[]? GCGSS magnitude, either V or Bmagphot.mag;em.opt.Bfloatnullablen_GCGSSmag[B] When 'B' GCGSS magnitude is Bmeta.notecharRA2[]? GSC right ascension (1950)pos.eq.ranullableDE2[]? GSC declination (1950)pos.eq.decnullableGSCmag[]? GSC magnitude, either V or Bmagphot.mag;em.opt.Bfloatnullablen1_GSCmag[B] When 'B' GSC magnitude is Bmeta.notecharn2_GSCmag[v] When 'v' GSC magnitude is variablemeta.notecharIRASIRAS PSC entrymeta.idcharRA3s[]? IRAS right ascension (1950)spos.eq.ranullableDE3[]? IRAS declination (1950)pos.eq.decnullableR1[]? log(25.F12/12.F25)/log(25/12), where F12 and F25 are the 12 and 25um IRAS fluxesphot.flux;arith.ratiofloatnullablen_R1[:] If present, at least one flux is of quality 2 in IRASmeta.notecharR2[]? log(60.F25/25.F60)/log(60/25), where F25 and F60 are the 25 and 60um IRAS fluxesphot.flux;arith.ratiofloatnullablen1_R2[:] If present, at least one flux is of quality 2meta.notecharSpIRIR spectral class, according to the letter codes defined by Volk & Cohen (2)src.spTypecharLRS[]? LRS spectral classsrc.spTypeintnullableRefsReferences to near IR photometry (3)meta.ref;pos.framecharAssAssociations with other catalogues (4)meta.id.assoccharFlagFlag (5)meta.code.errorchar_RA.icrsRight ascension (ICRS) (computed by VizieR, not part of the original data)pos.eq.ranullableindexed_DE.icrsDeclination (ICRS) (computed by VizieR, not part of the original data)pos.eq.decnullableindexed
J/A+AS/113/51/table2Suspected associationsrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintGCGSSStephenson number (see Note (1) in table1)meta.id;meta.mainintn_GCGSS[S] (see Note (1) in table1)meta.notecharRA1950GCGSS right ascension (1950)pos.eq.ra;meta.mainn_RA1950[*] When '*' the seconds were indicated as tenths of minutes in the original tablemeta.notecharDE1950GCGSS declination (1950)pos.eq.dec;meta.mainn_DE1950[*] When '*' the arcseconds were indicated as tenths of arcminutes in the original tablemeta.notecharGCGSSmag[]? GCGSS magnitude, either V or Bmagphot.mag;em.opt.Bfloatnullablen_GCGSSmag[B] When 'B' GCGSS magnitude is Bmeta.notecharIRASIRAS PSC entrymeta.idcharRA3s[]? IRAS right ascension (1950)spos.eq.ranullableDE3s[]? IRAS declination (1950)arcsecpos.eq.decnullableR1[]? log(25 F12/12 F25)/log(25/12), where F12 and F25 are the 12 and 25um IRAS fluxesphot.flux;arith.ratiofloatnullablen_R1[:] If present, at least one flux is of quality 2meta.notecharR2[]? log(60 F25/25 F60)/log(60/25), where F25 and F60 are the 25 and 60um IRAS fluxesphot.flux;arith.ratiofloatnullablen_R2[:] If present, at least one flux is of quality 2meta.notecharSpIRIR spectral class, according to the letter codes defined by Volk & Cohen (Note (2) in table1)src.spTypecharLRS[]? LRS spectral classsrc.spTypeintnullableRefsReferences to near IR photometry (Note (3) in table1)meta.ref;pos.framecharAssAssociations with other catalogues (Note (4) in table1)meta.id.assoccharFlagFlag (Note (5) in table1)meta.code.errorchar_RA.icrsRight ascension (ICRS) (computed by VizieR, not part of the original data)pos.eq.ranullableindexed_DE.icrsDeclination (ICRS) (computed by VizieR, not part of the original data)pos.eq.decnullableindexed
J/A+AS/113/51/rem1-2Remarks to table1 and table2recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintGCGSS[]? GCGSS number (Note (1) in table1)meta.idintnullableTextRemarksmeta.notechar
J/A+AS/113/51/table3Rejected associationsGSCmag[]? GSC magnitude, either V or Bmagphot.mag;em.opt.BfloatnullablerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintGCGSS[1/1347] GCGSS or Stephenson (1990) number (1)meta.noteintprimaryn_GCGSS[S] If S flag is present, star belongs to Stephenson's (1990) supplementary list (1)meta.notecharRA1950GCGSS right ascension (1950)pos.eq.ra;meta.mainn_RA1950[*] When '*' the seconds were indicated as tenths of minutes in the original tablemeta.notecharDE1950GCGSS declination (1950)pos.eq.dec;meta.mainn_DE1950[*] When '*' the arcseconds were indicated as tenths of arcminutes in the original tablemeta.notecharGCGSSmag[]? GCGSS magnitude, either V or Bmagphot.mag;em.opt.Bfloatnullablen_GCGSSmag[B] When 'B' GCGSS magnitude is Bmeta.notecharRA2[]? GSC right ascension (1950)pos.eq.ranullableDE2[]? GSC declination (1950)pos.eq.decnullablen1_GSCmag[B] When 'B' GSC magnitude is Bmeta.notecharn2_GSCmag[v] When 'v' GSC magnitude is variablemeta.notecharIRASIRAS PSC entrymeta.idcharRA3s[]? IRAS right ascension (1950)spos.eq.ranullableDE3[]? IRAS declination (1950)pos.eq.decnullableR1[]? log(25.F12/12.F25)/log(25/12), where F12 and F25 are the 12 and 25um IRAS fluxesphot.flux;arith.ratiofloatnullablen_R1[:] If present, at least one flux is of quality 2 in IRASmeta.notecharR2[]? log(60.F25/25.F60)/log(60/25), where F25 and F60 are the 25 and 60um IRAS fluxesphot.flux;arith.ratiofloatnullablen1_R2[:] If present, at least one flux is of quality 2meta.notecharSpIRIR spectral class, according to the letter codes defined by Volk & Cohen (2)src.spTypecharLRS[]? LRS spectral classsrc.spTypeintnullableRefsReferences to near IR photometry (3)meta.ref;pos.framecharAssAssociations with other catalogues (4)meta.id.assoccharFlagFlag (5)meta.code.errorchar_RA.icrsRight ascension (ICRS) (computed by VizieR, not part of the original data)pos.eq.ranullableindexed_DE.icrsDeclination (ICRS) (computed by VizieR, not part of the original data)pos.eq.decnullableindexed
J/A+AS/113/51/rem3Remarks to table3IRASIRAS PSC entrymeta.idcharTextRemarksmeta.notecharrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintGCGSS[]? GCGSS or Stephenson number (Note (1) in table1)meta.idintnullablen_GCGSS[S] (see Note (1) in table1)meta.notechar
J/A+AS/113/51/table4aPossibly extended sourcesrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintGCGSS[]? GCGSS or Stephenson number (Note (1) in table1)meta.idintnullablen_GCGSS[S] (see Note (1) in table1)meta.notecharIRASIRAS PSC entrymeta.idcharses1[]? IRAS PSC small extended structure flagmeta.code.errorintnullableTextText of remarksmeta.notechar
J/A+AS/113/51/table4bSources contaminated by cirrus or nearby sourcesIRASIRAS PSC entrymeta.idcharrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintGCGSS[]? GCGSS or Stephenson number (Note (1) in table1)meta.idintnullablen_GCGSS[S] (see Note (1) in table1)meta.notecharses1[]? IRAS PSC small extended structure flagmeta.code.errorintnullableTextText of remarksmeta.notechar