VII/110A/table3Revised northern "Abell Catalog"recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintACO[1,2712]+ "Abell" numbermeta.id;meta.mainintprimaryindexedRAB1950right ascension (B1950)pos.eq.ra;meta.mainDEB1950declination (B1950)pos.eq.dec;meta.mainBMtype[- I:] cluster classification in the Bautz- Morgan systemsrc.class.structcharCount[0,] number of cluster members between m3 and m3+2, corrected for backgroundctmeta.numberintXposrectangular coordinates of the apparent cluster center, referred to the south-east (lower left) edge of the Palomar Sky Survey prints (x coordinate)mmpos.cartesian.x;instr.plateintYpossame with above (y coordinate)mmpos.cartesian.y;instr.plateintGLONgalactic longitude l2degpos.galactic.lonGLATgalactic latitude b2degpos.galactic.latfloatz? cluster redshift from Struble and Rood (1987ApJS...63..555S)src.redshiftfloatnullableRichrichness, from Abell (1958ApJS....3..211A)src.class.richnessintDclassdistance class, from Abell (1958)src.class.distanceintm10red magnitude of the tenth brightest cluster member, from Abell (1958)magphot.magfloat_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
VII/110A/table5Supplementary southern clustersNF_2[1,4]? same with NF_1meta.noteintnullableObs_2[ACO] same with Obs_1meta.notecharu_m3[:?*] same with u_m1meta.code.errorcharrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintS[S]! prefix to the supplementary southern cluster numbermeta.id.part;meta.maincharACOS[1,1174]+ "Abell" number for supplementary southern clustermeta.idintprimaryindexedRAB1950+= right ascension (B1950)pos.eq.ra;meta.mainDEB1950declination (B1950)pos.eq.dec;meta.mainField[0-9F]! the Southern Sky Survey Field number in which the cluster is locatedmeta.id;obs.fieldcharXcenrectangular coordinates if the apparent cluster center, referred to the CENTER of the Southern Sky Survey Field (+ = east)mmpos.cartesian.x;instr.plateintYcensame with above (+ = north)mmpos.cartesian.y;instr.plateintAtype[ IR?:] cluster classification in Abell's system: I = irregular, R = regular, IR and RI = intermediate, ":" and "?" see file "\begin{tex}\vFile{VII/110A/./docu.txt}{docu.txt}\end{tex}"meta.notecharBMtype[- I:?]! cluster classification in the Bautz-Morgan systemsrc.class.structcharCountnumber of cluster members between m3 and m3+2, corrected for background (as a result of "universal" correction, it can be negative, see paper p11)ctmeta.numberintu_Count[:*?)] uncertainty of the Countmeta.code.error;phot.countcharm1weighted mean total V mag. estimated for the first-ranked cluster member (no galactic extinction correction has been applied)magphot.mag;em.opt.Vfloatu_m1[:?*] ":" = s.d. of more than +-0.5mag "?" = s.d. of more than +-1.0mag "*: = known or probable foreground objectmeta.code.errorcharm3weighted mean total V magnitude estimated for the third-ranked cluster member (again uncorrected)magphot.mag;em.opt.Vfloatm10weighted mean total V magnitude estimated for the tenth-ranked cluster member (again uncorrected)magphot.magfloatu_m10[:?*] same with u_m1meta.code.errorcharPrev[ BDdKOQRSs] sources of previous listings B = Braid and MacGillivray (1978MNRAS.182..241B), etc. see file "\begin{tex}\vFile{VII/110A/./docu.txt}{docu.txt}\end{tex}"meta.notecharXposrectangular coordinates of the apparent cluster center, referred to the south-east (lower left) edge of the Southern Sky Survey Field (x coordinate)mmpos.cartesian.x;instr.plateintYpossame with above (y coordinate)mmpos.cartesian.y;instr.plateintGLONgalactic longitude l2degpos.galactic.lonGLATgalactic latitude b2degpos.galactic.latfloatz? cluster redshift from Struble and Rood (1987ApJS...63..555S)src.redshiftfloatnullableu_z[)] uncertainty parenthesis, closemeta.code.error;src.redshiftcharRichrichness, from Abell (1958ApJS....3..211A)src.class.richnessintDclassdistance class, from Abell (1958)src.class.distanceintm10Amagnitude of the tenth brightest cluster member, corrected for galactic extinction following Abell's formulamagphot.magfloatNF_1[1,4] number of fields in which the cluster was foundmeta.numberintObs_1[ACO]! observer's initial (A = Abell, C = Corwin, O = Olowin)obs.observerchar_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
VII/110A/table6Overlap zone clustersDclassdistance class, from Abell (1958)src.class.distanceintrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintABELL[1,2712] "Abell" number for the clusters in the 10 deg overlap zone (-17 to -27 deg)meta.id;meta.mainintRAB1950+= right ascension (B1950)pos.eq.ra;meta.mainDEB1950declination (B1950)pos.eq.dec;meta.mainField[0-9F]! the Southern Sky Survey Field number in which the cluster is locatedmeta.id;obs.fieldcharXcenrectangular coordinates if the apparent cluster center, referred to the CENTER of the Southern Sky Survey Field (+ = east)mmpos.cartesian.x;instr.plateintYcensame with above (+ = north)mmpos.cartesian.y;instr.plateintAtype[ IR?:]! cluster classification in Abell's system: I = irregular, R = regular, IR and RI = intermediate, ":" and "?" see file "\begin{tex}\vFile{VII/110A/./docu.txt}{docu.txt}\end{tex}"meta.notecharBMtype[- I:?] cluster classification in the Bautz-Morgan systemsrc.class.structcharCountnumber of cluster members between m3 and m3+2, corrected for backgroundctmeta.numberintu_Count[:*?)] uncertainty of the Countmeta.code.error;phot.countcharm1weighted mean total V mag. estimated for the first-ranked cluster member (no galactic extinction correction has been applied)magphot.mag;em.opt.Vfloatu_m1[:?*] ":" = s.d. of more than +-0.5mag "?" = s.d. of more than +-1.0mag "*: = known or probable foreground objectmeta.code.errorcharm3weighted mean total V magnitude estimated for the third-ranked cluster member (again uncorrected)magphot.mag;em.opt.Vfloatu_m3[:?*] same with u_m1meta.code.errorcharm10weighted mean total V magnitude estimated for the tenth-ranked cluster member (again uncorrected)magphot.magfloatu_m10[:?*] same with u_m1meta.code.errorcharPrev[ BDdKOQRSs] sources of previous listings B = Braid and MacGillivray (1978MNRAS.182..241B), etc. see file "\begin{tex}\vFile{VII/110A/./docu.txt}{docu.txt}\end{tex}"meta.notecharXposrectangular coordinates of the apparent cluster center, referred to the south-east (lower left) edge of the Southern Sky Survey Field (x coordinate)mmpos.cartesian.x;instr.plateintYpossame with above (y coordinate)mmpos.cartesian.y;instr.plateintGLONgalactic longitude l2degpos.galactic.lonGLATgalactic latitude b2degpos.galactic.latfloatz? cluster redshift from Struble and Rood (1987ApJS...63..555S)src.redshiftfloatnullableu_z[)] uncertainty parenthesis, closemeta.code.error;src.redshiftcharRichrichness, from Abell (1958ApJS....3..211A)src.class.richnessintm10Amagnitude of the tenth brightest cluster member, corrected for galactic extinction following Abell's formulamagphot.mag;arith.difffloatNF_1[1,4] number of fields in which the cluster was foundmeta.numberintObs_1[ACO]! observer's initial (A = Abell, C = Corwin, O = Olowin)obs.observercharNF_2[1,4]? same with NF_1meta.noteintnullableObs_2[ACO] same with Obs_1meta.notechar_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
VII/110A/notesNotes to tables 4, 5 and 6.ACO[1,4076]? "Abell" numbermeta.id;meta.mainintnullablerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintPrefix[AS] prefix to the "Abell" cluster number blank for Abell number from table4.dat 'A' for Abell number from table6.dat 'S' for Abell number from table5.datmeta.id.part;meta.maincharField[ 0-9F] the Southern Sky Survey Field number in which the cluster is locatedmeta.id;obs.fieldcharNotesNotes for tables 4-6meta.notechar
VII/110A/table4Southern "Abell Catalog"Ycensame with above (+ = north)mmpos.cartesian.y;instr.plateintrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintACO[2713,4076]+ "Abell" number for the southern rich clustermeta.id;meta.mainintprimaryindexedRAB1950+= right ascension (B1950)pos.eq.ra;meta.mainDEB1950declination (B1950)pos.eq.dec;meta.mainField[0-9F]! the Southern Sky Survey Field number in which the cluster is locatedmeta.id;obs.fieldcharXcenrectangular coordinates if the apparent cluster center, referred to the CENTER of the Southern Sky Survey Field (+ = east)mmpos.cartesian.x;instr.plateintAtype[ IR?:]! cluster classification in Abell's system: I = irregu lar, R = regular, IR and RI = intermediate, ":" and "?" see file "\begin{tex}\vFile{VII/110A/./docu.txt}{docu.txt}\end{tex}"meta.notecharBMtype[- I:?]! cluster classification in the Bautz-Morgan systemsrc.class.structcharCount[0,] number of cluster members between m3 and m3+2, corrected for backgroundctmeta.numberintu_Count[:*?)] uncertainty of the Countmeta.code.error;phot.countcharm1? weighted mean total V mag. estimated for the first-ranked cluster member (no galactic extinction correction has been applied)magphot.mag;em.opt.Vfloatnullableu_m1[:?*] ":" = s.d. of more than +-0.5mag "?" = s.d. of more than +-1.0mag "*: = known or probable foreground objectmeta.code.errorcharm3weighted mean total V magnitude estimated for the third-ranked cluster member (again uncorrected)magphot.mag;em.opt.Vfloatu_m3[:?*] same with u_m1meta.code.errorcharm10weighted mean total V magnitude estimated for the tenth-ranked cluster member (again uncorrected)magphot.magfloatu_m10[:?*] same with u_m1meta.code.errorcharPrev[ BDdKOQRSs] sources of previous listings B = Braid and MacGillivray (1978MNRAS.182..241B), etc. see file "\begin{tex}\vFile{VII/110A/./docu.txt}{docu.txt}\end{tex}"meta.idcharXposrectangular coordinates of the apparent cluster center, referred to the south-east (lower left) edge of the Southern Sky Survey Field (x coordinate)mmpos.cartesian.x;instr.plateintYpossame with above (y coordinate)mmpos.cartesian.y;instr.plateintGLONgalactic longitude l2degpos.galactic.lonGLATgalactic latitude b2degpos.galactic.latfloatz? cluster redshift from Struble and Rood (1987ApJS...63..555S)src.redshiftfloatnullableu_z[)] uncertainty parenthesis, closemeta.code.error;src.redshiftcharRichrichness, from Abell (1958ApJS....3..211A)src.class.richnessintDclassdistance class, from Abell (1958)src.class.distanceintm10Amagnitude of the tenth brightest cluster member, corrected for galactic extinction following Abell's formulamagphot.mag;arith.difffloatNF_1[1,4] number of fields in which the cluster was foundmeta.numberintObs_1[ACO]! observer's initial (A = Abell, C = Corwin, O = Olowin)obs.observercharNF_2[1,4]? same with NF_1meta.noteintnullableObs_2[ACO] same with Obs_1meta.notecharNF_3[1,4]? same with NF_1meta.noteintnullableObs_3[ACO] same with Obs_1meta.notechar_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