This file was generated by ant_rep version 4. --------------------------------------------------------------------------------------------------------------- Column description: 1 (scan: src) - scan number based on the vex file with excluded pointing scans : source name 2 (vex) - indicates if this antenna was included in the vex file for this scan 3 (calc) - indicates if this antenna was included in the correlation of this scan based on precorrelation .calc 4 (wgt) - average weight for this antenna in the scan based on the difx log (for multiple correlations of the same scan only the last correlation is included in the averaging) 5 (ants) - number of antennas correlated for this scan (excluding the given one) / number of antennas in the vex-file for this scan (excluding the given one) 6 (fr/bs) - number of baselines with fringes found by fourfit / number of expected baselines in the correlation (taking into account only parallel hands, i. e. the first number of the previous column is multiplied by two) 7 (snr) - average snr for the found fringes 8 (missed) - explanation of column 5, noting which antennas are actually missing --------------------------------------------------------------------------------------------------------------- Antenna: Ov scan:src vex calc wgt ants fr/bs snr missed 0028:NGC1052 . . . 0/0 . . 0030:0234+285 + + 0.997 8/8 16/16 79 0033:NGC1052 . . . 0/0 . . 0035:NGC1052 . . . 0/0 . . 0037:NGC1052 + + 0.999 7/7 8/14 22 0040:NGC1052 + + 0.999 8/8 8/16 32 0042:NGC1052 + + 0.999 8/8 5/16 44 0045:NGC1052 + + 0.999 8/8 9/16 45 0049:NGC1052 + + 0.998 8/8 10/16 40 0052:NGC1052 + + 0.998 8/8 12/16 49 0056:0106+013 + + 0.999 9/9 18/18 133 0059:NGC1052 + + 0.985 9/9 10/18 25 0062:NGC1052 + + 0.987 9/9 13/18 24 0065:NGC1052 + + 0.988 9/9 10/18 16 0069:0420-014 + + 0.998 6/8 12/12 247 Pt,Sc 0072:NGC1052 + + 0.995 6/9 6/12 11 Pt,Sc,Mk 0075:NGC1052 + + 0.995 6/9 8/12 13 Pt,Sc,Mk 0078:NGC1052 + + 0.998 6/9 6/12 13 Pt,Sc,Mk 0082:0106+013 + + 0.999 9/9 18/18 155 0085:NGC1052 + + 0.999 9/9 10/18 14 0089:NGC1052 + + 0.999 9/9 11/18 17 0092:NGC1052 + + 0.993 9/9 10/18 17 0096:0106+013 + + 0.999 9/9 18/18 127 0099:NGC1052 + + 0.992 9/9 14/18 41 0102:NGC1052 + + 0.999 9/9 16/18 42 0105:NGC1052 + + 0.998 9/9 16/18 45 0109:0420-014 + + 0.999 9/9 18/18 216 0112:NGC1052 + + 0.991 9/9 14/18 45 0115:NGC1052 + + 0.999 7/7 12/14 39 0118:NGC1052 + + 0.999 7/7 12/14 30 0121:0420-014 + + 0.999 9/9 18/18 562 0124:NGC1052 + + 0.999 7/7 12/14 16 0127:NGC1052 + + 0.999 7/7 11/14 15 0130:NGC1052 + + 0.997 7/7 10/14 22 0133:0420-014 + + 0.999 9/9 18/18 472 0136:NGC1052 + + 0.996 6/6 12/12 12 0139:NGC1052 + + 0.999 6/6 6/12 9 0142:NGC1052 + + 0.994 5/5 4/10 9 0145:0420-014 + + 0.999 5/5 10/10 1047 0148:0420-014 + + 0.993 6/6 12/12 834 0223:BLLAC + + 0.999 7/7 14/14 170 0226:BLLAC + + 0.999 7/7 14/14 142 0228:NGC0315 + + 0.999 8/8 0/16 0 0230:NGC0315 + + 0.999 8/8 0/16 0 0232:BLLAC + + 0.999 8/8 16/16 308 0234:NGC0315 + + 0.999 8/8 4/16 8 0236:NGC0315 + + 0.999 8/8 11/16 17 0238:BLLAC + + 0.999 9/9 18/18 125 0240:NGC0315 + + 0.999 8/8 12/16 31 0242:NGC0315 + + 0.999 8/8 16/16 26 0244:NGC0315 + + 0.999 8/8 13/16 27 0246:BLLAC + + 0.999 9/9 18/18 481 0248:NGC0315 + + 0.992 8/8 15/16 32 0250:NGC0315 + + 0.995 8/8 16/16 26 0252:NGC0315 + + 0.999 8/8 16/16 23 0254:NGC0315 + + 0.999 8/8 16/16 29 0256:BLLAC + + 0.999 9/9 18/18 648 0258:NGC0315 + + 0.999 9/9 16/18 38 0260:NGC0315 + + 0.999 9/9 16/18 17 0262:NGC0315 + + 0.999 9/9 14/18 22 0264:BLLAC + + 0.999 9/9 18/18 442 0266:NGC0315 + + 0.999 9/9 18/18 48 0268:NGC0315 + + 0.999 9/9 14/18 10 0270:NGC0315 + + 0.999 9/9 14/18 18 0272:BLLAC + + 0.999 9/9 18/18 731 0274:NGC0315 + + 0.999 9/9 17/18 33 0276:NGC0315 + + 0.999 9/9 15/18 16 0278:NGC0315 + + 0.999 9/9 17/18 16 0280:BLLAC + + 0.999 9/9 16/18 330 0282:NGC0315 + + 0.999 9/9 16/18 28 Final: ------------------------------------------------------------------------------------------------------------- Final statistics per source, column description: 1 (ant) - which antenna 2 (source) - which source 3 (sched) - scheduled, how many scans were scheduled in the vex 4 (prtsp) - participated, how many scans were actually observed based on precorrelation .calc files 5 (wgt) - average weight for this antenna in the correlated scans based on the difx logs (for multiple correlations of the same scan only the last correlation is included in the averaging) 6 (expect) - expected, how many baselines*pols should be found based on participation, only LL and RR are included (unless a linear pol antenna is present), so in most cases should be all possible baselines based on participating antennas times 2 7 (fnd) - found, how many baselines*pols (with fringes or not) are found in the alist file, again, unless a linear pol antenna is present, only LL and RR are included. This is a santity check, must be fnd = expect. 8 (frng) - fringes, how many of fnd have a nonzero fringe code in the alist file 9 (snr) - average snr of frng ------------------------------------------------------------------------------------------------------------- ant source sched prtsp wgt expect fnd frng snr Ov 0234+285 1 1 0.997 16 16 16 79 Ov NGC1052 27 27 0.996 414 414 275 28 Ov 0106+013 3 3 0.999 54 54 54 138 Ov 0420-014 6 6 0.998 88 88 88 522 Ov BLLAC 9 9 0.999 152 152 150 388 Ov NGC0315 21 21 0.999 356 356 276 25 Accumulated: ------------------------------------------------------------------------------------------------------------- Accumulated statistics per antenna, all sources averaged, column description: 1 (ant) - which antenna 2 (sched) - scheduled, how many scans were scheduled in the vex 3 (prtsp) - participated, how many scans were actually observed based on precorrelation .calc files 4 (wgt) - average weight for this antenna in the correlated scans based on the difx logs (for multiple correlations of the same scan only the last correlation is included in the averaging) 5 (%) - participation ratio: prtsp*wgt/sched should be close to 100% in most cases 6 (expect) - expected, how many baselines*pols should be found based on participation, only LL and RR are included (unless a linear pol antenna is present), so in most cases should be all possible baselines based on participating antennas times 2 7 (fnd) - found, how many baselines*pols (with fringes or not) are found in the alist file, again, unless a linear pol antenna is present, only LL and RR are included. This is a santity check, must be fnd = expect. 8 (frng) - fringes, how many of fnd have a nonzero fringe code in the alist file 9 (%) - fringe ratio, frng/fnd 10 (snr) - average snr of frng ------------------------------------------------------------------------------------------------------------- ant sched prtsp wgt % expect fnd frng % snr Ov 67 67 0.998 100 1080 1080 859 80 149