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: Sc scan:src vex calc wgt ants fr/bs snr missed 0028:NGC1052 + + 0.999 5/5 7/10 10 0030:0234+285 + + 0.997 8/8 16/16 72 0033:NGC1052 + + 0.999 6/6 12/12 18 0035:NGC1052 + + 0.999 6/6 10/12 15 0037:NGC1052 + + 0.999 7/7 10/14 11 0040:NGC1052 + + 0.999 8/8 10/16 14 0042:NGC1052 + + 0.999 8/8 10/16 14 0045:NGC1052 + + 0.999 8/8 9/16 19 0049:NGC1052 + + 0.999 8/8 11/16 24 0052:NGC1052 + + 0.999 8/8 12/16 21 0056:0106+013 + + 0.999 9/9 18/18 202 0059:NGC1052 + + 0.999 9/9 10/18 21 0062:NGC1052 + + 0.999 9/9 12/18 16 0065:NGC1052 + + 0.170 9/9 5/18 11 0069:0420-014 + . . 0/8 . . 0072:NGC1052 + . . 0/9 . . 0075:NGC1052 + . . 0/9 . . 0078:NGC1052 + . . 0/9 . . 0082:0106+013 + + 0.999 9/9 18/18 111 0085:NGC1052 + + 0.999 9/9 14/18 10 0089:NGC1052 + + 0.999 9/9 10/18 12 0092:NGC1052 + + 0.999 9/9 5/18 10 0096:0106+013 + + 0.999 9/9 18/18 35 0099:NGC1052 + + 0.991 9/9 5/18 10 0102:NGC1052 + + 0.999 9/9 6/18 10 0105:NGC1052 + + 0.996 9/9 2/18 10 0109:0420-014 + + 0.995 9/9 18/18 431 0112:NGC1052 + + 0.999 9/9 2/18 8 0115:NGC1052 . . . 0/0 . . 0118:NGC1052 . . . 0/0 . . 0121:0420-014 + + 0.999 9/9 18/18 212 0124:NGC1052 . . . 0/0 . . 0127:NGC1052 . . . 0/0 . . 0130:NGC1052 . . . 0/0 . . 0133:0420-014 + + 0.999 9/9 18/18 120 0136:NGC1052 . . . 0/0 . . 0139:NGC1052 . . . 0/0 . . 0142:NGC1052 . . . 0/0 . . 0145:0420-014 . . . 0/0 . . 0148:0420-014 . . . 0/0 . . 0223:BLLAC + + 0.999 7/7 14/14 202 0226:BLLAC + + 0.999 7/7 14/14 126 0228:NGC0315 + + 0.998 8/8 6/16 10 0230:NGC0315 + + 0.999 8/8 9/16 14 0232:BLLAC + + 0.999 8/8 16/16 199 0234:NGC0315 + + 0.999 8/8 11/16 11 0236:NGC0315 + + 0.999 8/8 9/16 10 0238:BLLAC + + 0.999 9/9 18/18 225 0240:NGC0315 + + 0.999 8/8 10/16 13 0242:NGC0315 + + 0.999 8/8 16/16 16 0244:NGC0315 + + 0.999 8/8 9/16 11 0246:BLLAC + + 0.999 9/9 18/18 262 0248:NGC0315 + + 0.999 8/8 9/16 9 0250:NGC0315 + + 0.999 8/8 14/16 13 0252:NGC0315 + + 0.999 8/8 16/16 12 0254:NGC0315 + + 0.999 8/8 16/16 12 0256:BLLAC + + 0.999 9/9 18/18 336 0258:NGC0315 + + 0.999 9/9 13/18 10 0260:NGC0315 + + 0.999 9/9 16/18 12 0262:NGC0315 + + 0.999 9/9 12/18 11 0264:BLLAC + + 0.999 9/9 18/18 248 0266:NGC0315 + + 0.999 9/9 18/18 10 0268:NGC0315 + + 0.999 9/9 16/18 11 0270:NGC0315 + + 0.999 9/9 10/18 11 0272:BLLAC + + 0.999 9/9 18/18 152 0274:NGC0315 + + 0.999 9/9 3/18 9 0276:NGC0315 + + 0.999 9/9 11/18 9 0278:NGC0315 + + 0.999 9/9 15/18 11 0280:BLLAC + + 0.999 9/9 16/18 79 0282:NGC0315 + + 0.155 9/9 0/18 0 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 Sc NGC1052 22 19 0.955 308 308 162 15 Sc 0234+285 1 1 0.997 16 16 16 72 Sc 0106+013 3 3 0.999 54 54 54 116 Sc 0420-014 4 3 0.998 54 54 54 255 Sc BLLAC 9 9 0.999 152 152 150 207 Sc NGC0315 21 21 0.959 356 356 239 11 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 Sc 60 56 0.969 90 940 940 675 72 85