AGASC ID 1174033144

Info

Last Obs. 2022:335:21:05
magcatalog 7.96 ± 0.26
mag3 arcsec 8.53 ± 0.11
mag5 arcsec 8.53 ± 0.11
Nobs 51 (0 bad)
fok 99.5%
f3 arcsec 100.0%
f5 arcsec 100.0%

Timeline

Observation Info

OBSID Time Slot Row Col N Nmag est ok Nout fmag est ok fdr3 fdbox5 fmag est ok 3 ⟨ δ mag100s ⟨ mag ⟩ σmag Comments
4653 2004:192:00:39:52.995 6 -432.9 -263.2 14753 14258 17 99.9% 100.0% 100.0% 99.9% 0.02 8.40 0.00 --
4654 2004:197:07:42:05.987 6 -452.6 -230.2 14363 13864 10 99.7% 100.0% 100.0% 99.7% 0.02 8.41 0.00 --
4495 2004:265:17:23:55.929 7 183.5 339.1 29565 29065 31 99.9% 100.0% 100.0% 99.9% 0.02 8.48 0.00 --
5397 2005:333:22:21:58.714 7 345.9 -104.1 5852 5384 6 100.0% 100.0% 100.0% 100.0% 0.01 8.42 0.00 --
7228 2005:335:12:06:29.161 7 345.9 -104.1 9869 9867 7 100.0% 100.0% 100.0% 100.0% 0.01 8.41 0.00 --
7229 2005:336:08:28:41.666 7 345.9 -104.1 9670 9664 10 99.9% 100.0% 100.0% 99.9% 0.02 8.41 0.00 --
6735 2006:165:18:41:15.139 6 -304.7 -398.8 10827 10801 18 99.8% 100.0% 100.0% 99.7% 0.02 8.52 0.00 --
6736 2006:266:12:36:54.347 7 -427.3 308.2 10790 10722 13 99.4% 100.0% 100.0% 99.3% 0.03 8.61 0.00 --
7648 2007:106:05:26:17.135 7 213.7 -447.6 9676 9187 13 99.9% 100.0% 100.0% 99.9% 0.02 8.69 0.00 --
7649 2007:118:10:08:38.947 5 97.6 -487.2 9348 9342 8 99.9% 100.0% 100.0% 99.9% 0.02 8.56 0.00 --
9493 2008:056:20:18:43.420 7 -141.4 146.5 10027 10011 18 99.8% 100.0% 100.0% 99.8% 0.03 8.67 0.00 --
9496 2008:148:04:44:06.665 7 -307.1 337.3 13258 13242 18 99.9% 100.0% 100.0% 99.9% 0.02 8.68 0.00 --
9860 2008:149:10:08:46.517 7 -307.1 337.3 16059 16044 21 99.9% 100.0% 100.0% 99.9% 0.02 8.68 0.00 --
9499 2008:151:00:21:21.282 7 -459.0 287.8 16267 15774 18 99.9% 100.0% 100.0% 99.9% 0.02 8.70 0.00 --
9861 2008:173:05:06:30.811 7 -349.8 416.1 14044 14036 15 100.0% 100.0% 100.0% 100.0% 0.03 8.54 0.00 --
9497 2008:204:21:59:28.239 7 206.0 362.8 16188 16170 16 99.9% 100.0% 100.0% 99.9% 0.02 8.39 0.00 --
9889 2008:207:13:33:51.664 7 206.0 362.8 13254 13240 21 99.9% 100.0% 100.0% 99.9% 0.02 8.39 0.00 --
9486 2008:212:20:13:42.118 7 -322.5 276.8 19115 19102 21 99.9% 100.0% 100.0% 99.9% 0.02 8.37 0.00 --
9891 2008:214:14:40:47.889 7 -322.5 276.8 10878 10386 20 99.9% 100.0% 100.0% 99.9% 0.02 8.38 0.00 --
9489 2008:247:05:58:47.866 7 -321.5 393.5 28969 28642 45 98.9% 100.0% 100.0% 98.9% 0.02 8.66 0.00 --
9488 2008:249:21:07:22.508 7 -201.5 236.5 29348 29325 37 99.9% 100.0% 100.0% 99.9% 0.03 8.67 0.00 --
14140 2012:101:11:13:42.863 7 257.6 -422.7 5946 5946 3 100.0% 100.0% 100.0% 100.0% 0.02 8.47 0.00 --
20152 2018:170:08:29:37.796 7 -312.1 232.4 12282 12230 19 99.6% 100.0% 100.0% 99.6% 0.03 8.48 0.00 --
20153 2018:225:03:10:20.994 7 17.7 387.1 12268 12218 13 99.6% 100.0% 100.0% 99.6% 0.02 8.49 0.00 --
21177 2019:136:02:44:09.363 6 -274.9 -30.9 14713 14562 21 99.3% 100.0% 100.0% 99.3% 0.03 8.61 0.00 --
22218 2019:137:00:18:05.128 6 -275.1 -30.7 7863 7757 13 99.2% 100.0% 100.0% 99.2% 0.03 8.62 0.00 --
22219 2019:138:17:21:15.982 6 -275.9 -30.5 17165 17011 29 99.4% 100.0% 100.0% 99.4% 0.03 8.63 0.00 --
21178 2019:182:17:39:13.341 6 -243.9 143.6 14726 14428 13 98.3% 100.0% 100.0% 98.3% 0.05 8.44 0.00 --
22272 2019:183:09:57:54.641 6 -243.9 143.6 13738 13514 7 98.7% 100.0% 100.0% 98.7% 0.04 8.44 0.00 --
22273 2019:185:09:46:49.755 6 -245.7 144.6 7890 7804 8 99.5% 100.0% 100.0% 99.5% 0.03 8.43 0.00 --
21179 2019:238:08:17:08.070 6 -73.7 277.5 29344 29136 21 99.4% 100.0% 100.0% 99.4% 0.06 8.60 0.00 --
21180 2019:281:13:31:34.510 7 146.7 238.9 12266 12032 10 98.1% 100.0% 100.0% 98.1% 0.05 8.50 0.00 --
22866 2019:283:16:21:13.065 7 172.2 219.2 8348 8315 9 99.6% 100.0% 100.0% 99.6% 0.03 8.48 0.00 --
22867 2019:284:08:19:38.950 7 172.2 219.0 8839 8762 9 99.1% 100.0% 100.0% 99.1% 0.03 8.47 0.00 --
22310 2020:006:01:42:20.251 7 214.4 -146.6 9826 9766 18 99.4% 100.0% 100.0% 99.4% 0.02 8.67 0.00 --
23117 2020:006:16:58:46.002 7 215.8 -147.2 9842 9762 12 99.2% 100.0% 100.0% 99.2% 0.04 8.67 0.00 --
23118 2020:008:04:01:21.401 7 215.6 -147.0 9825 9802 13 99.8% 100.0% 100.0% 99.8% 0.03 8.66 0.00 --
23119 2020:011:05:50:41.062 7 215.0 -146.8 9839 9790 12 99.5% 100.0% 100.0% 99.5% 0.04 8.64 0.00 --
22311 2020:013:10:52:39.786 7 204.1 -162.2 17161 17073 19 99.5% 100.0% 100.0% 99.5% 0.06 8.60 0.00 --
23126 2020:014:09:48:50.186 7 204.5 -162.4 17162 17053 17 99.4% 100.0% 100.0% 99.4% 0.03 8.59 0.00 --
22846 2020:016:02:18:22.962 7 203.1 -161.8 14723 14679 29 99.7% 100.0% 100.0% 99.7% 0.03 8.58 0.00 --
22847 2020:026:16:09:05.189 7 119.6 -230.5 7399 7380 10 99.8% 100.0% 100.0% 99.7% 0.03 8.47 0.00 --
23131 2020:027:16:28:29.235 6 161.3 -204.1 16652 16529 24 99.3% 100.0% 100.0% 99.2% 0.04 8.45 0.00 --
22312 2020:053:19:38:23.847 7 -12.5 -260.6 14715 14610 11 99.3% 100.0% 100.0% 99.3% 0.03 8.37 0.00 --
22313 2020:066:19:50:32.610 7 -7.5 -260.6 4967 4933 6 99.3% 100.0% 100.0% 99.3% 0.02 8.44 0.00 --
24670 2022:047:05:44:24.468 7 -98.1 -351.9 24452 24106 10 98.6% 100.0% 100.0% 98.6% 0.07 8.38 0.00 --
25128 2022:159:09:03:58.133 6 -346.6 179.2 14704 14608 15 99.3% 100.0% 100.0% 99.3% 0.05 8.38 0.00 --
26959 2022:334:21:42:42.813 6 224.3 -66.6 2983 2917 3 98.8% 100.0% 100.0% 98.8% 0.06 8.59 0.00 --
27583 2022:335:05:08:14.942 6 223.7 -66.2 3475 3361 2 97.7% 99.9% 100.0% 97.6% 0.07 8.59 0.00 --
27584 2022:335:13:07:15.502 6 223.1 -66.0 3460 3413 2 99.5% 100.0% 100.0% 99.5% 0.05 8.59 0.00 --
27585 2022:335:21:05:20.710 6 222.9 -65.8 3457 3400 2 99.2% 100.0% 100.0% 99.2% 0.05 8.57 0.00 --

  • sample: One sample of ACA image telemetry. This could be a real image readout or it could be a null 4x4 image when the ACA is not tracking. Be aware that the sample period is faster for null 4x4 images (1.025 sec) than for typical 6x6 or 8x8 tracked images (2.05 or 4.1 sec respectively).
  • Kalman samples: Subset of samples when ACA could be tracking stars (AOPCADMD == NPNT & AOACASEQ == KALM)
  • dr3: Subset of tracked Kalman samples with radial centroid residual < 3 arcsec. This corresponds to "high quality" readouts. This effectively includes the track subset (AOACFCT == TRAK) because readouts with no TRAK are assigned an infinite centroid residual.
  • dbox5: Subset of tracked Kalman samples with centroid residual within a 5 arcsec box. This corresponds to spatial filter used by the OBC for inclusion in Kalman filter. This effectively includes the track subset (AOACFCT == TRAK) because readouts with no TRAK are assigned an infinite centroid residual.
  • track: Subset of Kalman samples where the image is being tracked (AOACFCT == TRAK)
  • sat_pix: Subset of Kalman samples with saturated pixel flag OK (AOACISP == OK)
  • ion_rad: Subset of Kalman samples with ionizing radiation flag OK (AOACIIR == OK)
  • mag_est_ok: Subset of Kalman samples that have a magnitude estimate (track & ion_rad)
  • n_total: Total number of sample regardless of OBC PCAD status
  • n: Synonym for n_total
  • n_kalman: Number of Kalman samples
  • n_dr3: Number of dr3 samples.
  • n_dbox5: Number of dbox5 samples.
  • n_track: Number of track samples.
  • n_ok_3: Number of (track & sat_pix & ion_rad & dr3) samples
  • n_ok_5: Number of (track & sat_pix & ion_rad & dbox5) samples
  • n_mag_est_ok: Number of (track & ion_rad) samples
  • n_mag_est_ok_3: Number of (track & ion_rad & dr3) samples
  • n_mag_est_ok_5: Number of (track & ion_rad & dbox5) samples
  • f_dr3: Fraction of mag-est-ok samples with centroid residual < 3 arcsec((mag_est_ok & n_dr3)/n_mag_est_ok)
  • f_dbox5: Fraction of mag-est-ok samples with centroid within 5 arcsec box((mag_est_ok & n_dbox5)/n_mag_est_ok)
  • f_mag_est_ok: n_mag_est_ok_3/n_kalman. This is a measure of the fraction of time during an observation that a magnitude estimate is available.
  • f_mag_est_ok_3: n_mag_est_ok_3/n_kalman.
  • f_mag_est_ok_5: n_mag_est_ok_5/n_kalman.
  • f_ok: n_ok_5 / n_kalman. Same as f_ok_5
  • f_ok_3: n_ok_3 / n_kalman. This is a measure of the fraction of time during an observation that the Kalman filter is getting high-quality star centroids.
  • f_ok_5: n_ok_5 / n_kalman. This is a measure of the fraction of time during an observation that the Kalman filter is getting any star centroid at all. This includes measurements out to 5 arcsec box halfwidth, so potentially 7 arcsec radial offset.