AGASC ID 574886496

Info

Last Obs. 2023:330:13:02
magcatalog 8.48 ± 0.08
mag3 arcsec 8.49 ± 0.01
mag5 arcsec 8.49 ± 0.01
Nobs 57 (0 bad)
fok 99.7%
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
2933 2002:169:18:38:24.170 3 245.8 92.2 9168 9121 9 100.0% 100.0% 100.0% 100.0% 0.01 8.49 0.00 --
6097 2005:035:23:23:57.208 7 -24.0 -238.0 28436 28370 19 99.9% 100.0% 100.0% 99.9% 0.02 8.49 0.00 --
8189 2007:009:08:03:16.858 7 -193.5 -167.4 30094 30026 25 100.0% 100.0% 100.0% 99.9% 0.03 8.49 0.00 --
8505 2007:012:02:06:30.074 7 -193.5 -167.4 41055 40971 51 99.9% 100.0% 100.0% 99.9% 0.02 8.49 0.00 --
8190 2007:153:02:30:43.379 7 296.2 20.6 28444 28373 26 100.0% 100.0% 100.0% 100.0% 0.02 8.48 0.00 --
10027 2008:278:00:29:15.753 7 -136.5 212.9 9899 9825 11 99.9% 100.0% 100.0% 99.9% 0.02 8.47 0.00 --
10025 2009:107:11:26:03.726 6 247.0 -136.2 9416 9348 16 99.9% 100.0% 100.0% 99.9% 0.02 8.51 0.00 --
10026 2009:119:07:14:11.744 7 268.5 -100.8 9176 9105 14 99.9% 100.0% 100.0% 99.9% 0.02 8.51 0.00 --
10542 2009:175:03:41:56.429 6 217.2 106.2 58687 58532 93 99.8% 100.0% 100.0% 99.8% 0.02 8.48 0.00 --
10543 2009:182:22:17:17.487 7 197.7 152.6 58706 58576 98 99.9% 100.0% 100.0% 99.9% 0.02 8.49 0.00 --
10925 2009:188:08:01:22.759 7 218.9 193.5 22127 22049 34 99.9% 100.0% 100.0% 99.9% 0.02 8.49 0.00 --
10544 2009:188:20:57:39.571 7 218.9 193.5 36400 36320 42 99.9% 100.0% 100.0% 99.9% 0.02 8.49 0.00 --
11104 2010:168:02:52:40.718 6 244.0 88.0 5030 4940 10 99.9% 100.0% 100.0% 99.9% 0.01 8.49 0.00 --
11800 2010:201:15:17:03.136 7 177.8 225.7 8439 8368 11 99.8% 100.0% 100.0% 99.8% 0.02 8.49 0.00 --
10545 2010:209:22:46:51.818 7 138.2 253.4 47098 47006 76 99.9% 100.0% 100.0% 99.9% 0.02 8.49 0.00 --
56102 2010:211:02:18:33.889 5 138.2 253.4 91 43 0 97.7% 100.0% 100.0% 97.7% 0.01 8.49 0.00 --
13796 2012:222:15:23:57.269 6 40.3 271.3 10096 10046 5 100.0% 100.0% 100.0% 100.0% 0.02 8.50 0.00 --
15616 2013:055:22:52:57.732 7 33.2 -245.6 1123 1052 3 99.7% 99.9% 100.0% 99.6% 0.02 8.52 0.00 --
16580 2014:034:19:56:37.073 7 -67.9 -245.7 23266 23180 13 99.9% 100.0% 100.0% 99.9% 0.03 8.49 0.00 --
53039 2014:035:09:36:38.720 7 -67.9 -245.7 98 53 1 100.0% 100.0% 100.0% 100.0% 0.01 8.50 0.00 --
17578 2015:016:13:25:16.111 6 -134.4 -187.7 5023 4967 1 100.0% 100.0% 100.0% 100.0% 0.02 8.49 0.00 --
16023 2015:020:00:11:44.053 6 -164.5 -185.6 5255 5188 6 99.9% 100.0% 100.0% 99.9% 0.02 8.48 0.00 --
17678 2015:172:02:21:29.792 7 242.2 60.9 5029 4924 4 99.6% 100.0% 100.0% 99.6% 0.02 8.49 0.00 --
17164 2015:209:15:39:19.740 7 -73.5 26.5 7946 7897 7 100.0% 100.0% 100.0% 100.0% 0.02 8.48 0.00 --
51720 2015:209:20:38:06.970 6 -73.5 26.5 143 26 0 100.0% 100.0% 100.0% 100.0% 0.01 8.48 0.00 --
18062 2016:026:19:38:21.679 6 -122.0 -175.4 12338 12246 14 99.7% 100.0% 100.0% 99.7% 0.03 8.48 0.00 --
18063 2016:055:00:21:54.783 7 32.9 -199.3 12346 12253 15 99.7% 100.0% 100.0% 99.7% 0.02 8.51 0.00 --
18064 2016:096:15:53:24.234 7 172.3 -131.8 12387 12268 16 99.5% 100.0% 100.0% 99.5% 0.03 8.51 0.00 --
18068 2016:115:19:46:41.574 7 204.0 -180.4 12344 12213 9 99.4% 100.0% 100.0% 99.4% 0.02 8.51 0.00 --
18069 2016:155:21:55:35.092 7 255.0 -31.7 12338 12229 11 99.5% 100.0% 100.0% 99.5% 0.02 8.51 0.00 --
18067 2016:183:23:11:29.114 7 222.7 99.8 12871 12776 20 99.7% 100.0% 100.0% 99.7% 0.02 8.49 0.00 --
18065 2016:211:07:32:34.700 6 109.8 293.1 12338 12095 16 98.6% 100.0% 100.0% 98.6% 0.03 8.49 0.00 --
18066 2016:247:09:54:27.018 6 -68.3 312.6 12446 12322 16 99.9% 100.0% 100.0% 99.9% 0.04 8.49 0.00 --
17860 2016:252:17:18:31.037 5 -64.8 268.3 25472 25286 23 99.8% 100.0% 100.0% 99.8% 0.03 8.48 0.00 --
19791 2016:254:13:27:43.392 5 -63.8 267.8 7705 7536 6 98.4% 100.0% 100.0% 98.4% 0.02 8.48 0.00 --
50715 2016:254:18:17:01.232 5 -65.7 268.6 199 89 0 100.0% 100.0% 100.0% 100.0% 0.01 8.48 0.00 --
19792 2016:255:08:10:47.733 5 -64.6 268.2 16400 16219 14 99.7% 100.0% 100.0% 99.7% 0.02 8.48 0.00 --
18070 2016:282:00:18:20.555 6 -184.9 162.9 12335 12126 8 98.9% 100.0% 100.0% 98.9% 0.04 8.48 0.00 --
18071 2016:308:07:14:38.953 7 -243.7 87.9 12379 12313 19 99.9% 100.0% 100.0% 99.9% 0.03 8.49 0.00 --
18072 2016:336:09:19:58.401 7 -266.8 -20.3 12557 12469 15 99.8% 100.0% 100.0% 99.8% 0.03 8.50 0.00 --
50516 2016:336:17:00:26.347 5 -268.0 -19.7 174 64 0 98.5% 100.0% 100.0% 98.5% 0.00 8.50 0.00 --
19305 2018:048:12:14:10.776 7 119.2 211.0 7952 7785 6 98.9% 100.0% 100.0% 98.9% 0.02 8.49 0.00 --
23460 2020:358:00:32:05.923 7 -249.1 -84.6 2577 2486 5 98.4% 100.0% 100.0% 98.4% 0.06 8.50 0.00 --
23461 2021:013:06:44:41.895 6 -182.2 -181.3 2581 2498 3 98.9% 100.0% 100.0% 98.9% 0.03 8.50 0.00 --
23462 2021:036:21:27:10.169 7 -60.8 -243.8 2589 2486 2 99.0% 100.0% 100.0% 99.0% 0.04 8.49 0.00 --
23463 2021:055:09:31:16.444 6 33.1 -246.2 2590 2435 7 96.8% 100.0% 100.0% 96.8% 0.05 8.53 0.00 --
23464 2021:082:10:58:07.991 6 139.4 -204.1 2588 2498 3 98.9% 100.0% 100.0% 98.9% 0.05 8.52 0.00 --
23465 2021:116:09:43:28.596 7 221.6 -114.5 2591 2486 2 98.7% 100.0% 100.0% 98.7% 0.04 8.54 0.00 --
23466 2021:150:16:01:56.106 6 254.3 7.9 2589 2500 2 99.1% 100.0% 100.0% 99.1% 0.02 8.51 0.00 --
23467 2021:174:08:51:10.882 7 226.5 127.5 2591 2466 3 98.3% 100.0% 100.0% 98.3% 0.02 8.51 0.00 --
23468 2021:204:19:52:25.673 6 131.1 234.1 2587 2511 1 99.3% 100.0% 100.0% 99.3% 0.03 8.51 0.00 --
23469 2021:243:22:57:50.070 7 -59.2 268.6 2578 2509 3 99.8% 100.0% 100.0% 99.8% 0.03 8.52 0.00 --
26111 2021:246:14:58:13.286 7 -24.5 272.9 2583 2504 5 99.0% 100.0% 100.0% 99.0% 0.04 8.51 0.00 --
23470 2021:262:00:26:21.918 6 -123.4 248.3 2821 2744 5 99.2% 100.0% 100.0% 99.2% 0.02 8.51 0.00 --
23471 2021:293:01:23:29.937 7 -217.5 168.8 2581 2497 4 98.9% 100.0% 100.0% 98.9% 0.03 8.53 0.00 --
26663 2023:325:19:55:56.302 3 -264.8 25.4 5479 5426 1 100.0% 100.0% 100.0% 100.0% 0.08 8.51 0.00 --
26664 2023:330:13:02:28.379 3 -263.7 43.8 9841 9789 4 100.0% 100.0% 100.0% 99.9% 0.09 8.51 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.