AGASC ID 896012968

Info

Last Obs. 2022:243:04:26
magcatalog 8.75 ± 0.11
mag3 arcsec 8.66 ± 0.01
mag5 arcsec 8.66 ± 0.01
Nobs 36 (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
5508 2005:157:23:36:36.873 4 168.5 135.1 546 546 3 100.0% 100.0% 100.0% 100.0% 0.02 8.68 0.00 --
6622 2006:259:18:19:42.733 3 246.4 70.9 5487 5017 8 99.9% 100.0% 100.0% 99.9% 0.02 8.66 0.00 --
6708 2007:041:08:28:02.738 4 292.8 376.6 11958 11947 15 99.9% 100.0% 100.0% 99.9% 0.02 8.66 0.00 --
8521 2007:062:21:37:33.365 4 292.8 376.6 12760 12747 19 99.9% 100.0% 100.0% 99.9% 0.02 8.67 0.00 --
7504 2008:039:15:33:41.732 6 14.9 425.1 2518 2517 2 100.0% 100.0% 100.0% 100.0% 0.02 8.67 0.00 --
7521 2008:039:17:31:01.863 3 -92.1 -316.4 3095 3094 4 100.0% 100.0% 100.0% 100.0% 0.02 8.64 0.00 --
8648 2008:137:13:23:44.633 4 378.7 -286.0 1068 1067 1 99.9% 100.0% 100.0% 99.9% 0.01 8.68 0.00 --
8647 2008:137:14:05:34.633 3 221.3 -346.8 1065 1063 4 99.8% 100.0% 100.0% 99.8% 0.02 8.67 0.00 --
8659 2008:137:21:03:54.633 4 354.3 -452.2 1067 1065 4 99.8% 100.0% 100.0% 99.8% 0.02 8.67 0.00 --
55445 2011:131:17:42:32.425 2 368.1 302.4 46 46 0 100.0% 100.0% 100.0% 100.0% 0.01 8.67 0.00 --
55436 2011:134:09:08:40.717 2 368.1 302.4 47 47 0 100.0% 100.0% 100.0% 100.0% 0.00 8.67 0.00 --
55430 2011:137:00:35:38.306 2 368.1 302.4 45 45 0 100.0% 100.0% 100.0% 100.0% 0.01 8.67 0.00 --
55425 2011:139:16:04:34.379 2 368.1 302.4 78 77 0 100.0% 100.0% 100.0% 100.0% 0.01 8.66 0.00 --
55420 2011:142:06:47:03.039 2 368.1 302.4 43 43 0 100.0% 100.0% 100.0% 100.0% 0.01 8.67 0.00 --
12689 2011:195:15:25:58.807 4 -275.4 -378.8 77322 77233 103 99.9% 100.0% 100.0% 99.9% 0.02 8.66 0.00 --
13509 2011:203:13:52:31.019 4 -275.6 -378.6 27809 27785 31 99.9% 100.0% 100.0% 99.9% 0.02 8.66 0.00 --
13704 2012:212:01:54:45.586 3 414.4 -436.0 12287 12281 10 100.0% 100.0% 100.0% 100.0% 0.02 8.68 0.00 --
51913 2015:125:05:18:50.599 2 327.4 348.3 267 267 0 100.0% 100.0% 100.0% 100.0% 0.01 8.66 0.00 --
17652 2015:129:20:45:50.857 5 327.4 348.3 13000 12963 13 99.7% 100.0% 100.0% 99.7% 0.02 8.66 0.00 --
16948 2015:195:15:15:42.695 5 -313.4 -350.6 19601 19465 21 99.3% 100.0% 100.0% 99.3% 0.03 8.66 0.00 --
17702 2015:196:04:47:32.505 5 -313.4 -350.6 18312 18267 11 99.8% 100.0% 100.0% 99.7% 0.02 8.66 0.00 --
51751 2015:196:15:54:40.907 2 -313.4 -350.6 30 30 0 100.0% 100.0% 100.0% 100.0% 0.00 8.67 0.00 --
17699 2015:198:10:46:33.136 5 -313.4 -350.6 9846 9803 7 99.6% 100.0% 100.0% 99.6% 0.03 8.66 0.00 --
17663 2015:205:03:54:19.533 5 -313.4 -350.6 28293 28212 23 99.7% 100.0% 100.0% 99.7% 0.03 8.67 0.00 --
17705 2015:206:14:05:55.547 5 -313.4 -350.6 4953 4932 11 99.6% 100.0% 100.0% 99.6% 0.03 8.66 0.00 --
17700 2015:243:16:15:31.423 4 -379.2 -283.0 7391 7385 9 99.9% 100.0% 100.0% 99.9% 0.03 8.67 0.00 --
18354 2015:244:20:52:13.224 4 -379.2 -283.0 15007 14991 16 99.9% 100.0% 100.0% 99.9% 0.03 8.67 0.00 --
18958 2017:128:21:45:40.813 7 -168.0 -295.6 559 558 0 100.0% 100.0% 100.0% 100.0% 0.02 8.66 0.00 --
24203 2022:076:19:36:58.451 7 218.7 126.9 2208 2158 0 97.7% 100.0% 100.0% 97.7% 0.04 8.68 0.00 --
24132 2022:103:15:26:29.283 6 -86.5 391.0 2209 2160 1 97.8% 100.0% 100.0% 97.8% 0.03 8.68 0.00 --
24223 2022:106:20:40:26.931 7 -9.7 -185.6 2309 2305 2 99.8% 100.0% 100.0% 99.8% 0.03 8.67 0.00 --
24139 2022:155:02:20:53.549 7 158.6 -119.8 2205 2167 3 98.3% 100.0% 100.0% 98.3% 0.02 8.70 0.00 --
24050 2022:165:16:33:59.569 6 -8.2 -253.8 2662 2655 5 99.7% 100.0% 100.0% 99.7% 0.03 8.67 0.00 --
24051 2022:165:18:21:12.304 7 93.4 -388.0 2667 2622 3 98.3% 100.0% 100.0% 98.3% 0.03 8.69 0.00 --
24013 2022:174:21:30:37.885 5 -474.6 308.6 2668 2612 3 97.9% 100.0% 100.0% 97.9% 0.03 8.68 0.00 --
24008 2022:243:04:26:56.017 7 -296.3 380.0 2671 2608 4 97.6% 100.0% 100.0% 97.6% 0.05 8.65 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.