AGASC ID 261624456

Info

Last Obs. 2024:224:20:20
magcatalog 7.26 ± 0.02
mag3 arcsec 7.27 ± 0.01
mag5 arcsec 7.27 ± 0.01
Nobs 32 (0 bad)
fok 100.0%
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 mag ⟩ 100s ⟨ mag ⟩ σmag Comments
3714 2003:024:03:11:05.979 7 297.5 -468.2 1142 1038 0 100.0% 100.0% 100.0% 100.0% 0.01 7.27 0.00 --
60346 2004:068:00:29:10.650 1 183.5 304.3 88 52 0 100.0% 100.0% 100.0% 100.0% 0.00 7.26 0.00 --
5957 2005:033:07:23:56.197 5 354.2 -427.3 9902 9847 6 100.0% 100.0% 100.0% 100.0% 0.01 7.27 0.00 --
5958 2005:051:20:47:40.670 4 468.7 -301.1 1123 1064 0 100.0% 100.0% 100.0% 100.0% 0.01 7.27 0.00 --
5959 2005:210:12:22:51.943 7 -329.7 491.0 8928 8868 4 100.0% 100.0% 100.0% 100.0% 0.01 7.28 0.00 --
5960 2005:220:07:50:56.042 5 -384.8 448.7 1114 1060 2 99.9% 100.0% 100.0% 99.9% 0.01 7.28 0.00 --
6474 2006:025:13:07:51.923 6 306.9 -462.1 1124 1056 0 100.0% 100.0% 100.0% 100.0% 0.01 7.27 0.00 --
6475 2006:219:11:40:22.589 4 -378.6 453.9 10189 10121 2 100.0% 100.0% 100.0% 100.0% 0.01 7.28 0.00 --
14255 2012:105:16:51:55.180 5 372.7 444.4 1124 1063 1 100.0% 100.0% 100.0% 100.0% 0.01 7.27 0.00 --
15459 2013:073:17:29:38.925 5 380.6 -23.8 687 626 0 100.0% 100.0% 100.0% 100.0% 0.01 7.28 0.00 --
15460 2013:073:17:56:28.925 5 362.4 -23.8 687 625 0 100.0% 100.0% 100.0% 100.0% 0.01 7.28 0.00 --
15461 2013:073:18:23:18.925 6 344.2 -23.8 684 623 1 99.8% 100.0% 100.0% 99.8% 0.01 7.28 0.00 --
15462 2013:073:18:50:08.925 5 317.0 -23.9 682 628 0 100.0% 100.0% 100.0% 100.0% 0.01 7.28 0.00 --
15463 2013:073:19:16:58.925 5 289.8 -24.1 683 623 0 100.0% 100.0% 100.0% 100.0% 0.01 7.28 0.00 --
15464 2013:073:19:43:48.925 5 262.6 -24.3 689 638 0 100.0% 100.0% 100.0% 100.0% 0.01 7.28 0.00 --
16374 2014:115:17:21:54.662 7 317.4 488.5 1129 1049 0 100.0% 100.0% 100.0% 100.0% 0.01 7.29 0.00 --
17323 2016:100:19:09:33.701 5 424.2 392.9 9905 9847 6 100.0% 100.0% 100.0% 100.0% 0.01 7.27 0.00 --
19838 2017:094:00:09:26.716 7 482.1 311.6 9905 9840 6 100.0% 100.0% 100.0% 100.0% 0.02 7.26 0.00 --
19839 2017:220:05:53:05.168 6 -381.0 445.7 9899 9842 6 100.0% 100.0% 100.0% 100.0% 0.01 7.26 0.00 --
49658 2017:314:17:21:24.109 2 -243.2 390.3 2528 2473 2 100.0% 100.0% 100.0% 100.0% 0.01 7.25 0.00 --
21794 2019:093:16:06:39.533 6 451.4 299.2 1479 1429 0 100.0% 100.0% 100.0% 100.0% 0.01 7.25 0.00 --
21795 2019:093:17:00:39.533 6 427.0 299.2 1477 1425 1 100.0% 100.0% 100.0% 100.0% 0.01 7.25 0.00 --
21796 2019:093:17:54:39.533 6 347.6 298.1 974 928 2 100.0% 100.0% 100.0% 100.0% 0.01 7.25 0.00 --
21797 2019:093:18:31:29.533 6 336.0 298.2 973 923 0 100.0% 100.0% 100.0% 100.0% 0.01 7.25 0.00 --
21798 2019:093:19:08:19.533 6 324.4 298.3 973 928 0 100.0% 100.0% 100.0% 100.0% 0.01 7.26 0.00 --
21799 2019:093:19:45:09.533 6 312.2 298.4 972 923 0 100.0% 100.0% 100.0% 100.0% 0.02 7.26 0.00 --
21800 2019:093:20:21:59.533 5 256.6 297.7 972 928 0 100.0% 100.0% 100.0% 100.0% 0.01 7.26 0.00 --
21801 2019:093:20:58:49.533 5 229.1 297.5 972 923 1 100.0% 100.0% 100.0% 100.0% 0.01 7.26 0.00 --
21802 2019:093:21:35:39.533 5 202.0 297.4 972 928 2 100.0% 100.0% 100.0% 100.0% 0.01 7.26 0.00 --
24941 2021:047:10:36:35.312 5 439.7 -343.5 3808 3725 1 100.0% 100.0% 100.0% 100.0% 0.02 7.25 0.00 --
29142 2024:021:21:48:44.754 4 282.3 -482.5 850 794 0 99.9% 100.0% 100.0% 99.9% 0.02 7.27 0.00 --
29452 2024:224:20:20:55.181 5 -350.1 469.3 2662 2613 0 100.0% 100.0% 100.0% 100.0% 0.02 7.29 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.