AGASC ID 413805792

Info

Last Obs. 2023:326:19:35
magcatalog 7.29 ± 0.05
mag3 arcsec 7.29 ± 0.01
mag5 arcsec 7.29 ± 0.01
Nobs 36 (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 mag100s ⟨ mag ⟩ σmag Comments
2572 2002:212:01:45:50.966 5 -321.1 322.3 32720 32672 11 100.0% 100.0% 100.0% 100.0% 0.01 7.30 0.00 --
4358 2002:223:19:39:13.000 4 -263.4 435.8 2621 2558 0 100.0% 100.0% 100.0% 100.0% 0.01 7.30 0.00 --
4511 2004:016:10:36:34.192 3 213.6 -318.3 47760 47695 21 100.0% 100.0% 100.0% 100.0% 0.02 7.29 0.00 --
10939 2010:025:12:59:26.777 4 129.2 -80.4 16237 16169 16 100.0% 100.0% 100.0% 100.0% 0.01 7.30 0.00 --
56488 2010:025:22:43:57.704 3 129.2 -80.4 166 21 0 100.0% 100.0% 100.0% 100.0% 0.00 7.31 0.00 --
10940 2010:026:11:49:00.939 4 87.8 -163.9 14879 14760 17 100.0% 100.0% 100.0% 100.0% 0.02 7.30 0.00 --
10941 2010:027:18:37:20.635 4 51.8 -248.7 14779 14698 10 100.0% 100.0% 100.0% 100.0% 0.01 7.30 0.00 --
10944 2010:032:10:42:11.476 3 143.0 -446.5 14048 13984 11 100.0% 100.0% 100.0% 100.0% 0.01 7.30 0.00 --
10945 2010:032:19:11:43.146 5 237.4 -471.2 14043 13987 9 100.0% 100.0% 100.0% 100.0% 0.02 7.30 0.00 --
10949 2010:036:04:39:05.259 4 451.3 -426.0 13809 13746 11 100.0% 100.0% 100.0% 100.0% 0.01 7.30 0.00 --
56470 2010:036:12:34:14.212 2 451.3 -426.0 157 24 0 100.0% 100.0% 100.0% 100.0% 0.00 7.30 0.00 --
10950 2010:038:16:52:51.809 4 356.2 -401.3 13751 13689 14 100.0% 100.0% 100.0% 100.0% 0.01 7.30 0.00 --
12099 2010:039:16:56:34.025 5 139.4 -63.6 3590 3450 4 99.9% 100.0% 100.0% 99.9% 0.02 7.30 0.00 --
10951 2010:042:13:43:58.426 5 305.5 -342.7 14686 14616 7 100.0% 100.0% 100.0% 100.0% 0.01 7.30 0.00 --
10952 2010:042:22:25:09.426 4 224.6 -231.2 15078 15016 9 100.0% 100.0% 100.0% 100.0% 0.01 7.30 0.00 --
10953 2010:043:07:03:45.426 5 238.0 -133.7 14539 14475 7 100.0% 100.0% 100.0% 100.0% 0.02 7.30 0.00 --
10957 2010:047:15:34:02.646 4 448.3 -200.1 14971 14888 12 100.0% 100.0% 100.0% 100.0% 0.01 7.30 0.00 --
10958 2010:048:00:37:57.716 4 350.7 -200.2 14981 14919 8 100.0% 100.0% 100.0% 100.0% 0.01 7.29 0.00 --
10962 2010:053:15:42:59.251 3 253.4 -297.3 14784 14720 7 100.0% 100.0% 100.0% 100.0% 0.02 7.29 0.00 --
10971 2010:067:21:11:03.161 6 310.8 195.7 14995 14932 13 100.0% 100.0% 100.0% 100.0% 0.01 7.29 0.00 --
56406 2010:068:06:11:42.456 3 310.8 195.7 160 26 0 100.0% 100.0% 100.0% 100.0% 0.00 7.29 0.00 --
10972 2010:068:19:55:31.440 5 401.5 229.9 14396 14238 14 99.9% 100.0% 100.0% 99.9% 0.01 7.29 0.00 --
12390 2011:025:10:56:10.605 6 168.8 432.7 19950 19895 7 100.0% 100.0% 100.0% 100.0% 0.01 7.30 0.00 --
55695 2011:025:22:37:57.932 4 168.8 432.7 92 47 0 100.0% 100.0% 100.0% 100.0% 0.01 7.30 0.00 --
16622 2014:176:05:07:16.276 4 -118.3 170.3 14045 13973 5 100.0% 100.0% 100.0% 100.0% 0.02 7.28 0.00 --
16659 2015:014:19:49:30.264 4 140.0 -304.4 68587 68502 19 100.0% 100.0% 100.0% 100.0% 0.02 7.30 0.00 --
18788 2016:055:07:53:10.864 4 357.1 -261.4 2586 2515 1 100.0% 100.0% 100.0% 100.0% 0.01 7.30 0.00 --
19607 2017:032:04:43:12.456 3 196.7 -397.9 13954 13844 10 100.0% 100.0% 100.0% 100.0% 0.01 7.29 0.00 --
19700 2017:148:15:35:05.852 7 266.5 379.7 14781 14701 6 100.0% 100.0% 100.0% 100.0% 0.02 7.28 0.00 --
19701 2017:241:01:37:47.074 3 -340.1 330.7 14776 14715 12 100.0% 100.0% 100.0% 100.0% 0.01 7.28 0.00 --
19702 2017:307:05:51:02.605 3 -332.3 -313.4 9901 9834 4 100.0% 100.0% 100.0% 100.0% 0.02 7.28 0.00 --
20836 2017:309:21:07:04.670 3 -332.0 -313.6 5023 4958 7 99.9% 100.0% 100.0% 99.9% 0.01 7.28 0.00 --
19698 2018:075:13:54:50.908 4 440.0 -91.3 15079 14992 3 100.0% 100.0% 100.0% 100.0% 0.02 7.28 0.00 --
20599 2018:231:10:32:29.384 6 -319.4 348.0 14202 14129 14 100.0% 100.0% 100.0% 100.0% 0.02 7.29 0.00 --
20848 2018:275:10:32:36.390 4 -468.5 4.2 13498 13419 6 100.0% 100.0% 100.0% 100.0% 0.01 7.30 0.00 --
29059 2023:326:19:35:21.280 6 -6.5 -181.0 4747 4626 1 100.0% 100.0% 100.0% 100.0% 0.03 7.30 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.