AGASC ID 167249880

Info

Last Obs. 2023:337:05:13
magcatalog 6.94 ± 0.05
mag3 arcsec 6.95 ± 0.02
mag5 arcsec 6.95 ± 0.02
Nobs 13 (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
24385 2020:323:02:40:34.137 6 -473.7 51.1 13666 13582 8 100.0% 100.0% 100.0% 100.0% 0.02 6.97 0.00 --
24386 2020:325:11:48:18.899 6 -473.7 51.1 12822 12743 8 100.0% 100.0% 100.0% 100.0% 0.02 6.98 0.00 --
24387 2020:326:03:18:19.569 6 -474.4 51.4 9897 9825 6 100.0% 100.0% 100.0% 100.0% 0.02 6.97 0.00 --
24389 2020:331:05:30:44.922 6 -444.1 177.2 7458 7401 6 100.0% 100.0% 100.0% 99.9% 0.01 6.97 0.00 --
24871 2020:331:17:59:45.739 6 -444.9 177.6 7455 7376 4 100.0% 100.0% 100.0% 100.0% 0.01 6.97 0.00 --
24868 2020:336:01:30:20.194 6 357.4 300.0 8927 8854 4 100.0% 100.0% 100.0% 100.0% 0.02 6.94 0.00 --
24388 2020:336:14:52:51.166 6 355.8 300.7 9908 9836 6 100.0% 100.0% 100.0% 100.0% 0.01 6.94 0.00 --
24390 2020:337:04:49:09.061 6 354.7 301.3 9909 9833 10 100.0% 100.0% 100.0% 100.0% 0.01 6.94 0.00 --
24880 2020:338:00:31:01.523 5 453.6 55.0 8779 8710 1 100.0% 100.0% 100.0% 100.0% 0.01 6.94 0.00 --
23406 2020:339:21:55:46.347 5 454.9 54.4 10397 10310 7 100.0% 100.0% 100.0% 100.0% 0.01 6.94 0.00 --
24878 2020:340:14:12:15.106 5 454.9 54.4 11506 11433 10 100.0% 100.0% 100.0% 100.0% 0.02 6.94 0.00 --
24879 2020:341:08:26:07.620 5 453.6 55.0 5028 4954 5 100.0% 100.0% 100.0% 100.0% 0.01 6.94 0.00 --
43928 2023:337:05:13:47.000 4 -110.5 -6.3 1509 1459 0 100.0% 100.0% 100.0% 100.0% 0.02 6.98 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.