AGASC ID 745936792

Info

Last Obs. 2024:224:16:55
magcatalog 8.64 ± 0.02
mag3 arcsec 8.66 ± 0.02
mag5 arcsec 8.66 ± 0.02
Nobs 14 (0 bad)
fok 99.9%
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
10524 2009:044:10:45:45.371 6 355.8 -345.5 4232 4174 6 100.0% 100.0% 100.0% 100.0% 0.02 8.66 0.00 --
57306 2009:044:13:16:29.014 4 355.8 -345.5 157 26 0 100.0% 100.0% 100.0% 100.0% 0.01 8.66 0.00 --
10126 2009:157:04:45:40.733 4 251.6 39.0 23076 22991 37 99.9% 100.0% 100.0% 99.8% 0.02 8.66 0.00 --
11114 2010:082:01:01:48.735 6 386.6 -265.7 17013 16914 29 99.9% 100.0% 100.0% 99.9% 0.02 8.67 0.00 --
14329 2011:234:15:14:00.489 3 -199.6 130.5 7136 7068 10 99.9% 100.0% 100.0% 99.9% 0.03 8.64 0.00 --
55236 2011:234:19:45:29.543 1 -199.6 130.5 83 47 0 100.0% 100.0% 100.0% 100.0% 0.01 8.63 0.00 --
14055 2011:248:11:21:05.029 3 -210.2 114.6 8921 8864 13 99.9% 100.0% 100.0% 99.9% 0.03 8.64 0.00 --
14056 2011:275:12:48:16.316 3 -221.2 89.1 13312 13255 16 99.9% 100.0% 100.0% 99.9% 0.03 8.64 0.00 --
14057 2011:316:08:18:29.469 4 -232.3 43.2 20347 20243 32 99.9% 100.0% 100.0% 99.9% 0.02 8.64 0.00 --
55063 2011:316:20:26:03.292 2 -232.3 43.2 88 45 0 100.0% 100.0% 100.0% 100.0% 0.01 8.65 0.00 --
26682 2024:045:07:44:44.452 5 -241.8 -437.5 2522 2471 0 100.0% 100.0% 100.0% 100.0% 0.05 8.65 0.00 --
29265 2024:045:14:44:22.158 5 -242.0 -437.5 2524 2475 1 100.0% 99.9% 100.0% 99.9% 0.04 8.65 0.00 --
26681 2024:191:02:27:56.081 5 406.8 163.8 6981 6927 3 100.0% 100.0% 100.0% 99.9% 0.10 8.68 0.00 --
29266 2024:224:16:55:40.808 7 190.7 438.7 2528 2467 1 100.0% 100.0% 100.0% 99.9% 0.04 8.68 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.