AGASC ID 894179704

Info

Last Obs. 2026:170:12:13
magcatalog 8.72 ± 0.02
mag3 arcsec 8.73 ± 0.02
mag5 arcsec 8.73 ± 0.02
Nobs 11 (0 bad)
fok 99.8%
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
2677 2002:132:08:59:22.096 6 -78.4 380.9 30844 30762 22 100.0% 100.0% 100.0% 99.9% 0.03 8.71 0.00 --
5469 2005:189:19:05:59.981 3 145.5 -417.5 14336 14260 26 99.9% 100.0% 100.0% 99.9% 0.02 8.75 0.00 --
6337 2005:206:14:37:13.504 3 103.2 -429.9 9714 9651 13 99.9% 100.0% 100.0% 99.9% 0.03 8.75 0.00 --
8984 2008:118:19:08:17.090 3 9.6 472.3 14280 14221 18 100.0% 100.0% 100.0% 100.0% 0.02 8.74 0.00 --
13711 2012:187:14:57:13.890 3 148.6 -417.6 31214 31135 33 99.9% 100.0% 100.0% 99.9% 0.03 8.75 0.00 --
14453 2012:190:06:23:42.086 3 148.6 -417.6 17066 16997 21 99.9% 100.0% 100.0% 99.9% 0.03 8.75 0.00 --
15761 2014:125:19:03:25.818 3 -127.3 372.7 41241 41027 31 99.7% 100.0% 100.0% 99.7% 0.04 8.71 0.00 --
19599 2017:114:23:30:39.294 5 58.3 466.3 14775 14634 19 99.6% 100.0% 100.0% 99.6% 0.03 8.72 0.00 --
19600 2017:184:13:09:32.470 3 194.0 -399.9 14560 14335 15 99.0% 100.0% 100.0% 99.0% 0.03 8.73 0.00 --
49966 2017:184:22:00:53.500 0 191.8 -395.1 170 48 0 100.0% 100.0% 100.0% 100.0% 0.01 8.73 0.00 --
32394 2026:170:12:13:31.090 5 223.6 -47.6 4807 4747 9 99.9% 99.3% 100.0% 99.2% 0.11 8.78 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.