AGASC ID 879625512

Info

Last Obs. 2026:206:04:52
magcatalog 8.65 ± 0.02
mag3 arcsec 8.68 ± 0.02
mag5 arcsec 8.68 ± 0.02
Nobs 12 (0 bad)
fok 98.8%
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
58461 2007:085:18:25:58.626 4 393.9 -222.1 5176 5115 9 99.9% 100.0% 100.0% 99.9% 0.02 8.67 0.00 --
22727 2019:346:17:19:45.515 6 333.1 83.4 12346 12163 13 99.2% 100.0% 100.0% 99.2% 0.03 8.66 0.00 --
23096 2019:349:08:46:56.309 6 333.7 76.5 12347 12187 17 99.4% 100.0% 100.0% 99.4% 0.03 8.66 0.00 --
22655 2020:099:15:08:29.480 6 89.7 -285.8 13076 12689 18 97.7% 100.0% 100.0% 97.7% 0.05 8.69 0.00 --
23213 2020:102:05:19:04.268 6 90.1 -286.0 11362 11032 14 97.8% 100.0% 100.0% 97.8% 0.05 8.70 0.00 --
23214 2020:103:09:53:35.123 6 89.3 -285.6 17219 16844 23 98.3% 100.0% 100.0% 98.3% 0.03 8.70 0.00 --
23029 2020:118:14:03:18.250 6 -197.5 -218.4 4093 3988 2 99.0% 100.0% 100.0% 99.0% 0.04 8.68 0.00 --
23235 2020:122:08:20:00.060 6 -198.3 -218.0 7458 7293 11 98.9% 100.0% 100.0% 98.9% 0.04 8.67 0.00 --
23236 2020:122:23:41:21.258 6 -199.1 -217.6 13312 13153 19 99.4% 100.0% 100.0% 99.4% 0.04 8.68 0.00 --
41326 2026:200:22:17:53.437 1 303.4 393.5 1456 1385 0 99.9% 100.0% 100.0% 99.9% 0.05 8.71 0.00 --
41319 2026:203:13:29:14.569 1 309.1 389.1 1934 1866 2 99.9% 100.0% 100.0% 99.9% 0.05 8.70 0.00 --
41307 2026:206:04:52:11.401 1 314.7 384.6 2097 2024 0 99.8% 100.0% 100.0% 99.8% 0.09 8.70 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.