AGASC ID 1032978936

Info

Last Obs. 2025:148:04:41
magcatalog 9.01 ± 0.02
mag3 arcsec 8.94 ± 0.02
mag5 arcsec 8.94 ± 0.02
Nobs 11 (0 bad)
fok 97.5%
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
20299 2018:177:18:15:49.798 5 60.4 80.4 56254 53484 43 95.2% 100.0% 100.0% 95.2% 0.08 8.94 0.00 --
21109 2018:180:21:29:06.983 6 62.1 79.6 29911 29129 19 97.7% 100.0% 100.0% 97.7% 0.08 8.94 0.00 --
20302 2018:281:11:55:55.340 6 102.4 -6.8 25583 25202 25 98.7% 100.0% 100.0% 98.7% 0.06 8.96 0.00 --
21871 2018:283:12:30:12.679 6 101.5 -6.4 1517 1410 2 98.1% 100.0% 100.0% 98.1% 0.03 8.96 0.00 --
20303 2019:024:05:54:26.068 3 -127.2 -20.5 18679 18278 21 98.2% 100.0% 100.0% 98.2% 0.08 8.94 0.00 --
22060 2019:025:16:52:49.398 3 -126.9 -20.7 17460 17151 11 98.6% 100.0% 100.0% 98.6% 0.08 8.93 0.00 --
22244 2019:154:20:22:50.410 3 -66.1 101.7 14773 14467 12 98.3% 100.0% 100.0% 98.3% 0.09 8.93 0.00 --
22246 2019:157:02:50:24.653 3 -66.1 101.7 14043 13739 12 98.4% 100.0% 100.0% 98.3% 0.10 8.94 0.00 --
20304 2019:157:15:05:22.629 3 -66.6 101.9 13799 13478 15 98.1% 100.0% 100.0% 98.1% 0.07 8.93 0.00 --
22245 2019:160:15:45:43.829 3 -66.1 101.7 13889 13705 8 99.2% 100.0% 100.0% 99.1% 0.10 8.93 0.00 --
42381 2025:148:04:41:10.870 5 39.4 -108.4 1716 1669 0 99.8% 99.9% 100.0% 99.7% 0.07 9.03 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.