AGASC ID 58724088

Info

Last Obs. 2025:196:12:10
magcatalog 6.62 ± 0.02
mag3 arcsec 6.63 ± 0.02
mag5 arcsec 6.63 ± 0.02
Nobs 11 (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 mag ⟩ 100s ⟨ mag ⟩ σmag Comments
6676 2006:327:05:57:00.273 6 354.8 -410.3 15763 15693 12 100.0% 100.0% 100.0% 100.0% 0.01 6.63 0.00 --
9101 2007:326:15:58:27.139 4 350.8 -414.3 16246 16163 8 100.0% 100.0% 100.0% 100.0% 0.01 6.62 0.00 --
9823 2008:326:19:08:25.084 4 350.3 -414.8 14783 14710 13 100.0% 100.0% 100.0% 100.0% 0.01 6.62 0.00 --
10128 2009:153:21:04:47.963 4 -441.0 373.2 15750 15696 6 100.0% 100.0% 100.0% 100.0% 0.02 6.61 0.00 --
10129 2009:210:05:14:54.796 6 -265.5 -486.7 15753 15699 14 100.0% 100.0% 100.0% 100.0% 0.01 6.62 0.00 --
15700 2014:267:18:46:04.076 6 -116.7 -469.5 6000 5928 0 100.0% 100.0% 100.0% 100.0% 0.01 6.61 0.00 --
17453 2015:201:00:08:22.234 4 -362.6 -434.6 5020 4942 4 100.0% 100.0% 100.0% 100.0% 0.01 6.63 0.00 --
23866 2021:189:21:11:37.856 5 -479.5 -295.2 10381 10302 3 100.0% 100.0% 100.0% 100.0% 0.01 6.64 0.00 --
25085 2021:190:11:44:15.559 5 -480.2 -294.8 10382 10293 6 100.0% 100.0% 100.0% 100.0% 0.02 6.64 0.00 --
23867 2022:132:09:54:28.540 3 -328.6 476.1 21113 21068 6 100.0% 100.0% 100.0% 100.0% 0.02 6.65 0.00 --
30052 2025:196:12:10:04.600 3 -450.9 -338.1 7259 7213 0 100.0% 100.0% 100.0% 100.0% 0.02 6.68 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.