AGASC ID 1092235392

Info

Last Obs. 2023:042:12:20
magcatalog 7.71 ± 0.10
mag3 arcsec 7.69 ± 0.01
mag5 arcsec 7.69 ± 0.01
Nobs 12 (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 mag ⟩ 100s ⟨ mag ⟩ σmag Comments
50961 2016:162:04:22:44.923 5 81.8 -270.6 625 624 0 99.8% 100.0% 100.0% 99.8% 0.01 7.70 0.00 --
24767 2021:017:15:54:45.833 6 433.8 -207.4 14720 14711 10 99.9% 100.0% 100.0% 99.9% 0.03 7.68 0.00 --
24944 2021:032:12:25:11.119 7 348.5 -331.9 6542 6509 5 99.5% 100.0% 100.0% 99.5% 0.02 7.69 0.00 --
23032 2021:037:07:07:04.630 7 348.9 -332.1 7869 7865 6 99.9% 100.0% 100.0% 99.9% 0.02 7.69 0.00 --
23030 2021:135:12:39:26.319 7 -137.0 -466.0 11775 11687 14 99.3% 100.0% 100.0% 99.2% 0.02 7.68 0.00 --
25034 2021:135:21:00:15.346 7 -136.8 -466.0 10687 10667 9 99.8% 100.0% 100.0% 99.8% 0.02 7.68 0.00 --
23031 2021:136:15:20:56.396 7 -137.6 -465.8 12769 12761 5 99.9% 100.0% 100.0% 99.9% 0.03 7.68 0.00 --
24765 2021:157:02:51:21.732 7 -421.1 -264.2 8812 8810 9 100.0% 100.0% 100.0% 100.0% 0.02 7.69 0.00 --
24766 2021:157:18:19:38.206 7 -421.9 -263.8 10962 10959 14 100.0% 100.0% 100.0% 100.0% 0.01 7.69 0.00 --
22699 2021:217:09:17:47.970 7 -407.8 306.5 12314 12307 11 99.9% 100.0% 100.0% 99.9% 0.02 7.70 0.00 --
22700 2021:225:18:11:18.511 7 -384.3 335.6 15365 15342 12 99.9% 100.0% 100.0% 99.9% 0.03 7.70 0.00 --
26517 2023:042:12:20:50.410 5 -265.2 -231.9 2468 2463 1 99.8% 100.0% 100.0% 99.8% 0.03 7.69 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.