AGASC ID 983307312

Info

Last Obs. 2023:240:20:23
magcatalog 8.54 ± 0.05
mag3 arcsec 8.56 ± 0.02
mag5 arcsec 8.56 ± 0.02
Nobs 11 (0 bad)
fok 99.2%
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
22653 2020:230:20:01:49.109 4 245.3 -7.7 17225 17000 27 99.1% 100.0% 100.0% 99.1% 0.03 8.56 0.00 --
24614 2020:231:20:14:54.475 4 246.8 -8.4 14301 14022 17 98.6% 100.0% 100.0% 98.6% 0.05 8.56 0.00 --
24615 2020:233:10:16:51.820 4 246.4 -8.2 4546 4444 8 99.4% 100.0% 100.0% 99.3% 0.03 8.56 0.00 --
25468 2021:358:18:54:12.939 5 -76.8 -212.0 11125 10932 10 99.0% 100.0% 100.0% 99.0% 0.06 8.55 0.00 --
26244 2021:359:08:19:07.241 5 -78.5 -211.3 11610 11429 13 99.2% 100.0% 100.0% 99.2% 0.06 8.55 0.00 --
65525 2022:091:22:30:30.713 3 -60.3 241.4 8433 8293 9 99.2% 100.0% 100.0% 99.2% 0.02 8.56 0.00 --
25902 2022:229:10:38:47.439 3 230.9 -3.0 14053 13921 15 99.6% 100.0% 100.0% 99.6% 0.05 8.60 0.00 --
25903 2022:353:09:30:14.073 3 -84.2 -209.6 2537 2425 1 98.3% 100.0% 100.0% 98.2% 0.04 8.55 0.00 --
25903 2022:353:09:30:14.073 3 -84.2 -209.4 2468 2425 1 98.3% 100.0% 100.0% 98.2% 0.04 8.55 0.00 --
27614 2022:354:07:07:09.721 3 -82.4 -210.5 2539 2437 1 98.6% 99.9% 100.0% 98.5% 0.05 8.54 0.00 --
25904 2023:198:14:51:57.822 3 134.7 203.3 7652 7596 4 99.9% 100.0% 100.0% 99.9% 0.06 8.54 0.00 --
26372 2023:240:20:23:27.694 3 156.9 -160.8 2044 1988 0 100.0% 100.0% 100.0% 100.0% 0.04 8.57 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.