AGASC ID 263462424

Info

Last Obs. 2025:012:00:16
magcatalog 8.88 ± 0.02
mag3 arcsec 8.92 ± 0.02
mag5 arcsec 8.92 ± 0.02
Nobs 14 (0 bad)
fok 99.7%
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
3046 2002:016:05:54:44.574 7 -477.6 442.4 75127 75022 61 99.9% 100.0% 100.0% 99.9% 0.04 8.93 0.00 --
3045 2002:018:15:45:58.100 7 -484.4 430.2 83273 83070 76 99.9% 100.0% 100.0% 99.9% 0.03 8.91 0.00 --
4853 2003:361:09:18:33.932 4 -21.0 283.2 10066 9949 13 99.9% 100.0% 100.0% 99.9% 0.03 8.89 0.00 --
5598 2005:105:05:08:09.873 3 -407.8 -471.4 57258 57157 66 99.9% 100.0% 100.0% 99.9% 0.03 8.91 0.00 --
6268 2005:108:00:21:03.889 3 -407.8 -471.4 12341 12257 15 99.7% 100.0% 100.0% 99.7% 0.02 8.91 0.00 --
25392 2022:030:18:20:09.269 3 -472.0 439.8 12335 12071 10 98.4% 100.0% 100.0% 98.4% 0.06 8.90 0.00 --
25800 2022:031:08:20:36.245 3 -471.9 439.8 14846 14565 15 98.4% 100.0% 100.0% 98.4% 0.04 8.91 0.00 --
25801 2022:031:22:05:28.461 3 -471.9 439.8 9956 9716 5 98.4% 100.0% 100.0% 98.3% 0.06 8.91 0.00 --
30550 2024:366:15:21:03.938 3 -454.9 455.4 1976 1929 1 100.0% 99.9% 100.0% 99.9% 0.09 8.95 0.00 --
30552 2025:003:08:20:57.635 3 -455.0 455.4 2401 2359 1 100.0% 100.0% 100.0% 100.0% 0.05 8.94 0.00 --
30706 2025:006:02:10:47.442 3 -454.0 454.9 3316 3283 2 99.9% 99.8% 100.0% 99.8% 0.11 8.95 0.00 --
30524 2025:008:16:33:52.986 3 -438.3 473.1 3770 3720 0 99.9% 99.9% 100.0% 99.8% 0.07 8.96 0.00 --
30554 2025:011:06:44:07.110 3 -452.6 462.0 2637 2600 1 100.0% 99.8% 100.0% 99.8% 0.06 8.96 0.00 --
30727 2025:012:00:16:58.622 3 -452.5 457.0 2629 2585 2 100.0% 98.4% 100.0% 98.4% 0.09 8.96 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.