AGASC ID 1093950240

Info

Last Obs. 2024:279:13:42
magcatalog 6.94 ± 0.03
mag3 arcsec 6.98 ± 0.02
mag5 arcsec 6.98 ± 0.02
Nobs 14 (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 mag100s ⟨ mag ⟩ σmag Comments
49997 2017:171:21:14:58.313 6 -90.0 337.4 821 755 7 100.0% 100.0% 100.0% 100.0% 0.01 6.93 0.00 --
27032 2023:032:12:50:51.665 7 -10.4 11.5 3512 3443 1 100.0% 100.0% 100.0% 100.0% 0.03 6.96 0.00 --
27689 2023:034:19:39:57.254 7 -10.7 11.6 3751 3698 0 100.0% 100.0% 100.0% 100.0% 0.03 6.97 0.00 --
27031 2023:266:23:21:29.322 7 -12.3 12.4 4972 4908 1 100.0% 100.0% 100.0% 100.0% 0.03 6.97 0.00 --
27033 2024:029:00:37:19.668 7 -11.7 12.0 2449 2381 4 100.0% 100.0% 100.0% 100.0% 0.03 7.02 0.00 --
29232 2024:029:07:50:29.131 7 -12.9 12.6 3021 2963 1 100.0% 100.0% 100.0% 100.0% 0.02 6.99 0.00 --
29233 2024:029:15:57:06.744 7 -14.4 13.3 3141 3081 0 100.0% 100.0% 100.0% 100.0% 0.02 6.98 0.00 --
29234 2024:030:18:07:40.525 7 -15.5 13.8 2390 2332 0 99.9% 100.0% 100.0% 99.9% 0.02 6.99 0.00 --
29374 2024:111:15:43:55.373 7 -10.1 11.3 6404 6333 1 100.0% 100.0% 100.0% 100.0% 0.03 7.01 0.00 --
26494 2024:112:11:35:22.033 7 -10.2 11.3 3757 3688 1 99.9% 100.0% 100.0% 99.9% 0.03 7.00 0.00 --
27034 2024:164:18:06:08.368 7 -9.1 10.8 4396 4335 0 100.0% 100.0% 100.0% 100.0% 0.02 6.99 0.00 --
29448 2024:167:23:41:30.618 7 -13.0 12.6 4483 4424 0 100.0% 100.0% 100.0% 100.0% 0.02 7.00 0.00 --
30463 2024:277:23:29:57.528 7 -11.5 11.9 4360 4298 0 100.0% 100.0% 100.0% 100.0% 0.03 6.96 0.00 --
27035 2024:279:13:42:39.266 7 -12.0 12.1 3506 3441 4 100.0% 100.0% 100.0% 100.0% 0.02 6.97 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.