AGASC ID 972690344

Info

Last Obs. 2024:209:07:31
magcatalog 6.83 ± 0.02
mag3 arcsec 6.84 ± 0.01
mag5 arcsec 6.84 ± 0.01
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 mag100s ⟨ mag ⟩ σmag Comments
4288 2002:266:12:09:34.000 3 380.5 317.2 4309 4211 2 100.0% 100.0% 100.0% 100.0% 0.01 6.83 0.00 --
21809 2019:206:13:40:54.342 3 145.4 472.8 13928 13863 13 100.0% 100.0% 100.0% 100.0% 0.01 6.82 0.00 --
24582 2021:187:05:16:19.202 3 -171.2 482.7 14776 14715 5 100.0% 100.0% 100.0% 100.0% 0.02 6.84 0.00 --
27012 2023:181:08:27:49.480 6 -388.2 347.0 4478 4433 3 100.0% 100.0% 100.0% 100.0% 0.02 6.83 0.00 --
27927 2023:182:21:32:53.866 7 -398.1 333.5 5208 5153 1 100.0% 100.0% 100.0% 100.0% 0.02 6.83 0.00 --
27106 2023:183:09:31:16.516 7 -399.3 334.1 5249 5175 2 100.0% 100.0% 100.0% 100.0% 0.02 6.83 0.00 --
28459 2024:200:22:15:07.445 7 64.3 494.6 4978 4915 0 100.0% 100.0% 100.0% 100.0% 0.02 6.85 0.00 --
29483 2024:202:16:05:27.836 3 89.4 489.3 2530 2478 2 100.0% 100.0% 100.0% 100.0% 0.01 6.85 0.00 --
62616 2024:206:05:48:25.995 3 108.5 483.3 3751 3699 3 100.0% 100.0% 100.0% 100.0% 0.02 6.85 0.00 --
29489 2024:208:13:38:51.798 3 160.7 465.3 3562 3502 1 100.0% 100.0% 100.0% 100.0% 0.02 6.85 0.00 --
28528 2024:209:07:31:58.632 3 131.1 476.5 3872 3823 1 100.0% 100.0% 100.0% 100.0% 0.02 6.85 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.