AGASC ID 1052777408

Info

Last Obs. 2026:008:14:25
magcatalog 8.26 ± 0.02
mag3 arcsec 8.29 ± 0.02
mag5 arcsec 8.29 ± 0.02
Nobs 13 (0 bad)
fok 99.6%
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
4971 2003:320:22:28:04.206 6 348.9 -213.8 12383 12324 4 100.0% 100.0% 100.0% 100.0% 0.01 8.28 0.00 --
10919 2009:185:13:50:08.712 6 -268.8 444.5 630 573 1 99.8% 100.0% 100.0% 99.8% 0.01 8.27 0.00 --
13122 2010:249:22:09:43.158 6 261.4 436.1 5027 4954 3 100.0% 100.0% 100.0% 100.0% 0.02 8.28 0.00 --
13485 2012:055:10:44:24.607 3 398.6 356.0 30435 30353 41 99.9% 100.0% 100.0% 99.9% 0.02 8.26 0.00 --
50279 2017:058:10:21:00.372 0 360.6 116.8 424 358 0 99.7% 100.0% 100.0% 99.7% 0.02 8.27 0.00 --
47433 2020:055:08:54:06.000 2 468.6 183.3 837 745 1 96.1% 100.0% 100.0% 96.1% 0.02 8.25 0.00 --
24640 2020:260:15:18:19.384 7 488.7 286.6 9907 9797 17 99.8% 100.0% 100.0% 99.8% 0.03 8.26 0.00 --
25362 2022:143:11:43:01.242 3 -445.3 259.3 18283 18119 9 99.4% 100.0% 100.0% 99.4% 0.04 8.30 0.00 --
25363 2022:144:17:40:30.161 3 -445.8 259.6 9895 9750 10 99.2% 100.0% 100.0% 99.2% 0.03 8.30 0.00 --
26427 2022:145:06:41:58.698 3 -445.7 259.5 10044 9867 7 98.8% 100.0% 100.0% 98.8% 0.03 8.31 0.00 --
29999 2026:001:19:50:20.725 3 242.2 -497.3 5460 5401 3 100.0% 100.0% 100.0% 100.0% 0.08 8.32 0.00 --
32081 2026:006:17:11:07.011 3 247.1 -495.4 3484 3424 1 100.0% 99.6% 100.0% 99.6% 0.06 8.32 0.00 --
30226 2026:008:14:25:30.975 3 246.2 -494.9 3024 2959 0 100.0% 100.0% 100.0% 100.0% 0.05 8.33 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.