AGASC ID 185337376

Info

Last Obs. 2024:048:14:27
magcatalog 8.99 ± 0.05
mag3 arcsec 8.95 ± 0.01
mag5 arcsec 8.95 ± 0.01
Nobs 14 (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
10709 2009:129:18:16:32.775 4 -307.1 -463.2 11865 11730 18 99.3% 100.0% 100.0% 99.3% 0.03 8.95 0.00 --
10909 2009:130:18:14:30.500 4 -307.1 -463.2 4538 4453 11 99.4% 100.0% 100.0% 99.4% 0.03 8.95 0.00 --
10710 2009:145:15:00:38.215 4 -331.6 -446.9 7950 7896 12 99.9% 100.0% 100.0% 99.9% 0.02 8.95 0.00 --
10912 2009:147:06:15:54.352 4 -331.6 -446.9 17758 17675 23 99.9% 100.0% 100.0% 99.9% 0.03 8.95 0.00 --
57085 2009:147:16:51:17.623 2 -331.6 -446.9 149 24 0 96.0% 100.0% 100.0% 96.0% 0.00 8.95 0.00 --
10910 2009:155:00:12:15.738 4 -325.2 -451.4 25543 25428 37 99.8% 100.0% 100.0% 99.8% 0.03 8.95 0.00 --
57069 2009:155:15:13:03.852 2 -325.2 -451.4 146 26 0 100.0% 100.0% 100.0% 100.0% 0.01 8.95 0.00 --
55735 2011:015:09:20:47.069 3 -140.8 374.9 86 48 0 98.0% 100.0% 100.0% 98.0% 0.01 8.95 0.00 --
46586 2021:040:23:19:38.483 3 457.2 23.2 828 764 0 98.1% 100.0% 100.0% 98.1% 0.03 8.92 0.00 --
46584 2021:041:04:59:21.564 2 455.9 43.9 348 268 0 96.1% 100.0% 100.0% 96.1% 0.05 8.96 0.00 --
46576 2021:044:00:40:16.650 2 370.8 271.3 592 532 1 98.7% 99.8% 100.0% 98.5% 0.03 8.93 0.00 --
46545 2021:059:11:18:11.186 2 -415.9 -450.4 2317 1831 0 97.1% 100.0% 100.0% 97.1% 0.06 8.96 0.00 --
43702 2024:045:23:07:08.661 4 -167.1 -36.7 813 780 2 99.9% 100.0% 100.0% 99.9% 0.05 9.00 0.00 --
43694 2024:048:14:27:09.454 4 -9.3 -272.4 818 777 1 99.9% 99.9% 100.0% 99.7% 0.05 8.98 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.