AGASC ID 648813664

Info

Last Obs. 2024:104:16:40
magcatalog 8.28 ± 0.08
mag3 arcsec 8.36 ± 0.01
mag5 arcsec 8.36 ± 0.01
Nobs 14 (0 bad)
fok 99.9%
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
4178 2003:215:20:11:10.932 6 471.1 -204.9 13554 13475 5 100.0% 100.0% 100.0% 100.0% 0.01 8.35 0.00 --
5823 2005:332:10:32:49.641 3 -428.1 279.7 19647 19567 17 99.9% 100.0% 100.0% 99.9% 0.03 8.36 0.00 --
5822 2005:333:10:23:43.849 3 -428.5 279.0 9896 9828 5 100.0% 100.0% 100.0% 100.0% 0.03 8.36 0.00 --
7242 2006:060:15:39:03.055 3 -465.5 202.7 18430 18377 13 100.0% 100.0% 100.0% 100.0% 0.01 8.37 0.00 --
6804 2006:148:06:48:20.570 3 -311.0 -446.0 5019 4964 8 99.9% 100.0% 100.0% 99.9% 0.01 8.36 0.00 --
7691 2007:055:18:58:01.149 3 -469.3 228.7 2974 2929 3 99.9% 100.0% 100.0% 99.9% 0.01 8.36 0.00 --
10424 2009:059:01:21:32.091 3 -413.4 63.4 2576 2529 8 99.8% 100.0% 100.0% 99.8% 0.01 8.35 0.00 --
10425 2009:059:03:11:52.912 3 -354.8 259.1 2577 2529 4 100.0% 100.0% 100.0% 100.0% 0.02 8.34 0.00 --
52944 2014:067:04:11:56.093 0 -245.0 250.4 1308 1256 0 99.2% 100.0% 100.0% 99.2% 0.02 8.33 0.00 --
48308 2019:084:12:24:02.171 1 -166.8 -157.3 3130 2651 12 99.2% 99.9% 100.0% 99.1% 0.02 8.34 0.00 --
46445 2021:093:20:34:46.230 2 99.9 241.1 824 764 0 99.5% 99.9% 100.0% 99.3% 0.02 8.36 0.00 --
46440 2021:094:06:13:59.956 1 94.8 -277.0 2536 2448 4 98.6% 100.0% 100.0% 98.6% 0.02 8.37 0.00 --
45043 2022:329:04:22:00.893 1 202.5 462.4 833 753 0 97.9% 100.0% 100.0% 97.9% 0.02 8.35 0.00 --
29363 2024:104:16:40:10.574 4 -206.6 -201.5 3500 3456 1 99.9% 100.0% 100.0% 99.9% 0.05 8.38 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.