AGASC ID 648813840

Info

Last Obs. 2025:084:13:19
magcatalog 9.26 ± 0.02
mag3 arcsec 9.25 ± 0.03
mag5 arcsec 9.25 ± 0.03
Nobs 16 (0 bad)
fok 99.6%
f3 arcsec 99.9%
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 3 -108.5 92.9 13601 13330 18 98.6% 100.0% 100.0% 98.6% 0.02 9.22 0.00 --
5651 2005:153:23:28:28.433 3 -405.8 -415.0 1602 1554 2 99.9% 99.9% 100.0% 99.8% 0.04 9.27 0.00 --
6356 2005:222:07:11:15.670 3 -97.4 92.6 18359 18284 28 99.9% 100.0% 100.0% 99.8% 0.03 9.22 0.00 --
6357 2005:223:16:53:09.990 3 -97.6 92.3 16237 16162 23 99.9% 100.0% 100.0% 99.9% 0.03 9.22 0.00 --
6358 2005:225:06:17:52.871 3 -97.8 92.0 15788 15714 10 99.9% 100.0% 100.0% 99.9% 0.04 9.22 0.00 --
59506 2005:225:16:02:52.188 0 -25.9 -199.9 1652 1608 3 100.0% 99.9% 99.9% 99.9% 0.02 9.22 0.00 --
5823 2005:332:10:32:49.641 4 121.1 -71.7 19650 19564 25 99.9% 100.0% 100.0% 99.9% 0.03 9.27 0.00 --
5822 2005:333:10:23:43.849 4 121.2 -71.5 9900 9821 11 99.9% 100.0% 100.0% 99.9% 0.03 9.27 0.00 --
7242 2006:060:15:39:03.055 4 134.2 -53.2 18436 18372 20 99.9% 100.0% 100.0% 99.9% 0.03 9.29 0.00 --
10424 2009:059:01:21:32.091 4 184.8 -193.2 2584 2531 4 99.9% 100.0% 100.0% 99.9% 0.03 9.28 0.00 --
10426 2009:059:04:43:42.912 3 -10.7 -134.4 2583 2515 5 99.4% 100.0% 100.0% 99.4% 0.04 9.22 0.00 --
10427 2009:059:06:15:32.912 3 47.7 60.4 2592 2507 3 98.6% 99.9% 100.0% 98.5% 0.03 9.27 0.00 --
52944 2014:067:04:11:56.093 1 364.2 21.7 1319 1259 3 99.4% 99.9% 100.0% 99.4% 0.03 9.29 0.00 --
48308 2019:084:12:24:02.171 7 483.6 -206.3 3120 2625 9 98.3% 99.8% 99.9% 98.1% 0.06 9.29 0.00 --
46440 2021:094:06:13:59.956 7 326.2 331.9 2533 2404 12 96.8% 99.7% 100.0% 96.5% 0.05 9.24 0.00 --
30869 2025:084:13:19:42.747 7 384.3 -185.0 1489 1412 0 97.6% 90.2% 99.9% 88.0% 0.09 9.34 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.