AGASC ID 261619992

Info

Last Obs. 2023:171:18:18
magcatalog 9.26 ± 0.11
mag3 arcsec 9.32 ± 0.02
mag5 arcsec 9.32 ± 0.02
Nobs 14 (0 bad)
fok 99.1%
f3 arcsec 99.8%
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
3714 2003:024:03:11:05.979 4 390.0 397.1 1037 1036 0 99.9% 100.0% 100.0% 99.9% 0.03 9.33 0.00 --
3677 2003:205:03:15:57.450 4 -418.2 -351.9 9845 9837 8 99.9% 100.0% 100.0% 99.9% 0.03 9.32 0.00 --
3715 2003:205:09:08:55.457 4 -417.2 -352.9 1067 1066 2 99.9% 99.9% 100.0% 99.8% 0.02 9.32 0.00 --
5045 2004:201:16:01:31.897 4 -432.3 -335.4 1049 1049 0 100.0% 100.0% 100.0% 100.0% 0.04 9.31 0.00 --
5044 2004:201:17:08:30.498 4 -432.1 -335.6 9698 9685 9 99.9% 100.0% 100.0% 99.8% 0.03 9.31 0.00 --
6475 2006:219:11:40:22.589 3 -349.0 -416.6 10174 10001 25 98.3% 98.8% 100.0% 97.1% 0.05 9.31 0.00 --
14370 2012:009:12:42:59.941 4 446.8 327.0 2414 2380 4 98.6% 100.0% 100.0% 98.6% 0.03 9.31 0.00 --
18414 2016:005:19:10:29.746 4 457.7 308.4 1068 1063 0 99.5% 100.0% 100.0% 99.5% 0.05 9.32 0.00 --
18415 2016:005:20:10:54.077 3 360.1 308.0 2040 1994 3 97.7% 100.0% 100.0% 97.7% 0.04 9.31 0.00 --
18365 2016:007:22:31:27.435 4 451.2 318.3 9834 9782 11 99.5% 100.0% 100.0% 99.5% 0.04 9.32 0.00 --
50582 2016:308:02:50:44.301 0 169.2 -319.5 197 195 0 99.0% 100.0% 100.0% 99.0% 0.03 9.36 0.00 --
19838 2017:094:00:09:26.716 4 -382.3 414.4 9842 9770 10 99.3% 100.0% 100.0% 99.3% 0.05 9.30 0.00 --
20707 2018:086:02:17:31.377 7 -276.3 490.2 9844 9603 4 97.6% 100.0% 100.0% 97.6% 0.13 9.31 0.00 --
25615 2023:171:18:18:13.751 7 -472.0 -283.5 2540 2539 0 100.0% 99.6% 100.0% 99.5% 0.12 9.35 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.