AGASC ID 182201632

Info

Last Obs. 2026:026:08:35
magcatalog 7.60 ± 0.02
mag3 arcsec 7.62 ± 0.01
mag5 arcsec 7.62 ± 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
7929 2007:263:19:16:48.444 6 -279.1 142.3 14252 14179 12 100.0% 100.0% 100.0% 100.0% 0.02 7.60 0.00 --
7930 2007:264:03:50:24.736 6 -468.0 189.5 14246 14198 11 100.0% 100.0% 100.0% 100.0% 0.02 7.62 0.00 --
7927 2007:269:17:06:39.134 5 -421.9 376.5 14776 14694 15 99.9% 100.0% 100.0% 99.9% 0.01 7.61 0.00 --
7928 2007:348:05:45:22.382 6 -59.1 278.6 14822 14767 11 100.0% 100.0% 100.0% 100.0% 0.01 7.60 0.00 --
7934 2008:004:16:57:44.085 7 146.8 -16.2 9419 9329 7 100.0% 100.0% 100.0% 100.0% 0.01 7.62 0.00 --
9804 2008:005:11:03:18.776 7 146.8 -16.2 5854 5770 4 100.0% 100.0% 100.0% 100.0% 0.01 7.62 0.00 --
7931 2008:040:23:46:01.918 4 75.7 -74.0 14783 14699 14 100.0% 100.0% 100.0% 100.0% 0.02 7.63 0.00 --
7933 2008:065:16:53:47.386 7 167.7 -492.7 14789 14717 10 99.9% 100.0% 100.0% 99.9% 0.02 7.62 0.00 --
47525 2020:020:21:38:19.919 4 -390.3 73.5 2039 1987 1 99.9% 100.0% 100.0% 99.9% 0.02 7.62 0.00 --
25448 2022:011:15:19:13.956 5 118.3 -240.5 7497 7411 5 99.9% 100.0% 100.0% 99.9% 0.04 7.64 0.00 --
26275 2022:016:00:51:57.956 5 120.2 -241.4 5025 4926 2 99.1% 100.0% 100.0% 99.1% 0.04 7.64 0.00 --
45748 2022:025:03:21:08.846 1 -266.1 372.5 697 645 3 99.5% 100.0% 100.0% 99.5% 0.02 7.63 0.00 --
26288 2022:111:17:18:58.654 4 -87.4 285.4 5027 4943 4 99.9% 100.0% 100.0% 99.9% 0.03 7.63 0.00 --
41764 2026:026:08:35:51.581 1 -135.7 138.9 327 288 1 100.0% 100.0% 100.0% 100.0% 0.02 7.63 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.