AGASC ID 480388568

Info

Last Obs. 2025:106:15:01
magcatalog 8.30 ± 0.02
mag3 arcsec 8.31 ± 0.01
mag5 arcsec 8.31 ± 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
7082 2006:306:11:57:55.988 4 -213.0 -341.1 21115 21032 33 99.9% 100.0% 100.0% 99.9% 0.02 8.32 0.00 --
8458 2006:308:23:17:51.468 4 -213.0 -341.1 21607 21512 25 99.9% 100.0% 100.0% 99.9% 0.01 8.32 0.00 --
11080 2009:309:13:05:14.521 6 -219.0 -355.3 8062 7937 7 99.9% 100.0% 100.0% 99.9% 0.02 8.30 0.00 --
11081 2009:359:02:03:11.698 5 203.2 -354.9 6826 6766 11 99.9% 100.0% 100.0% 99.9% 0.01 8.32 0.00 --
56569 2009:359:06:30:43.825 4 203.2 -354.9 154 26 0 100.0% 100.0% 100.0% 100.0% 0.00 8.32 0.00 --
11082 2010:042:08:42:15.958 6 386.5 -165.0 8061 7924 19 99.9% 100.0% 100.0% 99.9% 0.02 8.32 0.00 --
11083 2010:094:13:20:21.047 5 404.0 183.4 7340 7279 12 99.9% 100.0% 100.0% 99.9% 0.01 8.30 0.00 --
56354 2010:094:18:11:42.222 5 404.0 183.4 159 25 0 100.0% 100.0% 100.0% 100.0% 0.00 8.29 0.00 --
11084 2010:141:18:37:48.786 5 78.3 436.4 7462 7386 12 99.9% 100.0% 100.0% 99.9% 0.02 8.30 0.00 --
11085 2010:201:10:34:23.850 7 -295.7 314.0 7467 7393 10 99.9% 100.0% 100.0% 99.9% 0.02 8.29 0.00 --
11086 2010:248:14:58:19.781 7 -428.0 76.9 7858 7801 8 99.9% 100.0% 100.0% 99.9% 0.01 8.32 0.00 --
15803 2014:310:23:05:31.946 5 -207.5 -385.1 72345 72269 67 100.0% 100.0% 100.0% 100.0% 0.03 8.30 0.00 --
30085 2025:104:02:46:09.761 6 204.4 336.8 2534 2481 1 100.0% 100.0% 100.0% 100.0% 0.05 8.35 0.00 --
30902 2025:106:15:01:18.905 6 185.7 348.3 2536 2477 0 100.0% 100.0% 100.0% 100.0% 0.04 8.35 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.