AGASC ID 897610120

Info

Last Obs. 2024:190:13:51
magcatalog 8.61 ± 0.06
mag3 arcsec 8.46 ± 0.02
mag5 arcsec 8.46 ± 0.02
Nobs 13 (0 bad)
fok 99.6%
f3 arcsec 99.7%
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 mag ⟩ 100s ⟨ mag ⟩ σmag Comments
3800 2002:294:03:21:17.041 7 -49.0 363.6 12995 12832 8 99.1% 100.0% 100.0% 99.1% 0.01 8.44 0.00 --
2797 2002:312:05:33:21.893 6 -406.2 -489.5 24248 24178 12 100.0% 100.0% 100.0% 100.0% 0.02 8.46 0.00 --
4451 2004:199:10:34:38.886 4 -63.7 361.5 5020 4949 7 99.9% 100.0% 100.0% 99.9% 0.03 8.44 0.00 --
4452 2004:212:17:56:19.266 4 -49.7 363.6 9902 9828 9 99.9% 100.0% 100.0% 99.9% 0.02 8.44 0.00 --
4453 2004:223:03:50:48.058 4 -44.0 364.3 19654 19587 18 99.9% 100.0% 100.0% 99.9% 0.02 8.44 0.00 --
7534 2008:047:03:38:25.817 5 -165.8 -358.7 2584 2516 2 100.0% 100.0% 100.0% 100.0% 0.01 8.44 0.00 --
16748 2015:150:02:18:13.239 7 484.2 429.7 14775 14596 6 99.3% 100.0% 100.0% 99.3% 0.02 8.46 0.00 --
22389 2020:045:03:54:19.690 5 27.2 -335.9 22097 21825 17 99.1% 100.0% 100.0% 99.1% 0.05 8.47 0.00 --
23158 2020:046:11:03:03.262 5 27.2 -335.9 14777 14618 24 99.4% 100.0% 100.0% 99.3% 0.04 8.47 0.00 --
28007 2024:169:04:40:18.816 3 461.6 455.5 3485 3420 1 100.0% 100.0% 100.0% 99.9% 0.07 8.49 0.00 --
29456 2024:169:18:56:50.769 3 465.8 450.9 3223 3150 1 100.0% 99.9% 100.0% 99.9% 0.05 8.48 0.00 --
29457 2024:171:01:41:02.045 3 478.7 437.1 3807 3729 0 99.9% 100.0% 100.0% 99.9% 0.06 8.48 0.00 --
29480 2024:190:13:51:19.078 3 -480.2 -427.2 3447 3397 184 100.0% 87.9% 99.9% 87.8% 0.10 8.50 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.