AGASC ID 890504416

Info

Last Obs. 2026:158:22:09
magcatalog 9.44 ± 0.02
mag3 arcsec 9.56 ± 0.06
mag5 arcsec 9.56 ± 0.06
Nobs 14 (0 bad)
fok 97.7%
f3 arcsec 99.1%
f5 arcsec 99.9%

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
16336 2014:021:01:30:01.927 3 -307.8 -233.9 1604 1470 1 95.3% 99.9% 100.0% 95.3% 0.03 9.49 0.00 --
49172 2018:174:19:51:52.101 6 -286.2 307.7 1244 1150 1 98.1% 99.9% 100.0% 98.0% 0.04 9.39 0.00 --
48495 2019:018:10:41:00.043 4 67.7 -415.5 3565 2994 10 97.1% 99.9% 100.0% 97.0% 0.05 9.42 0.00 --
24759 2022:080:08:16:54.738 6 -487.6 349.5 9150 8695 12 95.7% 99.9% 100.0% 95.7% 0.13 9.55 0.00 --
24760 2022:081:22:36:14.628 6 -487.6 349.5 14289 13786 15 96.9% 100.0% 100.0% 96.9% 0.08 9.52 0.00 --
26367 2022:085:03:00:09.583 6 -488.9 350.1 5016 4904 14 99.1% 99.9% 100.0% 99.0% 0.06 9.54 0.00 --
24763 2022:123:12:33:01.128 6 -475.5 366.0 6482 6333 9 98.4% 99.8% 100.0% 98.2% 0.10 9.54 0.00 --
26406 2022:123:21:52:38.242 6 -475.8 366.2 8431 8253 8 98.7% 99.9% 100.0% 98.6% 0.06 9.57 0.00 --
24672 2022:128:18:57:01.774 6 -488.7 350.0 12336 12089 46 98.7% 100.0% 100.0% 98.6% 0.05 9.55 0.00 --
26416 2022:132:02:27:32.380 6 -490.4 350.8 12236 11817 22 97.2% 100.0% 100.0% 97.1% 0.06 9.56 0.00 --
24761 2022:141:20:09:28.767 6 -490.0 350.6 13551 13233 13 98.1% 99.9% 100.0% 98.0% 0.08 9.56 0.00 --
24762 2022:205:22:48:11.296 6 482.5 -309.1 5789 5584 2 97.4% 90.2% 99.2% 87.9% 0.25 9.64 0.00 --
26481 2022:211:12:12:07.772 6 482.2 -308.9 9094 8876 3 98.5% 97.1% 100.0% 95.7% 0.20 9.65 0.00 --
41431 2026:158:22:09:36.538 4 174.4 -127.2 1008 948 1 99.7% 99.1% 99.9% 98.7% 0.12 9.59 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.