AGASC ID 375526240

Info

Last Obs. 2025:219:12:21
magcatalog 8.75 ± 0.02
mag3 arcsec 8.77 ± 0.02
mag5 arcsec 8.77 ± 0.02
Nobs 13 (0 bad)
fok 98.9%
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
60004 2004:290:05:24:51.836 4 410.7 -393.1 3727 3681 6 100.0% 100.0% 100.0% 100.0% 0.02 8.77 0.00 --
17065 2015:187:05:17:24.313 4 -107.5 -265.1 4047 3996 2 100.0% 100.0% 100.0% 100.0% 0.03 8.76 0.00 --
17268 2015:335:11:05:00.300 3 -139.7 475.1 2581 2475 3 97.9% 100.0% 100.0% 97.9% 0.02 8.76 0.00 --
17269 2015:335:12:38:37.771 3 -306.4 432.8 2576 2532 2 100.0% 100.0% 100.0% 100.0% 0.02 8.75 0.00 --
17261 2015:335:21:44:35.377 5 360.7 403.6 2587 2525 2 99.9% 100.0% 100.0% 99.9% 0.03 8.79 0.00 --
17264 2015:335:23:45:30.906 5 176.2 320.1 2583 2496 6 98.7% 100.0% 100.0% 98.7% 0.03 8.77 0.00 --
17262 2015:341:11:46:46.658 5 406.6 340.2 2589 2489 4 98.5% 100.0% 100.0% 98.5% 0.02 8.77 0.00 --
20525 2018:010:23:32:01.932 3 324.2 -76.1 4057 3956 2 99.2% 100.0% 100.0% 99.2% 0.03 8.77 0.00 --
23064 2019:311:11:36:50.487 5 445.4 -31.9 11974 11739 20 98.6% 100.0% 100.0% 98.6% 0.03 8.79 0.00 --
22888 2019:333:23:14:12.645 5 267.8 375.5 15267 14952 17 98.4% 100.0% 100.0% 98.4% 0.08 8.75 0.00 --
23084 2019:334:17:24:42.563 4 255.9 384.1 15269 14992 22 98.7% 100.0% 100.0% 98.7% 0.04 8.76 0.00 --
42224 2025:216:21:02:09.206 6 142.5 -291.4 2025 1971 1 99.8% 100.0% 100.0% 99.8% 0.05 8.84 0.00 --
42216 2025:219:12:21:44.453 6 147.7 -289.0 2056 2008 8 99.8% 100.0% 100.0% 99.8% 0.05 8.84 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.