AGASC ID 652618520

Info

Last Obs. 2022:241:14:09
magcatalog 8.92 ± 0.06
mag3 arcsec 8.96 ± 0.02
mag5 arcsec 8.96 ± 0.02
Nobs 13 (0 bad)
fok 98.3%
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
51149 2016:088:03:34:41.132 3 169.6 221.0 28 28 0 100.0% 100.0% 100.0% 100.0% 0.01 8.95 0.00 --
23829 2021:097:15:01:30.560 5 156.6 232.5 6909 6778 4 98.1% 100.0% 100.0% 98.1% 0.04 8.95 0.00 --
25000 2021:098:05:26:55.912 7 157.2 232.1 6423 6240 8 97.2% 99.9% 100.0% 97.1% 0.08 8.95 0.00 --
25001 2021:098:20:23:15.438 7 157.4 232.1 10783 10516 4 97.5% 100.0% 100.0% 97.5% 0.07 8.96 0.00 --
24357 2021:100:13:58:38.054 5 155.4 232.9 8848 8648 15 97.7% 100.0% 100.0% 97.7% 0.07 8.97 0.00 --
25004 2021:101:13:43:40.351 5 156.0 232.7 8559 8436 12 98.6% 100.0% 100.0% 98.6% 0.07 8.96 0.00 --
24356 2021:103:18:12:11.226 6 65.4 277.4 13726 13554 13 98.7% 100.0% 100.0% 98.7% 0.09 8.96 0.00 --
24352 2021:117:01:06:44.978 5 -202.7 207.9 12282 12020 23 97.9% 100.0% 100.0% 97.8% 0.05 8.98 0.00 --
24355 2021:219:10:23:36.724 4 -268.2 -82.9 11775 11670 13 99.1% 100.0% 100.0% 99.1% 0.05 8.96 0.00 --
24353 2021:236:05:00:37.345 4 -255.4 -110.2 7372 7308 11 99.1% 100.0% 100.0% 99.1% 0.03 8.95 0.00 --
25023 2022:101:06:29:07.991 7 98.5 265.7 9357 9211 8 98.5% 100.0% 100.0% 98.5% 0.05 8.98 0.00 --
24354 2022:241:05:22:15.036 6 -232.0 -148.0 8351 8231 5 98.6% 100.0% 100.0% 98.6% 0.10 8.96 0.00 --
27328 2022:241:14:09:09.604 6 -244.2 -129.5 5654 5532 9 97.8% 100.0% 100.0% 97.8% 0.06 8.97 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.