AGASC ID 575541344

Info

Last Obs. 2025:281:13:35
magcatalog 9.37 ± 0.02
mag3 arcsec 9.37 ± 0.02
mag5 arcsec 9.37 ± 0.02
Nobs 12 (0 bad)
fok 99.2%
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
8452 2006:282:13:42:26.596 7 -194.3 231.1 9909 9821 16 99.9% 100.0% 100.0% 99.9% 0.03 9.37 0.00 --
7282 2006:283:04:29:48.853 7 -194.3 231.1 20614 20509 28 99.9% 100.0% 100.0% 99.9% 0.05 9.37 0.00 --
8451 2006:284:09:35:02.550 7 -194.3 231.1 23567 23433 37 99.8% 100.0% 100.0% 99.8% 0.05 9.37 0.00 --
8450 2006:285:06:46:22.212 7 -194.3 231.1 19178 19067 25 99.8% 100.0% 100.0% 99.8% 0.04 9.37 0.00 --
7281 2006:287:02:05:02.561 7 -194.3 231.1 21124 21015 31 99.8% 100.0% 100.0% 99.8% 0.04 9.37 0.00 --
20877 2017:339:15:42:45.923 6 -287.1 -27.8 12337 12011 21 97.8% 100.0% 100.0% 97.8% 0.10 9.38 0.00 --
19519 2017:341:21:16:53.524 6 -287.0 -27.9 18190 17724 26 97.7% 100.0% 100.0% 97.7% 0.10 9.38 0.00 --
20878 2017:345:02:34:36.018 6 -285.9 -28.4 10390 10118 20 97.9% 100.0% 100.0% 97.9% 0.10 9.37 0.00 --
20904 2017:360:05:01:27.146 5 -270.4 -88.2 17718 17499 31 99.2% 100.0% 100.0% 99.1% 0.07 9.37 0.00 --
19520 2017:363:12:03:21.413 6 -270.7 -88.1 9667 9522 16 99.2% 100.0% 100.0% 99.2% 0.07 9.37 0.00 --
20905 2017:364:02:37:24.244 5 -270.3 -88.3 13620 13436 23 99.2% 99.9% 100.0% 99.1% 0.07 9.37 0.00 --
29988 2025:281:13:35:58.575 7 -144.6 263.5 8624 8553 3 99.9% 100.0% 100.0% 99.8% 0.11 9.42 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.