AGASC ID 1165382424

Info

Last Obs. 2023:020:02:26
magcatalog 8.31 ± 0.06
mag3 arcsec 8.35 ± 0.02
mag5 arcsec 8.35 ± 0.02
Nobs 12 (0 bad)
fok 99.8%
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
9573 2007:242:01:39:28.122 6 -25.9 263.7 24958 24943 34 99.9% 100.0% 100.0% 99.9% 0.02 8.34 0.00 --
9574 2007:243:10:37:21.881 6 -25.9 263.7 22321 21839 31 99.9% 100.0% 100.0% 99.9% 0.02 8.34 0.00 --
9571 2007:244:16:05:41.950 6 -25.9 263.7 23021 23006 27 99.9% 100.0% 100.0% 99.9% 0.02 8.34 0.00 --
10123 2009:199:00:16:29.150 5 333.8 119.2 13748 13739 20 99.9% 100.0% 100.0% 99.9% 0.02 8.35 0.00 --
10808 2009:212:19:04:07.839 7 349.8 12.8 14724 14708 25 99.9% 100.0% 100.0% 99.9% 0.02 8.36 0.00 --
10807 2009:259:07:19:09.779 5 237.9 -246.4 13497 13488 22 99.9% 100.0% 100.0% 99.9% 0.02 8.37 0.00 --
10806 2009:261:23:52:21.141 5 237.9 -246.4 13786 13775 24 99.9% 100.0% 100.0% 99.9% 0.02 8.37 0.00 --
18851 2016:137:22:51:58.345 3 49.0 -309.1 16762 16730 16 99.8% 100.0% 100.0% 99.8% 0.03 8.37 0.00 --
51022 2016:138:09:10:18.137 1 49.0 -309.1 26 26 0 100.0% 100.0% 100.0% 100.0% 0.00 8.36 0.00 --
17456 2016:139:11:35:55.988 3 49.0 -309.1 14704 14574 15 99.1% 100.0% 100.0% 99.1% 0.02 8.37 0.00 --
26554 2023:017:18:13:55.488 3 461.6 178.5 4921 4903 6 99.6% 99.9% 100.0% 99.6% 0.04 8.37 0.00 --
27669 2023:020:02:26:00.221 3 461.4 178.5 4182 4164 3 99.6% 100.0% 100.0% 99.5% 0.05 8.38 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.