AGASC ID 837162096

Info

Last Obs. 2023:120:16:49
magcatalog 9.40 ± 0.09
mag3 arcsec 9.48 ± 0.03
mag5 arcsec 9.48 ± 0.03
Nobs 14 (0 bad)
fok 98.7%
f3 arcsec 99.5%
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
55153 2011:274:11:40:53.663 2 185.3 120.3 46 46 0 100.0% 100.0% 100.0% 100.0% 0.00 9.44 0.00 --
24465 2021:221:20:48:44.820 5 -226.3 61.8 14704 14277 9 97.1% 99.9% 100.0% 97.0% 0.12 9.51 0.00 --
24783 2021:224:09:36:03.715 4 -223.6 73.1 14724 14463 26 98.2% 99.9% 100.0% 98.2% 0.07 9.50 0.00 --
24467 2021:232:19:01:14.178 4 -190.4 137.4 14718 14585 26 99.1% 98.4% 100.0% 97.5% 0.15 9.47 0.00 --
24462 2021:234:16:37:16.571 4 -190.2 137.4 13229 13067 20 98.8% 99.6% 100.0% 98.4% 0.11 9.47 0.00 --
23678 2021:237:12:45:36.488 5 -131.3 197.8 13229 13079 24 98.9% 100.0% 100.0% 98.8% 0.07 9.48 0.00 --
25983 2021:238:08:09:22.671 5 -132.5 198.4 12271 12215 27 99.5% 99.9% 100.0% 99.5% 0.06 9.48 0.00 --
24469 2021:240:02:29:47.224 5 -132.1 198.2 12770 12702 13 99.5% 100.0% 100.0% 99.5% 0.08 9.48 0.00 --
24785 2021:243:11:56:19.194 4 -39.0 231.5 16166 16035 9 99.2% 98.5% 100.0% 97.7% 0.20 9.44 0.00 --
24714 2022:010:07:50:26.003 4 212.8 24.8 10792 10486 11 97.2% 100.0% 100.0% 97.2% 0.09 9.48 0.00 --
25991 2023:114:10:43:27.823 6 -220.1 -56.5 3648 3625 6 99.4% 100.0% 100.0% 99.4% 0.11 9.47 0.00 --
24466 2023:118:03:07:17.417 6 -221.8 -49.4 3614 3587 4 99.3% 99.7% 100.0% 98.9% 0.09 9.45 0.00 --
27817 2023:119:18:25:25.453 6 -220.0 -52.6 2525 2499 6 99.0% 98.0% 100.0% 97.0% 0.13 9.43 0.00 --
27814 2023:120:16:49:48.419 6 -223.3 -50.6 3595 3563 1 99.1% 99.9% 100.0% 99.0% 0.11 9.48 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.