AGASC ID 684985848

Info

Last Obs. 2022:253:23:24
magcatalog 9.14 ± 0.09
mag3 arcsec 9.16 ± 0.02
mag5 arcsec 9.16 ± 0.02
Nobs 11 (0 bad)
fok 98.4%
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 mag ⟩ 100s ⟨ mag ⟩ σmag Comments
10406 2009:268:08:50:07.969 4 -238.6 -274.2 22340 21784 37 97.5% 100.0% 100.0% 97.5% 0.02 9.15 0.00 --
12000 2009:272:12:12:00.386 4 -219.9 -287.4 36588 36413 46 99.5% 100.0% 100.0% 99.5% 0.05 9.15 0.00 --
10405 2009:275:22:23:01.296 4 -219.9 -287.4 40715 40568 60 99.6% 100.0% 100.0% 99.6% 0.04 9.15 0.00 --
55253 2011:221:14:22:14.245 2 60.8 374.9 48 48 0 100.0% 100.0% 100.0% 100.0% 0.00 9.17 0.00 --
21506 2019:252:09:50:23.825 5 -303.3 -144.0 15210 14854 25 97.7% 100.0% 100.0% 97.6% 0.06 9.18 0.00 --
22842 2019:255:01:56:38.842 5 -279.7 -179.4 26903 26220 27 97.5% 100.0% 100.0% 97.4% 0.10 9.16 0.00 --
23551 2021:102:13:45:58.168 5 -173.8 -470.5 8366 8234 12 98.4% 99.9% 100.0% 98.3% 0.06 9.14 0.00 --
25008 2021:103:01:56:56.116 5 -174.6 -470.1 9829 9768 19 99.4% 100.0% 100.0% 99.3% 0.05 9.14 0.00 --
23552 2021:158:04:12:04.262 5 -110.3 -487.1 19601 18955 37 96.7% 100.0% 100.0% 96.7% 0.05 9.15 0.00 --
46103 2021:248:23:32:09.464 4 -386.3 186.2 265 256 0 96.6% 100.0% 100.0% 96.6% 0.03 9.20 0.00 --
27342 2022:253:23:24:33.785 7 -363.3 -175.4 4942 4766 48 96.4% 99.2% 99.6% 95.6% 0.07 9.19 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.