AGASC ID 391516224

Info

Last Obs. 2023:327:04:44
magcatalog 9.29 ± 0.04
mag3 arcsec 9.38 ± 0.03
mag5 arcsec 9.38 ± 0.03
Nobs 9 (0 bad)
fok 98.5%
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
61190 2002:137:10:38:41.841 6 257.2 222.5 10295 10203 44 99.6% 100.0% 100.0% 99.6% 0.02 9.37 0.00 --
3014 2002:137:16:43:25.563 7 244.1 234.3 15173 15112 15 99.9% 100.0% 100.0% 99.9% 0.03 9.37 0.00 --
25746 2021:330:20:22:19.837 3 358.8 -349.7 14877 14603 23 98.6% 100.0% 100.0% 98.6% 0.11 9.38 0.00 --
25756 2022:028:21:46:32.578 6 420.4 297.5 7468 7255 9 98.1% 100.0% 100.0% 98.1% 0.06 9.39 0.00 --
26287 2022:029:10:12:24.996 6 420.6 297.4 6979 6761 14 97.9% 100.0% 100.0% 97.8% 0.04 9.40 0.00 --
25755 2022:086:07:29:21.666 6 -163.8 490.0 24535 23988 25 98.1% 100.0% 100.0% 98.1% 0.10 9.37 0.00 --
25751 2022:126:09:02:59.180 6 -267.8 441.0 16387 15887 18 97.3% 100.0% 100.0% 97.3% 0.08 9.40 0.00 --
25745 2023:079:01:24:20.340 6 -171.7 486.8 13627 13366 2 98.4% 100.0% 100.0% 98.4% 0.17 9.36 0.00 --
28933 2023:327:04:44:58.139 6 308.4 -391.2 2533 2480 0 99.9% 100.0% 100.0% 99.9% 0.06 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.