AGASC ID 837551376

Info

Last Obs. 2023:264:10:25
magcatalog 9.45 ± 0.07
mag3 arcsec 9.46 ± 0.03
mag5 arcsec 9.46 ± 0.03
Nobs 11 (3 bad)
fok 99.5%
f3 arcsec 99.8%
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
2977 2002:254:00:42:32.835 7 427.3 -365.5 72686 72552 60 99.9% 100.0% 100.0% 99.9% 0.05 9.46 0.00 --
7821 2007:194:11:14:49.531 4 -82.7 160.8 7461 7376 17 99.6% 100.0% 100.0% 99.6% 0.04 9.41 0.00 --
52579 2014:217:20:43:52.410 0 -456.5 201.8 2317 2176 0 95.7% 100.0% 100.0% 95.6% 0.06 9.44 0.00 --
24467 2021:232:19:01:14.178 6 371.4 455.1 14801 14552 12 98.8% 99.8% 100.0% 98.6% 0.13 9.45 0.00 --
24462 2021:234:16:37:16.571 6 371.7 455.0 13321 13045 27 98.6% 99.4% 100.0% 98.0% 0.13 9.46 0.00 --
24782 2023:232:23:21:16.237 6 342.7 477.6 3616 3558 0 99.9% 98.3% 100.0% 98.3% 0.27 9.50 0.00 --
28491 2023:237:07:28:47.105 6 443.4 379.4 3700 3618 279 99.8% 99.8% 100.0% 99.6% 0.23 9.50 0.00 --
28884 2023:253:23:34:20.167 6 442.7 -359.4 2060 1995 16 99.7% 97.5% 100.0% 97.3% 0.10 9.50 0.00 --
24468 2023:262:10:33:20.870 6 310.0 -475.4 0 0 -1 0.0% 0.0% 0.0% 0.0% inf inf inf Error: No level 0 data.
28918 2023:263:22:38:16.722 6 294.4 -486.4 0 0 -1 0.0% 0.0% 0.0% 0.0% inf inf inf Error: No level 0 data.
25991 2023:264:10:25:11.212 6 290.0 -489.7 0 0 -1 0.0% 0.0% 0.0% 0.0% inf inf inf Error: No level 0 data.

  • 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.