AGASC ID 1090028832

Info

Last Obs. 2024:278:10:14
magcatalog 8.41 ± 0.02
mag3 arcsec 8.42 ± 0.03
mag5 arcsec 8.42 ± 0.03
Nobs 12 (0 bad)
fok 99.3%
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
4559 2004:156:06:10:01.705 4 39.0 334.9 36731 36645 15 100.0% 100.0% 100.0% 100.0% 0.03 8.41 0.00 --
13287 2012:168:13:26:26.191 3 77.4 365.2 5376 5316 9 99.9% 100.0% 100.0% 99.9% 0.02 8.42 0.00 --
54547 2012:168:16:44:25.537 1 77.4 365.2 87 47 0 100.0% 100.0% 100.0% 100.0% 0.01 8.43 0.00 --
23030 2021:135:12:39:26.319 3 351.2 249.1 11860 11519 11 97.9% 100.0% 100.0% 97.9% 0.03 8.40 0.00 --
25034 2021:135:21:00:15.346 3 351.2 249.1 10781 10475 10 98.0% 100.0% 100.0% 98.0% 0.04 8.40 0.00 --
23031 2021:136:15:20:56.396 3 350.5 249.4 12835 12556 21 98.3% 100.0% 100.0% 98.3% 0.03 8.40 0.00 --
25022 2021:178:21:57:51.666 3 290.7 -295.4 12348 12178 15 99.1% 100.0% 100.0% 99.1% 0.04 8.43 0.00 --
27420 2023:069:03:33:54.971 6 -343.1 72.3 7412 7270 3 98.8% 100.0% 100.0% 98.8% 0.03 8.42 0.00 --
27418 2024:228:04:33:55.104 5 316.0 29.9 5639 5566 4 100.0% 100.0% 100.0% 100.0% 0.05 8.45 0.00 --
27351 2024:229:19:16:20.030 6 312.4 -43.1 12971 12893 7 99.9% 100.0% 100.0% 99.9% 0.06 8.48 0.00 --
27419 2024:277:13:19:14.427 7 297.8 -98.9 4240 4171 0 100.0% 100.0% 100.0% 100.0% 0.06 8.46 0.00 --
30464 2024:278:10:14:07.662 7 287.7 -118.6 3077 3012 3 100.0% 100.0% 100.0% 100.0% 0.04 8.46 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.