AGASC ID 655891488

Info

Last Obs. 2024:358:01:14
magcatalog 6.91 ± 0.02
mag3 arcsec 6.91 ± 0.01
mag5 arcsec 6.91 ± 0.01
Nobs 12 (0 bad)
fok 100.0%
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
4935 2004:007:00:24:12.131 7 242.9 179.6 6735 6669 3 100.0% 100.0% 100.0% 100.0% 0.01 6.91 0.00 --
5793 2005:079:16:55:21.265 5 191.7 257.1 19478 19414 11 99.9% 100.0% 100.0% 99.9% 0.01 6.91 0.00 --
53808 2013:096:07:24:26.631 3 -442.2 96.0 379 335 0 100.0% 100.0% 100.0% 100.0% 0.01 6.93 0.00 --
53796 2013:096:12:16:13.728 3 -442.5 94.3 307 266 0 100.0% 100.0% 100.0% 100.0% 0.00 6.93 0.00 --
53114 2014:003:17:29:11.745 4 -30.6 -231.0 1800 1735 2 99.9% 100.0% 100.0% 99.9% 0.01 6.91 0.00 --
17197 2015:152:06:20:40.134 5 -269.4 -68.2 15152 15085 5 100.0% 100.0% 100.0% 100.0% 0.01 6.92 0.00 --
17670 2015:161:14:55:43.340 5 -269.4 -68.2 25200 25143 11 100.0% 100.0% 100.0% 100.0% 0.01 6.91 0.00 --
51838 2015:162:05:50:36.911 4 -269.4 -68.2 87 47 0 100.0% 100.0% 100.0% 100.0% 0.00 6.92 0.00 --
17669 2015:168:22:15:27.070 5 -269.4 -68.2 14358 14298 10 100.0% 100.0% 100.0% 100.0% 0.01 6.91 0.00 --
50192 2017:092:16:00:13.271 5 -338.7 -125.6 394 342 1 100.0% 100.0% 100.0% 100.0% 0.01 6.91 0.00 --
50180 2017:092:20:50:36.000 5 -338.4 -126.3 318 272 0 100.0% 100.0% 100.0% 100.0% 0.01 6.91 0.00 --
42836 2024:358:01:14:06.000 0 118.0 -211.5 874 830 0 100.0% 100.0% 100.0% 100.0% 0.02 6.97 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.