AGASC ID 673457728

Info

Last Obs. 2022:240:12:53
magcatalog 8.34 ± 0.22
mag3 arcsec 8.35 ± 0.03
mag5 arcsec 8.35 ± 0.03
Nobs 13 (0 bad)
fok 99.0%
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
56179 2010:170:21:27:05.078 7 123.2 477.7 50 50 0 100.0% 100.0% 100.0% 100.0% 0.01 8.38 0.00 --
24522 2021:202:01:04:44.613 3 249.7 -396.2 12756 12739 12 99.9% 100.0% 100.0% 99.9% 0.03 8.32 0.00 --
24524 2021:206:14:31:31.809 3 251.5 -397.1 14479 14334 16 99.0% 100.0% 100.0% 99.0% 0.05 8.32 0.00 --
24518 2021:223:04:15:24.297 4 430.9 -179.9 13933 13859 10 99.5% 100.0% 100.0% 99.5% 0.03 8.37 0.00 --
24521 2021:223:21:07:04.887 4 431.4 -180.1 9329 9202 14 98.6% 100.0% 100.0% 98.6% 0.03 8.37 0.00 --
25682 2021:226:22:33:08.529 4 434.6 -181.6 5435 5345 9 98.3% 100.0% 100.0% 98.3% 0.03 8.34 0.00 --
24523 2021:227:23:05:34.937 4 457.7 -118.2 14698 14459 18 98.4% 100.0% 100.0% 98.4% 0.05 8.34 0.00 --
24520 2021:244:07:18:36.504 4 465.4 -79.8 14815 14561 8 99.0% 99.9% 99.9% 98.9% 0.06 8.35 0.00 --
26119 2021:326:00:57:13.084 3 446.4 179.7 5913 5802 7 98.1% 100.0% 100.0% 98.1% 0.06 8.30 0.00 --
26216 2021:327:01:13:11.434 3 466.9 99.3 8836 8710 3 98.6% 100.0% 100.0% 98.6% 0.05 8.32 0.00 --
23439 2022:206:11:35:39.496 5 300.5 -362.9 12280 12242 5 99.7% 100.0% 100.0% 99.7% 0.06 8.38 0.00 --
26478 2022:207:01:00:41.100 5 299.1 -362.3 10328 10317 12 99.9% 100.0% 100.0% 99.9% 0.04 8.39 0.00 --
24519 2022:240:12:53:02.280 7 463.1 -96.9 14996 14819 7 98.8% 100.0% 100.0% 98.8% 0.05 8.34 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.