AGASC ID 920651808

Info

Last Obs. 2023:075:07:03
magcatalog 7.23 ± 0.03
mag3 arcsec 7.24 ± 0.02
mag5 arcsec 7.24 ± 0.02
Nobs 14 (0 bad)
fok 99.9%
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 mag100s ⟨ mag ⟩ σmag Comments
4168 2003:140:22:40:07.414 3 -459.7 -391.0 22560 22558 16 100.0% 100.0% 100.0% 100.0% 0.01 7.26 0.00 --
4170 2003:144:03:42:45.485 3 -459.5 -190.6 22987 22354 11 100.0% 100.0% 100.0% 100.0% 0.01 7.25 0.00 --
5809 2005:090:16:46:02.266 4 -153.8 -391.9 4031 3487 1 98.3% 99.9% 99.9% 98.2% 0.01 7.24 0.00 --
9526 2008:086:11:54:32.531 4 -46.5 -290.4 20580 20569 15 99.9% 100.0% 100.0% 99.9% 0.01 7.22 0.00 --
18139 2016:123:19:34:23.016 4 -10.4 -241.3 2411 2411 0 100.0% 100.0% 100.0% 100.0% 0.01 7.22 0.00 --
18133 2016:141:15:24:32.410 4 -150.5 -289.4 2716 2715 0 100.0% 100.0% 100.0% 100.0% 0.01 7.22 0.00 --
18128 2016:183:06:03:30.845 4 -206.9 299.8 2445 2444 2 100.0% 100.0% 100.0% 100.0% 0.01 7.22 0.00 --
50911 2016:183:08:15:37.302 1 -206.9 299.8 188 188 0 100.0% 100.0% 100.0% 100.0% 0.01 7.22 0.00 --
18123 2016:232:20:17:24.696 4 -314.5 57.0 2406 2404 1 100.0% 100.0% 100.0% 100.0% 0.01 7.23 0.00 --
18127 2016:249:10:24:34.160 4 283.6 132.5 2415 2415 3 100.0% 100.0% 100.0% 100.0% 0.02 7.23 0.00 --
50727 2016:249:12:21:12.137 1 283.0 132.7 39 39 0 100.0% 100.0% 100.0% 100.0% 0.01 7.23 0.00 --
46409 2021:107:12:04:40.652 1 -294.9 -364.9 467 467 0 100.0% 100.0% 100.0% 100.0% 0.01 7.24 0.00 --
44745 2023:072:14:22:31.880 1 63.8 -241.4 520 520 0 100.0% 100.0% 100.0% 100.0% 0.02 7.25 0.00 --
44734 2023:075:07:03:22.580 1 52.3 -243.8 524 524 0 100.0% 100.0% 100.0% 100.0% 0.01 7.24 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.