AGASC ID 890506624

Info

Last Obs. 2022:211:12:12
magcatalog 8.93 ± 0.05
mag3 arcsec 8.95 ± 0.03
mag5 arcsec 8.95 ± 0.03
Nobs 16 (0 bad)
fok 98.6%
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
14235 2011:230:01:15:38.348 3 458.8 240.6 10249 10237 11 99.9% 100.0% 100.0% 99.9% 0.03 8.92 0.00 --
12331 2011:232:16:04:22.975 3 458.8 240.6 20004 19981 27 99.9% 100.0% 100.0% 99.9% 0.02 8.91 0.00 --
13627 2012:163:03:31:22.732 4 -58.2 251.9 1535 1532 1 99.8% 100.0% 100.0% 99.8% 0.02 8.90 0.00 --
13629 2012:189:01:30:32.694 3 -34.2 255.4 1566 1526 1 97.5% 100.0% 100.0% 97.5% 0.02 8.92 0.00 --
13268 2012:191:01:18:41.748 4 -33.4 255.6 1564 1530 4 97.9% 99.9% 100.0% 97.8% 0.02 8.91 0.00 --
16336 2014:021:01:30:01.927 6 310.2 -216.0 1542 1460 0 94.7% 100.0% 100.0% 94.7% 0.03 8.93 0.00 --
24759 2022:080:08:16:54.738 5 116.7 205.0 9083 8942 11 98.5% 100.0% 100.0% 98.5% 0.04 8.94 0.00 --
24760 2022:081:22:36:14.628 5 116.7 205.0 14231 14071 17 98.9% 100.0% 100.0% 98.8% 0.06 8.97 0.00 --
26367 2022:085:03:00:09.583 5 115.5 205.6 4950 4880 11 98.6% 100.0% 100.0% 98.5% 0.04 8.96 0.00 --
24763 2022:123:12:33:01.128 5 123.3 200.6 6437 6282 7 97.6% 100.0% 100.0% 97.5% 0.05 8.96 0.00 --
26406 2022:123:21:52:38.242 5 123.1 200.6 8361 8099 13 96.9% 100.0% 100.0% 96.9% 0.05 8.96 0.00 --
24672 2022:128:18:57:01.774 5 115.7 205.4 12252 11883 24 97.0% 100.0% 100.0% 97.0% 0.05 8.98 0.00 --
26416 2022:132:02:27:32.380 5 114.1 206.2 12160 11910 16 97.9% 100.0% 100.0% 97.9% 0.06 8.97 0.00 --
24761 2022:141:20:09:28.767 5 114.5 206.0 13487 13390 14 99.3% 100.0% 100.0% 99.3% 0.05 8.96 0.00 --
24762 2022:205:22:48:11.296 5 -125.6 -186.1 5718 5609 1 98.1% 100.0% 100.0% 98.1% 0.06 8.95 0.00 --
26481 2022:211:12:12:07.772 5 -125.8 -186.1 9011 8952 4 99.3% 100.0% 100.0% 99.3% 0.05 8.97 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.