AGASC ID 890504456

Info

Last Obs. 2022:211:12:12
magcatalog 8.13 ± 0.04
mag3 arcsec 8.17 ± 0.01
mag5 arcsec 8.17 ± 0.01
Nobs 13 (0 bad)
fok 99.4%
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
16336 2014:021:01:30:01.927 4 -299.8 -160.9 1542 1541 1 99.9% 100.0% 100.0% 99.9% 0.02 8.15 0.00 --
19711 2017:174:23:21:39.815 4 216.2 429.3 12783 12749 11 99.7% 100.0% 100.0% 99.7% 0.02 8.14 0.00 --
48495 2019:018:10:41:00.043 5 75.3 -342.0 3494 3061 3 99.3% 100.0% 100.0% 99.3% 0.03 8.16 0.00 --
24759 2022:080:08:16:54.738 4 -461.4 417.8 9083 9048 9 99.6% 100.0% 100.0% 99.6% 0.03 8.18 0.00 --
24760 2022:081:22:36:14.628 4 -461.4 417.8 14231 14157 7 99.5% 100.0% 100.0% 99.5% 0.03 8.17 0.00 --
26367 2022:085:03:00:09.583 4 -462.6 418.5 4950 4920 5 99.4% 100.0% 100.0% 99.4% 0.02 8.17 0.00 --
24763 2022:123:12:33:01.128 4 -447.0 433.4 6437 6378 4 99.1% 100.0% 100.0% 99.1% 0.03 8.18 0.00 --
26406 2022:123:21:52:38.242 4 -447.2 433.6 8361 8226 4 98.4% 100.0% 100.0% 98.4% 0.03 8.18 0.00 --
24672 2022:128:18:57:01.774 4 -462.4 418.3 12252 12211 16 99.7% 100.0% 100.0% 99.7% 0.03 8.18 0.00 --
26416 2022:132:02:27:32.380 4 -464.1 419.1 12160 12096 22 99.5% 100.0% 100.0% 99.5% 0.03 8.18 0.00 --
24761 2022:141:20:09:28.767 4 -463.7 418.9 13487 13408 9 99.4% 100.0% 100.0% 99.4% 0.03 8.17 0.00 --
24762 2022:205:22:48:11.296 4 458.8 -378.2 5718 5651 3 98.8% 100.0% 100.0% 98.8% 0.03 8.16 0.00 --
26481 2022:211:12:12:07.772 4 458.6 -378.0 9011 8948 6 99.3% 100.0% 100.0% 99.3% 0.03 8.16 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.