AGASC ID 1092491384

Info

Last Obs. 2024:240:06:08
magcatalog 9.17 ± 0.02
mag3 arcsec 9.11 ± 0.02
mag5 arcsec 9.11 ± 0.02
Nobs 11 (0 bad)
fok 99.7%
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
4420 2003:076:19:37:06.511 6 289.4 376.0 37330 37165 25 99.7% 100.0% 100.0% 99.7% 0.04 9.11 0.00 --
4445 2003:272:11:30:45.775 7 -371.1 -276.0 14226 14163 18 99.9% 100.0% 100.0% 99.9% 0.03 9.10 0.00 --
4446 2004:035:16:12:08.866 6 213.5 432.0 14784 14683 19 99.9% 100.0% 100.0% 99.9% 0.03 9.11 0.00 --
4569 2004:235:12:59:01.156 7 -282.8 -367.1 24617 24559 19 99.9% 100.0% 100.0% 99.9% 0.02 9.10 0.00 --
4570 2004:278:04:59:59.936 7 -391.9 -259.6 24527 24435 30 99.8% 100.0% 100.0% 99.8% 0.02 9.10 0.00 --
4571 2004:302:08:26:28.782 7 -447.9 -158.3 25019 24944 14 99.9% 100.0% 100.0% 99.9% 0.05 9.09 0.00 --
5475 2005:134:02:18:14.229 6 455.8 50.9 73407 73013 51 99.9% 99.9% 100.0% 99.8% 0.06 9.12 0.00 --
6290 2005:166:20:24:02.736 6 250.6 -372.2 10755 10688 15 99.9% 100.0% 100.0% 99.9% 0.02 9.13 0.00 --
58376 2007:149:06:23:33.980 5 -374.9 -250.1 5158 5099 19 99.6% 99.9% 100.0% 99.5% 0.03 9.10 0.00 --
12410 2011:135:16:10:12.626 6 460.3 37.6 14844 14448 22 97.7% 100.0% 100.0% 97.7% 0.02 9.11 0.00 --
28205 2024:240:06:08:27.293 6 251.5 -182.9 2046 1993 2 99.9% 100.0% 100.0% 99.9% 0.08 9.18 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.