AGASC ID 504890688

Info

Last Obs. 2023:223:18:00
magcatalog 9.17 ± 0.05
mag3 arcsec 9.19 ± 0.02
mag5 arcsec 9.19 ± 0.02
Nobs 14 (0 bad)
fok 95.9%
f3 arcsec 96.1%
f5 arcsec 96.1%

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
4731 2004:019:05:44:08.991 3 315.2 -427.4 27952 27871 32 99.9% 100.0% 100.0% 99.9% 0.03 9.20 0.00 --
5296 2004:021:10:28:25.980 3 315.2 -427.4 46241 44748 36 99.9% 70.4% 70.4% 70.3% 0.03 9.20 0.00 --
5297 2004:024:01:24:22.823 3 315.2 -427.4 11071 11008 8 100.0% 100.0% 100.0% 100.0% 0.02 9.20 0.00 --
4733 2004:128:13:22:55.371 4 304.9 466.9 12345 12251 13 99.9% 100.0% 100.0% 99.9% 0.02 9.20 0.00 --
4736 2004:306:18:24:57.930 4 -297.4 -408.5 38284 38175 54 99.9% 100.0% 100.0% 99.9% 0.03 9.19 0.00 --
6152 2004:312:06:34:56.807 4 -297.4 -408.5 80025 79619 95 99.9% 100.0% 100.0% 99.8% 0.04 9.19 0.00 --
6170 2004:357:01:02:55.365 3 105.7 -465.7 23757 23674 24 99.9% 100.0% 100.0% 99.9% 0.03 9.21 0.00 --
6175 2004:359:16:23:25.528 3 105.7 -465.7 20141 20076 28 99.9% 100.0% 100.0% 99.9% 0.03 9.21 0.00 --
6169 2004:365:01:46:45.504 3 155.2 -451.2 14782 14710 21 99.9% 100.0% 100.0% 99.9% 0.03 9.21 0.00 --
4737 2005:001:14:16:30.167 3 173.5 -444.4 10877 10807 12 99.9% 100.0% 100.0% 99.9% 0.03 9.21 0.00 --
9546 2007:337:05:39:12.785 4 -234.7 9.9 14777 14711 23 99.9% 100.0% 100.0% 99.9% 0.02 9.17 0.00 --
14341 2011:239:10:16:20.812 3 -454.1 250.5 24366 24263 37 99.9% 100.0% 100.0% 99.9% 0.03 9.17 0.00 --
19304 2017:312:20:33:29.228 4 -323.8 -363.7 18421 17997 18 98.0% 100.0% 100.0% 98.0% 0.09 9.15 0.00 --
27863 2023:223:18:00:04.466 7 -395.2 297.8 2793 2740 0 100.0% 99.9% 100.0% 99.9% 0.08 9.19 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.