AGASC ID 897076488

Info

Last Obs. 2024:165:14:09
magcatalog 9.60 ± 0.05
mag3 arcsec 9.40 ± 0.02
mag5 arcsec 9.40 ± 0.02
Nobs 13 (0 bad)
fok 98.9%
f3 arcsec 99.9%
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
2684 2002:185:17:50:43.150 6 453.7 -32.8 6362 6297 5 99.9% 100.0% 100.0% 99.9% 0.03 9.42 0.00 --
2685 2002:216:23:38:28.654 6 436.8 -115.2 6885 6824 6 99.9% 100.0% 100.0% 99.9% 0.05 9.42 0.00 --
2683 2002:252:16:50:47.900 5 433.1 -126.7 7393 7328 6 99.9% 100.0% 100.0% 99.9% 0.02 9.41 0.00 --
2797 2002:312:05:33:21.893 5 416.2 -140.2 24276 23920 18 98.8% 100.0% 100.0% 98.8% 0.07 9.39 0.00 --
59639 2005:151:15:43:53.489 0 -146.5 411.5 2979 2864 5 97.4% 99.9% 100.0% 97.3% 0.03 9.39 0.00 --
6769 2006:147:12:16:01.898 3 -428.1 184.6 20139 19949 32 99.4% 100.0% 100.0% 99.4% 0.04 9.40 0.00 --
9132 2008:220:20:29:40.358 3 436.6 -122.4 70400 70127 135 99.7% 100.0% 100.0% 99.7% 0.06 9.41 0.00 --
9133 2008:223:23:35:33.297 3 436.2 -123.6 26978 26702 36 99.2% 100.0% 100.0% 99.2% 0.04 9.40 0.00 --
14616 2013:118:19:18:45.236 3 -435.1 170.8 7490 7215 5 97.2% 100.0% 100.0% 97.2% 0.04 9.41 0.00 --
15645 2013:119:00:10:08.417 3 -432.1 172.2 26192 25415 22 97.2% 100.0% 100.0% 97.2% 0.08 9.39 0.00 --
16749 2015:219:20:06:13.224 3 424.5 -122.4 15061 14770 16 98.4% 100.0% 100.0% 98.4% 0.05 9.40 0.00 --
16750 2015:311:15:48:23.747 3 416.5 -145.8 14783 14288 20 97.3% 100.0% 100.0% 97.2% 0.05 9.40 0.00 --
29445 2024:165:14:09:37.747 6 -323.3 242.5 5211 5145 1 99.7% 98.1% 100.0% 97.8% 0.17 9.38 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.