AGASC ID 763500112

Info

Last Obs. 2025:130:00:15
magcatalog 6.15 ± 0.03
mag3 arcsec 6.12 ± 0.03
mag5 arcsec 6.12 ± 0.03
Nobs 12 (0 bad)
fok 100.0%
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
6934 2006:121:20:29:52.612 6 296.8 -387.6 26147 26086 4 100.0% 100.0% 100.0% 100.0% 0.02 6.13 0.00 --
7329 2006:124:08:27:07.353 6 296.8 -387.6 29788 29712 5 100.0% 100.0% 100.0% 100.0% 0.02 6.10 0.00 --
15141 2013:218:18:23:28.399 6 301.7 -350.8 2589 2530 0 100.0% 100.0% 100.0% 100.0% 0.01 6.13 0.00 --
15143 2013:277:15:13:08.897 6 -213.0 262.9 2581 2528 0 100.0% 100.0% 100.0% 100.0% 0.02 6.14 0.00 --
19598 2017:227:01:37:02.395 6 173.6 -452.7 7214 7130 1 100.0% 100.0% 100.0% 100.0% 0.02 6.16 0.00 --
49849 2017:227:06:07:41.054 4 170.7 -447.6 184 55 0 100.0% 100.0% 100.0% 100.0% 0.01 6.16 0.00 --
20626 2017:227:20:27:57.145 6 172.5 -452.2 12801 12635 1 100.0% 100.0% 100.0% 100.0% 0.02 6.16 0.00 --
20627 2017:229:14:51:20.902 6 173.7 -452.8 10432 10343 1 100.0% 100.0% 100.0% 100.0% 0.02 6.16 0.00 --
49844 2017:229:21:23:10.826 4 170.7 -447.6 186 51 0 100.0% 100.0% 100.0% 100.0% 0.01 6.16 0.00 --
20628 2017:231:06:16:23.445 6 173.4 -452.7 5518 5428 2 100.0% 100.0% 100.0% 100.0% 0.01 6.16 0.00 --
19596 2017:281:23:27:18.020 5 -359.2 366.8 34381 34311 4 100.0% 100.0% 100.0% 100.0% 0.02 6.09 0.00 --
28819 2025:130:00:15:33.966 3 249.5 -425.9 1388 1336 0 100.0% 100.0% 100.0% 100.0% 0.02 6.14 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.