AGASC ID 132401928

Info

Last Obs. 2025:214:14:47
magcatalog 7.30 ± 0.02
mag3 arcsec 7.31 ± 0.01
mag5 arcsec 7.31 ± 0.01
Nobs 13 (0 bad)
fok 99.9%
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
52997 2014:046:04:50:50.832 4 -423.1 -109.7 931 888 0 100.0% 100.0% 100.0% 100.0% 0.01 7.32 0.00 --
49917 2017:198:03:23:06.825 3 156.2 -357.8 1868 1812 3 100.0% 100.0% 100.0% 100.0% 0.02 7.30 0.00 --
20207 2018:317:18:05:54.301 6 49.8 444.2 14783 14694 13 100.0% 100.0% 100.0% 99.9% 0.02 7.31 0.00 --
20186 2018:323:02:29:30.485 7 13.7 447.9 4542 4460 2 100.0% 100.0% 100.0% 100.0% 0.01 7.31 0.00 --
20208 2019:035:14:13:54.586 7 -417.8 -141.3 9895 9812 7 100.0% 100.0% 100.0% 99.9% 0.02 7.31 0.00 --
22080 2019:036:02:36:21.161 7 -417.7 -141.4 9899 9778 6 99.4% 100.0% 100.0% 99.4% 0.02 7.31 0.00 --
21200 2019:120:02:43:29.126 7 -204.0 -377.3 2091 2031 1 100.0% 100.0% 100.0% 100.0% 0.01 7.30 0.00 --
21201 2019:126:07:35:30.934 6 -102.5 -413.0 4532 4453 2 100.0% 100.0% 100.0% 100.0% 0.02 7.30 0.00 --
21202 2019:135:15:49:38.321 6 63.7 -416.6 2584 2490 0 100.0% 100.0% 100.0% 100.0% 0.01 7.31 0.00 --
21203 2019:144:09:56:10.080 6 12.3 -422.4 5999 5927 4 100.0% 100.0% 100.0% 100.0% 0.02 7.32 0.00 --
21204 2019:153:15:53:06.269 7 90.1 -410.3 14780 14723 7 100.0% 100.0% 100.0% 100.0% 0.01 7.31 0.00 --
21205 2019:162:01:45:00.459 7 176.5 -381.6 34292 34195 23 100.0% 100.0% 100.0% 100.0% 0.01 7.31 0.00 --
29798 2025:214:14:47:41.191 4 401.5 149.4 5915 5845 0 100.0% 100.0% 100.0% 100.0% 0.03 7.34 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.