AGASC ID 235947248

Info

Last Obs. 2024:335:11:16
magcatalog 6.60 ± 0.02
mag3 arcsec 6.61 ± 0.03
mag5 arcsec 6.61 ± 0.03
Nobs 14 (0 bad)
fok 86.2%
f3 arcsec 86.2%
f5 arcsec 86.2%

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
17252 2015:092:08:33:59.374 5 -383.7 418.6 46479 46408 14 100.0% 100.0% 100.0% 100.0% 0.01 6.59 0.00 --
51972 2015:093:11:36:15.186 3 -383.7 418.6 83 46 0 100.0% 100.0% 100.0% 100.0% 0.01 6.59 0.00 --
50707 2016:257:09:35:53.151 3 412.1 -335.2 11089 10970 0 99.9% 3.1% 3.1% 3.1% 0.12 6.87 0.00 --
43959 2023:328:23:35:08.761 1 139.0 17.0 830 762 1 100.0% 100.0% 100.0% 100.0% 0.01 6.62 0.00 --
28898 2023:341:17:05:26.439 5 129.2 470.7 1649 1605 0 99.9% 100.0% 100.0% 99.9% 0.02 6.63 0.00 --
28899 2023:342:21:22:24.288 4 73.2 242.9 1725 1669 0 100.0% 100.0% 100.0% 100.0% 0.02 6.62 0.00 --
28900 2023:348:19:11:01.233 5 -258.7 212.1 1595 1559 0 100.0% 100.0% 100.0% 100.0% 0.01 6.63 0.00 --
28905 2023:349:20:56:49.736 4 -173.5 275.4 1617 1562 1 100.0% 100.0% 100.0% 100.0% 0.01 6.62 0.00 --
29144 2024:322:10:53:55.951 4 298.9 110.5 1846 1781 1 100.0% 99.9% 100.0% 99.9% 0.01 6.63 0.00 --
28901 2024:324:14:43:04.580 4 70.5 -252.0 1899 1833 0 100.0% 100.0% 100.0% 100.0% 0.02 6.64 0.00 --
42944 2024:328:22:02:06.520 2 299.0 -422.5 4181 3695 1 100.0% 100.0% 100.0% 100.0% 0.02 6.63 0.00 --
28904 2024:331:05:11:50.759 4 -209.8 -80.0 1691 1634 0 100.0% 100.0% 100.0% 100.0% 0.02 6.64 0.00 --
28902 2024:332:01:55:16.440 5 265.1 -223.0 1898 1848 1 100.0% 100.0% 100.0% 100.0% 0.02 6.65 0.00 --
29145 2024:335:11:16:31.608 5 -102.2 304.5 1734 1675 0 100.0% 100.0% 100.0% 100.0% 0.02 6.64 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.