AGASC ID 266995040

Info

Last Obs. 2022:247:21:06
magcatalog 7.82 ± 0.07
mag3 arcsec 7.83 ± 0.01
mag5 arcsec 7.83 ± 0.01
Nobs 13 (0 bad)
fok 99.5%
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
5005 2005:103:04:24:53.020 3 -98.1 378.1 22036 22018 23 99.9% 100.0% 100.0% 99.9% 0.02 7.82 0.00 --
7692 2007:127:12:39:13.353 3 -284.6 294.1 2569 2568 4 100.0% 100.0% 100.0% 100.0% 0.01 7.81 0.00 --
15186 2014:019:23:29:11.331 3 301.7 257.2 44792 44784 21 100.0% 100.0% 100.0% 100.0% 0.02 7.82 0.00 --
16564 2014:022:16:16:14.376 3 301.7 257.2 22375 22370 11 100.0% 100.0% 100.0% 100.0% 0.02 7.82 0.00 --
16565 2014:024:06:02:42.179 3 301.7 257.2 10319 10316 9 100.0% 100.0% 100.0% 100.0% 0.01 7.82 0.00 --
24749 2020:363:02:04:23.677 4 91.6 -286.2 13229 13127 8 99.2% 100.0% 100.0% 99.2% 0.03 7.83 0.00 --
24489 2021:280:07:13:18.037 3 67.6 -403.7 13722 13681 11 99.7% 100.0% 100.0% 99.7% 0.02 7.83 0.00 --
24490 2022:089:21:28:04.485 3 -100.2 425.9 14510 14396 15 99.2% 100.0% 100.0% 99.2% 0.04 7.84 0.00 --
23844 2022:175:08:57:25.521 3 -419.1 -91.8 14491 14466 12 99.8% 100.0% 100.0% 99.8% 0.02 7.85 0.00 --
24488 2022:216:11:47:09.017 3 -269.9 -319.5 13749 13566 7 98.7% 100.0% 100.0% 98.7% 0.04 7.83 0.00 --
24491 2022:219:22:59:48.077 3 -269.9 -319.5 13728 13436 3 97.9% 100.0% 100.0% 97.9% 0.04 7.83 0.00 --
24490 2022:246:03:52:29.269 3 -99.7 -401.7 5840 5767 4 98.8% 100.0% 100.0% 98.8% 0.02 7.82 0.00 --
27331 2022:247:21:06:08.987 3 -141.1 -389.8 5088 5042 2 99.1% 100.0% 100.0% 99.1% 0.02 7.83 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.