AGASC ID 645137032

Info

Last Obs. 2024:076:01:56
magcatalog 7.99 ± 0.04
mag3 arcsec 8.01 ± 0.02
mag5 arcsec 8.01 ± 0.02
Nobs 12 (0 bad)
fok 99.4%
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
58442 2007:098:13:02:41.372 0 417.9 416.3 3449 3387 3 99.9% 100.0% 100.0% 99.9% 0.01 8.00 0.00 --
58430 2007:109:02:22:53.981 3 -148.5 -30.0 1652 1606 2 99.9% 100.0% 100.0% 99.9% 0.02 8.00 0.00 --
22573 2020:133:17:12:36.708 3 330.7 147.9 6002 5892 5 99.2% 100.0% 100.0% 99.2% 0.02 8.00 0.00 --
26865 2023:069:02:01:15.515 5 -212.0 -417.7 944 891 0 99.1% 100.0% 100.0% 99.1% 0.02 8.00 0.00 --
44753 2023:069:21:20:01.007 2 -311.0 -317.7 1328 1254 0 99.0% 100.0% 100.0% 99.0% 0.03 8.01 0.00 --
44744 2023:072:15:35:29.706 2 326.3 -303.4 581 506 1 97.9% 100.0% 100.0% 97.9% 0.02 8.00 0.00 --
44740 2023:072:19:24:56.000 2 314.6 -315.0 399 319 5 97.9% 100.0% 100.0% 97.9% 0.02 8.01 0.00 --
44738 2023:072:22:10:40.334 2 305.3 -323.8 326 253 0 99.2% 100.0% 100.0% 99.2% 0.01 8.02 0.00 --
44735 2023:075:05:09:28.024 2 150.7 -415.2 1009 1000 0 99.1% 100.0% 100.0% 99.1% 0.03 8.02 0.00 --
27724 2023:075:05:09:28.024 2 150.9 -415.4 1076 1000 0 99.1% 100.0% 100.0% 99.1% 0.02 8.00 0.00 --
44730 2023:075:10:53:36.000 2 137.3 -419.8 513 513 1 100.0% 100.0% 100.0% 100.0% 0.02 8.02 0.00 --
27724 2023:075:10:53:36.000 2 137.4 -419.8 591 513 1 100.0% 100.0% 100.0% 100.0% 0.02 8.00 0.00 --
44728 2023:075:13:01:35.532 2 132.6 -421.2 275 274 0 99.6% 100.0% 100.0% 99.6% 0.02 8.01 0.00 --
27724 2023:075:13:01:35.532 2 132.7 -421.2 339 274 0 99.6% 100.0% 100.0% 99.6% 0.02 8.00 0.00 --
29320 2024:076:01:56:58.522 5 -486.7 -32.4 2850 2706 2 99.9% 100.0% 100.0% 99.9% 0.02 8.06 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.