AGASC ID 647891312

Info

Last Obs. 2026:100:12:18
magcatalog 9.84 ± 0.02
mag3 arcsec 9.80 ± 0.05
mag5 arcsec 9.80 ± 0.05
Nobs 12 (0 bad)
fok 97.5%
f3 arcsec 96.9%
f5 arcsec 99.9%

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
13822 2012:025:18:03:47.248 4 -123.1 270.7 5038 4929 8 99.1% 100.0% 100.0% 99.0% 0.07 9.78 0.00 --
54910 2012:025:21:15:25.212 2 -122.9 270.6 44 44 0 100.0% 100.0% 100.0% 100.0% 0.03 9.78 0.00 --
13822 2012:025:21:15:25.212 2 -123.1 270.7 90 44 0 100.0% 100.0% 100.0% 100.0% 0.03 9.77 0.00 --
13665 2012:321:22:45:51.305 4 -130.4 267.3 4837 4666 7 98.1% 100.0% 100.0% 98.1% 0.03 9.75 0.00 --
13665 2012:321:22:45:51.305 4 -130.3 267.2 4757 4665 7 98.1% 100.0% 100.0% 98.1% 0.03 9.77 0.00 --
54161 2012:322:02:15:19.297 2 -130.4 267.3 85 44 0 97.8% 100.0% 100.0% 97.8% 0.01 9.75 0.00 --
46454 2021:088:23:45:40.060 3 -77.6 -313.6 2272 2032 44 91.5% 96.8% 99.5% 88.6% 0.09 9.81 0.00 --
45658 2022:068:18:27:12.439 6 -157.3 -353.9 323 251 0 94.7% 97.6% 100.0% 92.5% 0.04 9.82 0.00 --
45657 2022:068:22:34:44.656 6 -157.6 -353.8 322 270 0 98.9% 98.5% 100.0% 97.4% 0.07 9.81 0.00 --
45648 2022:070:23:30:28.928 7 -161.5 -352.0 325 249 1 96.9% 96.4% 100.0% 93.4% 0.06 9.85 0.00 --
45647 2022:071:05:22:35.545 6 -162.3 -351.6 324 268 7 97.5% 94.4% 99.3% 92.0% 0.10 9.84 0.00 --
45646 2022:071:15:50:44.321 7 -163.4 -351.1 324 240 2 91.6% 88.3% 100.0% 80.9% 0.05 9.84 0.00 --
41565 2026:100:09:21:52.141 7 358.0 216.0 826 768 0 100.0% 97.9% 100.0% 97.9% 0.15 9.92 0.00 --
41563 2026:100:12:18:59.292 7 358.3 215.5 2492 2416 7 99.2% 85.2% 99.9% 84.5% 0.16 9.88 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.