AGASC ID 395842632

Info

Last Obs. 2023:065:21:49
magcatalog 9.35 ± 0.15
mag3 arcsec 9.12 ± 0.03
mag5 arcsec 9.12 ± 0.03
Nobs 13 (0 bad)
fok 98.3%
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
4726 2004:325:06:14:54.767 4 -82.9 270.5 19584 19566 25 99.9% 100.0% 100.0% 99.9% 0.03 9.11 0.00 --
20999 2018:310:02:27:30.568 5 -66.8 296.6 7525 7448 8 99.0% 100.0% 100.0% 98.9% 0.05 9.09 0.00 --
23482 2020:332:02:52:16.532 4 -86.9 258.4 14220 14191 19 99.8% 100.0% 100.0% 99.8% 0.05 9.09 0.00 --
23483 2020:362:12:18:28.118 4 -164.5 205.2 14709 14392 23 97.8% 100.0% 100.0% 97.8% 0.06 9.10 0.00 --
23484 2021:024:18:09:27.763 4 -225.4 117.4 14791 14389 12 97.3% 100.0% 100.0% 97.3% 0.08 9.09 0.00 --
23485 2021:052:00:29:31.386 4 -243.9 -31.6 15969 15773 17 98.8% 100.0% 100.0% 98.7% 0.04 9.12 0.00 --
23486 2021:078:12:17:55.103 4 -155.0 -190.5 14703 14403 16 98.0% 100.0% 100.0% 97.9% 0.08 9.14 0.00 --
23487 2021:108:07:13:57.622 4 17.2 -255.8 14704 14504 13 98.6% 99.7% 100.0% 98.4% 0.15 9.15 0.00 --
23488 2021:135:01:43:17.644 4 92.5 -244.7 14724 14380 22 97.7% 100.0% 100.0% 97.7% 0.06 9.15 0.00 --
23489 2021:163:12:53:48.283 4 169.6 -209.1 14702 14322 17 97.4% 100.0% 100.0% 97.4% 0.05 9.13 0.00 --
23490 2021:189:12:16:04.227 4 200.1 -185.9 14708 14343 24 97.5% 100.0% 100.0% 97.5% 0.06 9.10 0.00 --
23491 2021:218:15:10:43.110 4 273.5 -73.7 14708 14424 12 98.1% 100.0% 100.0% 98.0% 0.11 9.16 0.00 --
25118 2023:065:21:49:24.251 6 -465.9 -411.5 7868 7712 55 98.0% 99.9% 100.0% 97.9% 0.15 9.20 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.