AGASC ID 395460552

Info

Last Obs. 2023:361:21:07
magcatalog 8.99 ± 0.25
mag3 arcsec 8.98 ± 0.02
mag5 arcsec 8.98 ± 0.02
Nobs 13 (0 bad)
fok 99.8%
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
3480 2002:127:23:13:54.243 6 215.7 228.1 45436 45350 39 99.9% 100.0% 100.0% 99.9% 0.03 8.97 0.00 --
3052 2002:129:18:15:07.976 6 215.7 228.1 76450 76285 78 99.9% 100.0% 100.0% 99.8% 0.04 8.97 0.00 --
3089 2002:183:15:45:14.569 5 65.3 313.7 41647 41484 38 99.8% 100.0% 100.0% 99.8% 0.04 8.97 0.00 --
7829 2007:078:12:54:32.988 6 295.4 -21.2 24842 24754 50 99.9% 100.0% 100.0% 99.9% 0.02 9.00 0.00 --
7830 2007:202:10:15:49.261 4 -9.9 318.6 24534 24431 42 99.9% 100.0% 100.0% 99.8% 0.03 8.96 0.00 --
9219 2008:062:10:07:52.839 5 247.9 -150.2 24537 24438 45 99.8% 100.0% 100.0% 99.8% 0.03 8.98 0.00 --
9218 2008:087:03:02:25.406 6 295.7 45.3 33827 33702 53 99.9% 100.0% 100.0% 99.9% 0.02 8.97 0.00 --
9217 2008:089:02:39:08.002 6 295.7 45.3 61104 60973 109 99.9% 100.0% 100.0% 99.9% 0.02 8.97 0.00 --
16089 2014:043:19:32:08.988 5 167.3 -236.7 85763 85327 70 99.6% 100.0% 100.0% 99.6% 0.05 9.00 0.00 --
16090 2014:067:15:06:40.637 6 272.0 -108.5 34545 34429 36 99.9% 100.0% 100.0% 99.9% 0.04 9.01 0.00 --
25025 2021:123:10:10:09.091 5 222.5 210.9 24543 24176 25 98.8% 100.0% 100.0% 98.8% 0.08 8.98 0.00 --
29179 2023:360:11:53:04.081 6 -75.8 -287.0 4399 4328 0 99.9% 99.8% 100.0% 99.7% 0.13 8.97 0.00 --
29180 2023:361:21:07:55.730 6 -67.0 -288.7 10460 10391 1 100.0% 100.0% 100.0% 99.9% 0.14 8.98 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.