AGASC ID 239473688

Info

Last Obs. 2025:340:08:55
magcatalog 9.05 ± 0.02
mag3 arcsec 9.10 ± 0.02
mag5 arcsec 9.10 ± 0.02
Nobs 14 (0 bad)
fok 99.7%
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
57429 2008:358:04:52:32.628 4 -15.6 -455.8 997 945 2 99.8% 99.9% 100.0% 99.7% 0.03 9.08 0.00 --
57424 2008:360:20:09:24.290 1 8.5 -456.3 1929 1871 4 99.7% 99.8% 100.0% 99.5% 0.03 9.11 0.00 --
16204 2013:356:22:25:03.904 3 212.5 -349.4 19632 19505 22 99.6% 100.0% 100.0% 99.6% 0.04 9.11 0.00 --
16557 2013:359:14:23:35.409 3 212.5 -349.4 27033 26919 20 99.8% 100.0% 100.0% 99.8% 0.04 9.11 0.00 --
16558 2013:361:17:33:50.658 3 212.5 -349.4 41220 40984 42 99.6% 100.0% 100.0% 99.6% 0.06 9.11 0.00 --
16205 2013:364:07:45:09.097 3 212.5 -349.4 48243 48005 40 99.6% 100.0% 100.0% 99.6% 0.06 9.11 0.00 --
16559 2014:002:06:31:54.124 3 212.5 -349.4 42049 41919 37 99.8% 100.0% 100.0% 99.8% 0.05 9.10 0.00 --
16207 2014:086:22:45:37.431 4 313.2 -257.8 29416 29318 20 99.9% 100.0% 100.0% 99.9% 0.04 9.09 0.00 --
16604 2014:091:10:32:14.385 4 317.5 -252.3 32408 32186 25 99.5% 100.0% 100.0% 99.5% 0.03 9.09 0.00 --
16206 2014:094:19:23:27.078 4 317.5 -252.3 57473 57290 61 99.8% 100.0% 100.0% 99.8% 0.04 9.08 0.00 --
52873 2014:096:04:50:50.628 1 317.5 -252.3 95 48 1 100.0% 100.0% 100.0% 100.0% 0.01 9.08 0.00 --
31039 2025:339:11:33:06.981 6 295.6 25.0 3383 3323 1 99.9% 99.9% 100.0% 99.8% 0.07 9.06 0.00 --
32032 2025:339:23:06:19.452 7 290.7 -34.0 3754 3699 3 100.0% 100.0% 100.0% 99.9% 0.07 9.13 0.00 --
32033 2025:340:08:55:47.655 7 290.2 -33.8 2896 2846 1 99.9% 100.0% 100.0% 99.8% 0.05 9.14 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.