AGASC ID 374350312

Info

Last Obs. 2024:352:23:48
magcatalog 8.43 ± 0.02
mag3 arcsec 8.45 ± 0.01
mag5 arcsec 8.45 ± 0.01
Nobs 14 (0 bad)
fok 99.9%
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
3237 2003:074:03:11:36.881 4 414.2 383.7 46485 46419 36 100.0% 100.0% 100.0% 100.0% 0.02 8.45 0.00 --
56648 2009:330:04:36:34.714 0 -442.4 92.3 399 353 1 100.0% 100.0% 100.0% 100.0% 0.03 8.44 0.00 --
13992 2011:309:19:02:46.726 3 180.2 -266.7 18435 18378 23 100.0% 100.0% 100.0% 99.9% 0.02 8.46 0.00 --
55075 2011:311:13:31:53.057 0 214.1 -247.8 349 306 1 100.0% 100.0% 100.0% 100.0% 0.01 8.45 0.00 --
54157 2012:322:07:26:36.494 0 -400.5 469.5 757 703 2 98.7% 100.0% 100.0% 98.7% 0.02 8.44 0.00 --
54142 2012:330:05:58:02.030 1 168.4 409.2 2043 1984 7 99.6% 99.9% 100.0% 99.5% 0.05 8.44 0.00 --
17278 2015:344:03:15:48.893 7 479.6 -105.9 2584 2531 2 100.0% 100.0% 100.0% 100.0% 0.02 8.47 0.00 --
17273 2015:345:18:34:56.239 6 -109.9 -468.7 2583 2516 5 99.9% 100.0% 100.0% 99.9% 0.02 8.45 0.00 --
49646 2017:319:20:00:44.923 0 -47.3 277.1 3744 3690 11 99.7% 100.0% 100.0% 99.7% 0.03 8.44 0.00 --
49644 2017:320:03:11:17.118 0 -50.4 269.2 4049 3960 4 98.9% 100.0% 100.0% 98.9% 0.03 8.43 0.00 --
20521 2018:273:02:01:05.620 4 278.1 -315.6 4051 3972 1 99.9% 100.0% 100.0% 99.9% 0.03 8.43 0.00 --
20520 2018:279:12:30:55.174 3 -97.6 310.1 4096 4023 5 99.6% 100.0% 100.0% 99.6% 0.03 8.41 0.00 --
42859 2024:352:22:32:25.938 3 -188.3 -34.5 314 273 0 99.6% 100.0% 100.0% 99.6% 0.03 8.50 0.00 --
42857 2024:352:23:48:07.000 3 -188.3 -34.7 318 276 1 100.0% 100.0% 100.0% 100.0% 0.02 8.50 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.