AGASC ID 76813936

Info

Last Obs. 2024:325:04:10
magcatalog 7.16 ± 0.02
mag3 arcsec 7.16 ± 0.01
mag5 arcsec 7.16 ± 0.01
Nobs 14 (0 bad)
fok 100.0%
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
61023 2002:266:18:31:42.714 0 -88.9 -211.2 4824 4775 3 100.0% 100.0% 100.0% 100.0% 0.01 7.14 0.00 --
60668 2003:189:17:58:52.669 1 -219.4 -228.0 10613 10563 7 100.0% 100.0% 100.0% 100.0% 0.01 7.14 0.00 --
4095 2003:238:07:37:03.040 3 431.7 -85.6 1222 1165 1 100.0% 100.0% 100.0% 100.0% 0.01 7.14 0.00 --
5786 2005:290:09:07:38.328 3 259.6 -472.8 14779 14722 10 100.0% 100.0% 100.0% 100.0% 0.01 7.15 0.00 --
17490 2015:020:06:49:45.047 3 304.5 -445.7 59122 59063 13 100.0% 100.0% 100.0% 100.0% 0.02 7.15 0.00 --
17170 2015:309:19:43:45.952 3 247.8 -462.7 12707 12641 3 100.0% 100.0% 100.0% 100.0% 0.02 7.15 0.00 --
18702 2015:319:08:05:47.906 3 247.8 -462.7 12341 12249 6 100.0% 100.0% 100.0% 100.0% 0.02 7.16 0.00 --
18703 2016:014:17:24:11.650 3 273.3 -446.1 13175 13101 5 100.0% 100.0% 100.0% 100.0% 0.01 7.15 0.00 --
49455 2018:026:17:28:53.802 0 149.0 -273.3 1836 1780 0 100.0% 100.0% 100.0% 100.0% 0.01 7.13 0.00 --
27457 2022:275:18:39:54.831 3 -22.9 92.8 6243 6157 5 100.0% 100.0% 100.0% 100.0% 0.02 7.16 0.00 --
43148 2024:260:04:33:31.520 0 236.8 379.6 908 849 0 99.9% 100.0% 100.0% 99.9% 0.01 7.17 0.00 --
28673 2024:266:00:50:29.062 3 49.7 -78.9 3268 3203 1 100.0% 100.0% 100.0% 100.0% 0.02 7.19 0.00 --
30080 2024:266:21:08:18.573 3 58.5 -72.5 4243 4182 1 100.0% 100.0% 100.0% 100.0% 0.03 7.19 0.00 --
28303 2024:325:04:10:36.012 3 87.7 -32.5 10340 10288 2 100.0% 100.0% 100.0% 100.0% 0.03 7.19 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.