AGASC ID 649599704

Info

Last Obs. 2024:081:20:29
magcatalog 8.63 ± 0.10
mag3 arcsec 8.67 ± 0.01
mag5 arcsec 8.67 ± 0.01
Nobs 10 (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
2971 2002:080:04:22:51.556 3 325.4 -185.7 53065 52968 45 100.0% 100.0% 100.0% 100.0% 0.02 8.67 0.00 --
3559 2003:153:20:41:40.979 5 -343.7 221.8 2601 2503 4 99.9% 100.0% 100.0% 99.8% 0.02 8.66 0.00 --
6867 2006:017:08:41:23.305 5 326.0 -188.2 14863 14792 20 99.9% 100.0% 100.0% 99.9% 0.02 8.67 0.00 --
7360 2007:056:22:58:01.157 5 328.7 -190.1 1124 1067 2 99.9% 100.0% 100.0% 99.9% 0.01 8.67 0.00 --
7361 2007:192:16:50:51.526 5 -344.3 217.8 1116 1066 0 100.0% 100.0% 100.0% 100.0% 0.02 8.65 0.00 --
52951 2014:062:06:42:11.346 0 -58.4 263.4 1356 1287 0 99.6% 100.0% 100.0% 99.6% 0.02 8.63 0.00 --
45611 2022:088:12:21:19.944 4 -4.1 106.5 1844 1821 2 98.8% 99.9% 100.0% 98.6% 0.05 8.68 0.00 --
24252 2022:088:12:21:19.944 4 -4.2 106.5 1902 1822 2 98.8% 99.9% 100.0% 98.6% 0.05 8.68 0.00 --
45604 2022:091:03:04:56.003 4 -1.5 106.7 283 276 0 97.5% 100.0% 100.0% 97.5% 0.04 8.68 0.00 --
65525 2022:091:03:04:56.003 4 -1.6 106.7 339 276 0 97.5% 100.0% 100.0% 97.5% 0.04 8.68 0.00 --
45599 2022:091:09:00:51.392 4 -1.7 106.7 279 275 0 98.6% 100.0% 100.0% 98.6% 0.05 8.68 0.00 --
65525 2022:091:09:00:51.392 4 -1.8 106.7 337 276 0 98.6% 100.0% 100.0% 98.6% 0.05 8.68 0.00 --
29333 2024:081:20:29:30.028 4 374.4 -187.7 2460 2398 0 100.0% 100.0% 100.0% 100.0% 0.06 8.68 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.