AGASC ID 649730488

Info

Last Obs. 2024:104:16:40
magcatalog 7.79 ± 0.05
mag3 arcsec 7.81 ± 0.01
mag5 arcsec 7.81 ± 0.01
Nobs 13 (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
5651 2005:153:23:28:28.433 4 190.5 -446.1 1607 1555 2 99.9% 100.0% 100.0% 99.9% 0.01 7.81 0.00 --
5823 2005:332:10:32:49.641 7 -473.3 -34.7 19657 19576 23 100.0% 100.0% 100.0% 100.0% 0.01 7.82 0.00 --
5822 2005:333:10:23:43.849 7 -473.2 -35.5 9910 9773 11 99.4% 100.0% 100.0% 99.4% 0.01 7.82 0.00 --
7242 2006:060:15:39:03.055 7 -458.1 -114.9 18431 18373 19 100.0% 100.0% 100.0% 100.0% 0.01 7.82 0.00 --
7691 2007:055:18:58:01.149 7 -467.8 -89.0 2975 2929 4 99.9% 100.0% 100.0% 99.9% 0.01 7.81 0.00 --
10424 2009:059:01:21:32.091 6 -407.7 -254.1 2577 2533 2 100.0% 100.0% 100.0% 100.0% 0.01 7.80 0.00 --
10425 2009:059:03:11:52.912 7 -347.9 -57.9 2581 2526 7 99.9% 100.0% 100.0% 99.9% 0.01 7.79 0.00 --
52944 2014:067:04:11:56.093 4 -223.5 -65.5 1311 1266 1 100.0% 100.0% 100.0% 100.0% 0.02 7.79 0.00 --
48308 2019:084:12:24:02.171 6 -58.0 -455.9 3152 2669 7 99.9% 100.0% 100.0% 99.9% 0.02 7.79 0.00 --
46445 2021:093:20:34:46.230 5 417.5 234.3 834 765 2 99.6% 99.9% 100.0% 99.5% 0.02 7.79 0.00 --
46440 2021:094:06:13:59.956 6 412.0 -257.8 2546 2478 3 99.8% 100.0% 100.0% 99.8% 0.02 7.80 0.00 --
45043 2022:329:04:22:00.893 0 149.7 148.4 825 768 1 100.0% 100.0% 100.0% 100.0% 0.02 7.80 0.00 --
29363 2024:104:16:40:10.574 3 -41.0 68.1 3506 3456 4 99.9% 100.0% 100.0% 99.9% 0.03 7.83 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.