AGASC ID 897716896

Info

Last Obs. 2022:166:07:26
magcatalog 7.33 ± 0.11
mag3 arcsec 7.30 ± 0.01
mag5 arcsec 7.30 ± 0.01
Nobs 16 (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
8730 2008:133:21:54:56.474 5 -273.7 -398.7 1184 1183 3 99.9% 100.0% 100.0% 99.9% 0.02 7.31 0.00 --
8729 2008:133:23:00:03.074 3 -434.0 -459.0 1065 1064 0 100.0% 100.0% 100.0% 100.0% 0.01 7.32 0.00 --
8741 2008:135:04:58:53.074 5 -243.4 -232.2 1067 1067 1 100.0% 100.0% 100.0% 100.0% 0.01 7.30 0.00 --
8740 2008:135:05:40:43.074 4 -403.0 -291.0 1067 1066 1 99.9% 100.0% 100.0% 99.9% 0.01 7.31 0.00 --
9960 2009:046:23:26:23.870 4 145.9 347.4 8758 8753 5 99.9% 100.0% 100.0% 99.9% 0.01 7.30 0.00 --
57300 2009:047:04:43:54.219 1 145.9 347.4 22 22 0 100.0% 100.0% 100.0% 100.0% 0.00 7.30 0.00 --
13589 2011:304:18:42:24.342 6 56.6 376.7 1152 1152 2 100.0% 100.0% 100.0% 100.0% 0.01 7.31 0.00 --
13538 2011:306:18:25:38.144 3 339.3 191.2 1157 1157 1 100.0% 100.0% 100.0% 100.0% 0.01 7.30 0.00 --
13559 2011:307:03:31:22.826 7 480.0 97.3 1160 1160 0 100.0% 100.0% 100.0% 100.0% 0.01 7.30 0.00 --
13560 2011:307:04:16:12.826 4 327.3 23.8 1155 1154 1 99.9% 100.0% 100.0% 99.9% 0.01 7.31 0.00 --
52760 2014:141:06:45:18.615 1 62.7 61.5 2483 2483 4 100.0% 100.0% 100.0% 100.0% 0.01 7.30 0.00 --
23914 2021:192:02:49:14.563 4 285.3 311.4 2648 2647 1 100.0% 100.0% 100.0% 100.0% 0.02 7.29 0.00 --
23915 2021:192:04:57:34.834 3 219.8 483.0 2671 2671 0 100.0% 100.0% 100.0% 100.0% 0.01 7.30 0.00 --
23918 2021:192:09:47:04.834 3 435.3 435.8 2667 2667 2 100.0% 100.0% 100.0% 100.0% 0.01 7.30 0.00 --
23912 2022:111:20:39:11.205 4 -237.0 -373.6 2655 2653 1 99.9% 100.0% 100.0% 99.9% 0.02 7.31 0.00 --
24053 2022:166:07:26:02.053 3 -291.3 -48.4 2670 2669 1 100.0% 100.0% 100.0% 100.0% 0.01 7.32 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.