AGASC ID 897722208

Info

Last Obs. 2022:240:21:55
magcatalog 8.81 ± 0.10
mag3 arcsec 8.38 ± 0.02
mag5 arcsec 8.38 ± 0.02
Nobs 13 (0 bad)
fok 99.3%
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 mag ⟩ 100s ⟨ mag ⟩ σmag Comments
8715 2008:135:01:29:43.074 7 -475.1 47.8 1067 1066 1 99.9% 100.0% 100.0% 99.9% 0.01 8.38 0.00 --
8739 2008:135:06:22:33.074 6 -256.1 438.7 1065 1062 2 99.7% 99.9% 99.9% 99.6% 0.01 8.35 0.00 --
8738 2008:135:07:04:23.074 5 -416.3 381.0 1064 1064 1 100.0% 100.0% 100.0% 100.0% 0.01 8.36 0.00 --
13536 2011:304:17:06:29.830 4 426.7 -477.4 1154 1153 1 99.9% 99.9% 100.0% 99.8% 0.01 8.37 0.00 --
13589 2011:304:18:42:24.342 7 -152.8 -440.6 1152 1152 0 100.0% 100.0% 100.0% 100.0% 0.01 8.36 0.00 --
18996 2017:043:17:40:15.313 6 -349.0 -147.0 3489 3475 2 99.6% 100.0% 100.0% 99.6% 0.02 8.37 0.00 --
24199 2022:076:14:13:35.066 6 -193.0 -445.6 2209 2163 1 97.9% 100.0% 100.0% 97.9% 0.03 8.36 0.00 --
24078 2022:095:01:14:47.088 7 293.6 -371.0 2196 2185 3 99.5% 100.0% 100.0% 99.5% 0.03 8.40 0.00 --
24137 2022:103:22:13:37.425 7 -318.7 -262.0 2206 2184 4 99.0% 100.0% 100.0% 99.0% 0.03 8.40 0.00 --
23911 2022:114:16:10:39.890 6 133.4 269.5 2632 2617 3 99.4% 100.0% 100.0% 99.4% 0.03 8.38 0.00 --
45533 2022:115:13:46:09.729 4 206.1 261.1 2910 2888 0 99.2% 100.0% 100.0% 99.2% 0.05 8.38 0.00 --
24073 2022:181:12:51:36.965 6 -169.5 117.7 2193 2163 1 98.7% 100.0% 100.0% 98.6% 0.02 8.40 0.00 --
23919 2022:240:21:55:18.436 6 429.5 -420.9 2877 2848 2 99.0% 100.0% 100.0% 99.0% 0.03 8.38 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.