AGASC ID 1040062216

Info

Last Obs. 2023:271:15:25
magcatalog 7.88 ± 0.03
mag3 arcsec 7.88 ± 0.01
mag5 arcsec 7.88 ± 0.01
Nobs 15 (0 bad)
fok 99.8%
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
21866 2018:323:01:01:18.221 6 463.2 157.9 1619 1527 3 99.9% 100.0% 100.0% 99.9% 0.01 7.86 0.00 --
25768 2023:075:19:01:40.183 5 -390.1 -304.1 3629 3621 5 99.8% 100.0% 100.0% 99.8% 0.02 7.87 0.00 --
27724 2023:075:19:01:40.183 5 -390.2 -304.1 3664 3621 5 99.8% 100.0% 100.0% 99.8% 0.02 7.87 0.00 --
27743 2023:076:04:30:47.000 5 -410.2 -279.3 4230 4157 1 99.6% 100.0% 100.0% 99.6% 0.04 7.87 0.00 --
25772 2023:094:05:16:11.148 5 -422.6 -259.9 2723 2672 2 99.6% 100.0% 100.0% 99.6% 0.02 7.87 0.00 --
25773 2023:095:20:11:24.917 5 -424.0 -256.5 2524 2456 0 99.6% 100.0% 100.0% 99.6% 0.02 7.88 0.00 --
25774 2023:096:02:53:24.532 5 -425.2 -255.5 4447 4387 2 99.7% 100.0% 100.0% 99.7% 0.02 7.87 0.00 --
27791 2023:099:09:44:48.559 5 -446.0 -221.1 12280 12214 8 99.8% 100.0% 100.0% 99.8% 0.05 7.89 0.00 --
25775 2023:105:05:05:45.295 5 -470.1 -166.6 7885 7826 4 99.8% 100.0% 100.0% 99.8% 0.03 7.88 0.00 --
25769 2023:180:20:20:12.266 5 -433.3 264.4 2993 2943 1 100.0% 100.0% 100.0% 100.0% 0.03 7.89 0.00 --
27925 2023:181:22:50:53.284 5 -449.7 236.5 3989 3936 2 99.9% 100.0% 100.0% 99.9% 0.03 7.89 0.00 --
25771 2023:188:04:50:57.288 5 -405.3 310.5 3011 2970 2 99.9% 100.0% 100.0% 99.9% 0.03 7.88 0.00 --
27941 2023:189:17:29:37.689 5 -402.6 309.2 4111 4053 0 100.0% 100.0% 100.0% 100.0% 0.03 7.88 0.00 --
25236 2023:209:02:28:22.581 7 86.0 498.8 3760 3692 1 100.0% 100.0% 100.0% 100.0% 0.03 7.89 0.00 --
27964 2023:209:14:38:05.696 7 93.7 497.2 3805 3692 4 100.0% 100.0% 100.0% 100.0% 0.03 7.88 0.00 --
25776 2023:271:15:25:30.678 5 391.6 306.4 7421 7345 4 100.0% 100.0% 100.0% 100.0% 0.03 7.88 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.