AGASC ID 1573072

Info

Last Obs. 2023:288:00:40
magcatalog 8.86 ± 0.09
mag3 arcsec 8.96 ± 0.04
mag5 arcsec 8.96 ± 0.04
Nobs 16 (0 bad)
fok 99.5%
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
60007 2004:285:08:07:19.613 1 57.4 -104.2 5168 5114 10 99.8% 100.0% 100.0% 99.8% 0.02 8.95 0.00 --
19453 2017:246:16:59:22.564 4 -393.8 -127.9 14287 14024 20 98.7% 100.0% 100.0% 98.7% 0.05 8.92 0.00 --
26730 2022:348:22:33:12.569 5 -34.7 -119.9 9603 9428 2 98.8% 99.9% 100.0% 98.7% 0.11 8.94 0.00 --
27133 2023:272:04:57:37.386 4 106.0 94.4 2602 2541 1 99.9% 100.0% 100.0% 99.9% 0.06 8.96 0.00 --
28935 2023:274:01:27:20.924 4 76.3 123.8 2772 2713 3 100.0% 99.9% 100.0% 99.9% 0.09 8.96 0.00 --
28936 2023:274:08:40:10.703 4 81.0 119.8 1959 1890 1 99.8% 99.9% 100.0% 99.8% 0.05 8.96 0.00 --
27132 2023:276:15:09:54.926 4 113.3 84.2 3805 3738 5 99.9% 100.0% 100.0% 99.9% 0.06 8.95 0.00 --
28949 2023:277:01:00:11.511 4 116.3 76.7 3074 3001 1 99.9% 100.0% 100.0% 99.9% 0.06 8.97 0.00 --
28950 2023:277:09:45:46.816 4 117.6 71.0 3272 3200 1 100.0% 99.9% 100.0% 99.9% 0.05 8.96 0.00 --
27130 2023:283:05:24:22.610 4 65.0 -99.6 2535 2482 1 100.0% 100.0% 100.0% 100.0% 0.04 9.00 0.00 --
28968 2023:283:13:32:08.487 4 60.0 -102.5 2538 2476 5 99.8% 100.0% 100.0% 99.8% 0.04 9.01 0.00 --
28969 2023:285:00:26:25.970 4 62.2 -104.2 2530 2478 1 100.0% 100.0% 100.0% 100.0% 0.07 9.00 0.00 --
27131 2023:285:15:31:19.558 4 39.7 -115.1 2532 2482 0 100.0% 100.0% 100.0% 100.0% 0.06 9.00 0.00 --
28970 2023:286:06:22:35.643 4 34.2 -117.0 3021 2970 5 100.0% 100.0% 100.0% 99.9% 0.04 8.99 0.00 --
27134 2023:287:09:14:52.339 4 24.2 -118.8 3025 2958 0 99.9% 100.0% 100.0% 99.9% 0.03 9.01 0.00 --
28971 2023:288:00:40:06.015 4 13.0 -121.5 3996 3933 1 99.9% 100.0% 100.0% 99.9% 0.08 9.00 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.