AGASC ID 837161472

Info

Last Obs. 2023:269:00:11
magcatalog 9.63 ± 0.09
mag3 arcsec 9.63 ± 0.02
mag5 arcsec 9.63 ± 0.02
Nobs 15 (1 bad)
fok 99.4%
f3 arcsec 99.9%
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
2977 2002:254:00:42:32.835 6 119.3 393.0 72679 72507 71 99.9% 100.0% 100.0% 99.8% 0.08 9.61 0.00 --
2966 2002:357:16:32:40.981 3 359.5 171.7 38699 38565 21 99.9% 100.0% 100.0% 99.9% 0.07 9.60 0.00 --
12828 2011:269:20:23:37.709 3 275.6 292.0 79827 79593 100 99.8% 100.0% 100.0% 99.8% 0.05 9.63 0.00 --
12829 2011:272:06:45:59.701 3 275.6 292.0 91966 91507 250 99.6% 100.0% 100.0% 99.5% 0.10 9.61 0.00 --
55153 2011:274:11:40:53.663 0 275.6 292.0 93 47 0 100.0% 100.0% 100.0% 100.0% 0.01 9.55 0.00 --
12830 2011:274:22:42:04.425 3 275.6 292.0 24137 23992 77 99.6% 100.0% 100.0% 99.6% 0.09 9.61 0.00 --
24465 2021:221:20:48:44.820 3 -407.8 -7.3 14776 14352 19 97.6% 100.0% 100.0% 97.6% 0.08 9.68 0.00 --
23678 2021:237:12:45:36.488 3 -310.5 273.1 13312 12944 18 97.8% 99.9% 100.0% 97.8% 0.11 9.66 0.00 --
25983 2021:238:08:09:22.671 3 -311.8 273.6 12336 12135 23 98.9% 99.9% 100.0% 98.8% 0.09 9.66 0.00 --
24469 2021:240:02:29:47.224 3 -311.3 273.4 12825 12522 21 98.1% 100.0% 100.0% 98.0% 0.10 9.66 0.00 --
24784 2021:245:12:49:45.504 3 -172.2 376.4 12294 11664 16 98.4% 99.9% 100.0% 98.4% 0.12 9.64 0.00 --
24520 2021:245:12:49:45.504 3 -172.2 376.6 12350 11663 16 98.4% 99.9% 100.0% 98.4% 0.12 9.64 0.00 --
28873 2023:243:12:36:40.646 6 -205.1 356.8 1090 1027 3 99.4% 81.0% 97.2% 80.5% 0.13 9.62 0.00 --
24464 2023:243:14:35:21.102 7 -258.7 320.1 2039 1992 2 99.5% 92.2% 98.7% 91.8% 0.18 9.61 0.00 --
28883 2023:250:18:25:19.047 7 40.5 407.6 3659 3591 4 99.8% 96.3% 100.0% 96.1% 0.15 9.65 0.00 --
24463 2023:269:00:11:53.717 7 303.1 263.7 0 0 -1 0.0% 0.0% 0.0% 0.0% inf inf inf Error: No level 0 data.

  • 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.