AGASC ID 76556792

Info

Last Obs. 2024:264:03:41
magcatalog 8.53 ± 0.02
mag3 arcsec 8.55 ± 0.03
mag5 arcsec 8.55 ± 0.03
Nobs 12 (0 bad)
fok 98.8%
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 mag ⟩ 100s ⟨ mag ⟩ σmag Comments
24257 2020:266:00:49:03.336 5 -18.8 -423.6 12331 12056 16 98.2% 100.0% 100.0% 98.2% 0.03 8.53 0.00 --
24256 2020:268:02:32:21.780 5 -19.0 -423.5 7459 7276 8 98.3% 100.0% 100.0% 98.3% 0.04 8.54 0.00 --
24658 2020:268:17:34:21.495 5 -18.7 -423.6 7458 7186 16 97.1% 100.0% 100.0% 97.0% 0.03 8.53 0.00 --
23379 2020:270:19:31:30.237 5 -19.1 -423.4 13070 12851 15 98.7% 100.0% 100.0% 98.7% 0.03 8.54 0.00 --
24657 2020:271:08:57:23.050 5 -20.2 -422.9 12823 12633 13 99.1% 100.0% 100.0% 99.1% 0.03 8.54 0.00 --
45878 2021:339:22:10:38.284 5 -243.2 -369.2 1240 1168 11 98.2% 99.5% 99.8% 97.6% 0.03 8.55 0.00 --
28889 2023:251:18:23:03.821 6 -442.2 -8.1 3744 3684 1 99.9% 100.0% 100.0% 99.9% 0.07 8.60 0.00 --
27058 2024:241:03:15:28.467 7 -409.7 177.1 3751 3622 3 100.0% 100.0% 100.0% 100.0% 0.06 8.60 0.00 --
29516 2024:245:10:54:49.020 7 -421.7 139.6 3787 3734 1 99.9% 100.0% 100.0% 99.9% 0.05 8.59 0.00 --
27057 2024:258:06:20:08.828 6 -352.6 -253.9 3645 3597 3 100.0% 99.9% 100.0% 99.9% 0.07 8.59 0.00 --
26503 2024:260:22:56:47.222 6 -332.1 -278.3 2980 2931 0 99.9% 100.0% 100.0% 99.9% 0.05 8.60 0.00 --
30076 2024:264:03:41:07.532 7 -245.4 -352.6 2618 2565 1 100.0% 100.0% 100.0% 100.0% 0.06 8.58 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.