AGASC ID 836111720

Info

Last Obs. 2024:240:08:51
magcatalog 7.14 ± 0.02
mag3 arcsec 7.16 ± 0.01
mag5 arcsec 7.16 ± 0.01
Nobs 14 (0 bad)
fok 100.0%
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
51734 2015:202:01:04:57.934 7 -290.0 -486.8 3706 3644 10 99.9% 100.0% 100.0% 99.9% 0.02 7.16 0.00 --
51616 2015:263:03:39:45.700 0 333.5 -303.5 1167 1103 0 99.9% 100.0% 100.0% 99.9% 0.01 7.16 0.00 --
25094 2021:201:11:54:03.969 7 460.3 -394.2 5028 4941 4 100.0% 100.0% 100.0% 100.0% 0.02 7.13 0.00 --
27197 2023:221:01:47:11.191 4 -91.1 -30.0 4973 4921 1 100.0% 100.0% 100.0% 100.0% 0.02 7.15 0.00 --
28371 2023:221:19:31:34.578 4 -89.0 -35.5 3744 3690 3 99.9% 100.0% 100.0% 99.9% 0.02 7.16 0.00 --
27194 2023:226:11:30:20.840 4 -99.5 35.0 3621 3573 0 100.0% 100.0% 100.0% 100.0% 0.02 7.16 0.00 --
28484 2023:230:14:56:57.591 4 -76.1 78.1 3864 3811 1 100.0% 100.0% 100.0% 100.0% 0.03 7.15 0.00 --
27195 2024:102:22:25:46.780 4 -43.5 -76.1 2527 2467 1 99.9% 100.0% 100.0% 99.9% 0.03 7.17 0.00 --
29369 2024:103:13:34:41.516 4 -45.5 -75.2 1670 1612 0 100.0% 100.0% 100.0% 100.0% 0.02 7.17 0.00 --
26930 2024:213:16:06:36.445 4 -56.2 -69.2 4234 4169 1 100.0% 100.0% 100.0% 100.0% 0.03 7.18 0.00 --
29493 2024:214:07:23:39.116 4 -58.0 -68.1 4354 4290 0 100.0% 100.0% 100.0% 100.0% 0.03 7.18 0.00 --
29494 2024:215:01:02:43.802 4 -59.5 -67.1 3704 3640 0 100.0% 100.0% 100.0% 100.0% 0.02 7.18 0.00 --
27196 2024:239:15:29:28.199 4 -9.9 109.7 4723 4678 1 100.0% 100.0% 100.0% 100.0% 0.03 7.17 0.00 --
29517 2024:240:08:51:11.241 4 -7.8 110.2 2530 2471 1 100.0% 100.0% 100.0% 100.0% 0.02 7.17 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.