AGASC ID 690636928

Info

Last Obs. 2024:005:16:43
magcatalog 9.20 ± 0.11
mag3 arcsec 9.29 ± 0.02
mag5 arcsec 9.29 ± 0.02
Nobs 14 (0 bad)
fok 97.9%
f3 arcsec 99.7%
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
4882 2004:247:05:40:58.992 6 -83.0 -418.8 5021 4960 7 99.9% 100.0% 100.0% 99.9% 0.03 9.26 0.00 --
4886 2004:247:17:21:38.992 7 313.7 -239.1 5022 4952 11 99.8% 100.0% 100.0% 99.8% 0.03 9.28 0.00 --
4887 2004:248:14:10:00.486 7 300.8 -438.6 5024 4966 5 99.9% 100.0% 100.0% 99.9% 0.02 9.27 0.00 --
59368 2005:299:06:12:42.136 5 -301.1 -271.7 91 40 0 97.6% 97.5% 97.5% 95.1% 0.02 9.27 0.00 --
10266 2009:150:21:17:03.273 5 362.5 393.3 5563 5400 14 98.6% 100.0% 100.0% 98.6% 0.03 9.26 0.00 --
15174 2013:221:14:22:24.060 6 199.7 -366.0 19702 19394 15 98.8% 100.0% 100.0% 98.8% 0.03 9.29 0.00 --
16263 2013:222:16:50:54.869 6 199.7 -366.0 19010 18731 22 98.9% 100.0% 100.0% 98.9% 0.04 9.29 0.00 --
53488 2013:223:04:14:43.967 6 199.7 -366.0 93 47 0 100.0% 100.0% 100.0% 100.0% 0.01 9.29 0.00 --
15173 2013:226:17:01:28.232 6 271.8 -375.2 21291 20427 18 96.3% 100.0% 100.0% 96.3% 0.04 9.29 0.00 --
16264 2013:229:09:00:00.653 6 271.8 -375.2 18380 17379 31 95.0% 100.0% 100.0% 95.0% 0.06 9.29 0.00 --
46604 2021:033:02:39:34.622 3 137.5 -43.1 2717 2120 27 94.9% 94.2% 99.6% 89.5% 0.06 9.29 0.00 --
28329 2023:359:02:01:05.135 5 -456.6 322.9 4958 4906 4 99.9% 99.8% 100.0% 99.7% 0.09 9.29 0.00 --
29169 2023:361:03:40:04.140 5 -447.9 334.4 3983 3932 3 99.9% 94.5% 100.0% 94.4% 0.10 9.29 0.00 --
29170 2024:005:16:43:39.101 5 -439.1 351.0 3253 3200 0 100.0% 100.0% 100.0% 99.9% 0.07 9.30 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.