AGASC ID 1130630400

Info

Last Obs. 2022:159:09:03
magcatalog 8.55 ± 0.10
mag3 arcsec 8.54 ± 0.01
mag5 arcsec 8.54 ± 0.01
Nobs 13 (0 bad)
fok 99.2%
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
4495 2004:265:17:23:55.929 4 -441.6 -329.9 29562 29069 30 99.9% 100.0% 100.0% 99.9% 0.02 8.54 0.00 --
5400 2005:248:14:34:19.897 3 -391.0 -450.0 16673 16657 20 99.9% 100.0% 100.0% 99.9% 0.01 8.54 0.00 --
5397 2005:333:22:21:58.714 3 -438.0 368.8 5846 5377 13 99.9% 100.0% 100.0% 99.9% 0.01 8.54 0.00 --
7228 2005:335:12:06:29.161 3 -438.0 368.8 9869 9862 14 99.9% 100.0% 100.0% 99.9% 0.01 8.54 0.00 --
7229 2005:336:08:28:41.666 3 -438.0 368.8 9670 9662 9 99.9% 100.0% 100.0% 99.9% 0.02 8.54 0.00 --
9499 2008:151:00:21:21.282 4 316.5 -198.1 16270 15778 26 99.9% 100.0% 100.0% 99.9% 0.02 8.54 0.00 --
9861 2008:173:05:06:30.811 3 233.7 -288.5 14044 14022 25 99.9% 100.0% 100.0% 99.8% 0.02 8.54 0.00 --
9484 2008:232:06:24:51.788 3 -278.1 -393.0 27636 27526 37 99.6% 100.0% 100.0% 99.6% 0.02 8.53 0.00 --
20803 2017:288:17:50:07.768 7 468.5 88.1 15841 15515 7 97.9% 100.0% 100.0% 97.9% 0.03 8.51 0.00 --
20152 2018:170:08:29:37.796 3 296.2 -451.2 12282 12181 16 99.2% 100.0% 100.0% 99.2% 0.03 8.53 0.00 --
24670 2022:047:05:44:24.468 4 308.9 467.9 24452 24111 19 98.6% 100.0% 100.0% 98.6% 0.08 8.54 0.00 --
25127 2022:149:23:01:27.489 5 423.5 -331.8 14712 14203 7 96.5% 100.0% 100.0% 96.5% 0.05 8.56 0.00 --
25128 2022:159:09:03:58.133 4 367.2 -393.2 14704 14442 14 98.2% 100.0% 100.0% 98.2% 0.06 8.55 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.