AGASC ID 684983496

Info

Last Obs. 2024:244:05:40
magcatalog 9.40 ± 0.02
mag3 arcsec 9.38 ± 0.03
mag5 arcsec 9.38 ± 0.03
Nobs 13 (0 bad)
fok 98.0%
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
57662 2008:217:15:02:04.009 3 235.8 -155.9 3218 3161 10 99.8% 100.0% 100.0% 99.8% 0.03 9.42 0.00 --
14194 2011:221:09:49:15.601 3 -233.3 376.6 7189 6936 10 97.6% 99.9% 100.0% 97.5% 0.03 9.36 0.00 --
55253 2011:221:14:22:14.245 0 -233.3 376.6 84 46 0 95.8% 100.0% 100.0% 95.8% 0.01 9.36 0.00 --
15107 2013:265:22:55:19.466 3 -300.6 -430.8 5070 5001 8 99.7% 100.0% 100.0% 99.7% 0.03 9.38 0.00 --
15312 2013:272:15:41:25.676 3 -310.6 -453.5 9899 9837 9 99.9% 100.0% 100.0% 99.8% 0.03 9.37 0.00 --
23547 2020:309:15:37:51.052 4 410.2 430.1 9908 9711 25 98.7% 100.0% 100.0% 98.7% 0.04 9.40 0.00 --
23548 2020:315:16:48:43.526 4 405.3 435.8 9942 9707 14 98.8% 100.0% 100.0% 98.8% 0.08 9.39 0.00 --
23549 2020:330:22:48:13.541 4 391.8 449.1 9995 9643 5 97.0% 99.9% 99.9% 97.0% 0.11 9.39 0.00 --
23550 2020:359:02:03:30.564 4 401.3 440.8 9875 9619 18 98.3% 99.6% 100.0% 97.9% 0.11 9.35 0.00 --
23552 2021:158:04:12:04.262 3 -401.1 -434.2 19651 18803 23 95.9% 100.0% 100.0% 95.9% 0.08 9.39 0.00 --
46103 2021:248:23:32:09.464 1 -242.8 -70.4 321 261 1 98.5% 100.0% 100.0% 98.5% 0.04 9.42 0.00 --
43195 2024:241:16:35:47.471 5 -324.5 -379.3 810 761 0 99.9% 100.0% 100.0% 99.9% 0.07 9.44 0.00 --
43187 2024:244:05:40:16.010 5 -172.9 -469.2 815 765 0 100.0% 98.4% 99.9% 98.4% 0.08 9.46 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.