AGASC ID 1091706216

Info

Last Obs. 2025:157:05:48
magcatalog 9.04 ± 0.02
mag3 arcsec 9.03 ± 0.01
mag5 arcsec 9.03 ± 0.01
Nobs 14 (1 bad)
fok 99.6%
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
4434 2003:111:03:20:10.850 7 231.7 126.7 23020 22911 25 99.8% 100.0% 100.0% 99.8% 0.03 9.03 0.00 --
4568 2004:217:13:07:13.347 7 -173.1 10.1 24532 24460 20 99.9% 100.0% 100.0% 99.9% 0.02 9.02 0.00 --
6261 2005:124:19:22:31.978 5 452.9 275.5 5028 4962 6 99.9% 100.0% 100.0% 99.9% 0.02 9.03 0.00 --
8155 2007:296:12:57:39.799 4 168.6 64.6 1368 1300 0 99.9% 99.9% 99.9% 99.8% 0.03 9.01 0.00 --
10088 2009:173:16:23:43.158 6 -58.6 282.8 5023 4964 10 99.8% 100.0% 100.0% 99.8% 0.02 9.01 0.00 --
10982 2010:156:11:46:15.349 4 31.2 369.1 48923 48794 79 99.9% 100.0% 100.0% 99.9% 0.02 9.03 0.00 --
12519 2011:164:04:07:34.267 3 337.9 -457.5 9659 9571 17 99.8% 100.0% 100.0% 99.8% 0.02 9.03 0.00 --
55355 2011:166:01:21:11.650 6 124.2 -211.4 95 47 1 100.0% 100.0% 100.0% 100.0% 0.01 9.04 0.00 --
12530 2011:167:12:28:21.290 6 -52.4 -110.3 9779 9699 10 99.7% 100.0% 100.0% 99.7% 0.03 9.02 0.00 --
19004 2017:036:10:07:47.308 7 152.3 15.1 19490 19146 22 98.6% 100.0% 100.0% 98.5% 0.04 9.02 0.00 --
50328 2017:036:21:35:44.604 6 151.4 19.2 244 115 1 94.3% 100.0% 100.0% 94.3% 0.01 9.03 0.00 --
20148 2018:168:04:20:54.523 4 223.4 285.2 5032 4936 10 99.7% 100.0% 100.0% 99.6% 0.03 9.01 0.00 --
22377 2020:158:01:12:44.895 5 -50.3 -144.7 12344 12149 16 98.9% 100.0% 100.0% 98.9% 0.06 9.01 0.00 --
28008 2025:157:05:48:43.363 6 -182.5 271.3 0 0 -1 0.0% 0.0% 0.0% 0.0% inf inf inf Error: No level 0 data.

  • 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.