AGASC ID 58854408

Info

Last Obs. 2024:239:21:16
magcatalog 7.72 ± 0.02
mag3 arcsec 7.72 ± 0.02
mag5 arcsec 7.72 ± 0.02
Nobs 16 (0 bad)
fok 99.9%
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
11231 2009:223:07:27:09.585 4 80.9 273.7 27464 27332 34 99.7% 100.0% 100.0% 99.7% 0.02 7.71 0.00 --
51781 2015:186:01:18:33.313 1 206.5 363.2 246 196 1 100.0% 100.0% 100.0% 100.0% 0.01 7.71 0.00 --
51779 2015:186:04:02:51.540 1 204.7 364.2 340 288 0 99.7% 100.0% 100.0% 99.7% 0.01 7.71 0.00 --
51772 2015:188:18:55:40.054 2 205.9 -48.8 3718 3666 10 99.7% 100.0% 100.0% 99.7% 0.02 7.73 0.00 --
18921 2017:170:06:07:23.168 3 199.1 419.0 27496 27410 17 100.0% 100.0% 100.0% 100.0% 0.02 7.71 0.00 --
20100 2017:172:14:04:11.260 3 199.8 418.6 21574 21470 10 100.0% 100.0% 100.0% 100.0% 0.02 7.71 0.00 --
20101 2017:175:12:08:08.297 3 199.2 418.9 17224 17130 18 100.0% 100.0% 100.0% 100.0% 0.02 7.71 0.00 --
20102 2017:176:18:16:57.367 3 200.1 418.5 8497 8433 9 100.0% 100.0% 100.0% 100.0% 0.01 7.70 0.00 --
49986 2017:176:23:28:16.969 0 194.7 423.5 183 43 1 100.0% 100.0% 100.0% 100.0% 0.01 7.71 0.00 --
20103 2017:189:01:40:47.399 7 -73.9 462.1 14788 14712 7 100.0% 100.0% 100.0% 100.0% 0.03 7.71 0.00 --
49150 2018:185:02:57:20.098 1 -445.5 -4.9 820 766 2 100.0% 100.0% 100.0% 100.0% 0.01 7.72 0.00 --
27051 2022:326:01:52:22.242 4 47.1 93.6 2552 2502 1 100.0% 100.0% 100.0% 100.0% 0.02 7.73 0.00 --
27570 2022:327:22:31:11.671 4 50.6 91.9 4438 4358 1 99.8% 100.0% 100.0% 99.8% 0.04 7.73 0.00 --
62617 2024:161:23:07:53.948 4 -28.2 -79.7 7188 7135 2 100.0% 100.0% 100.0% 100.0% 0.04 7.75 0.00 --
26502 2024:203:04:05:13.190 3 71.6 -41.2 7158 7107 4 100.0% 100.0% 100.0% 100.0% 0.03 7.77 0.00 --
27053 2024:239:21:16:29.306 5 87.9 39.1 7411 7348 1 100.0% 100.0% 100.0% 100.0% 0.03 7.76 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.