AGASC ID 629016912

Info

Last Obs. 2023:004:12:51
magcatalog 7.76 ± 0.10
mag3 arcsec 7.78 ± 0.01
mag5 arcsec 7.78 ± 0.01
Nobs 14 (0 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
54005 2013:019:20:50:20.095 6 428.6 -484.8 1316 1316 1 100.0% 100.0% 100.0% 100.0% 0.01 7.78 0.00 --
25849 2021:341:18:11:31.348 4 300.0 199.4 13725 13628 6 99.3% 100.0% 100.0% 99.3% 0.03 7.77 0.00 --
25851 2021:364:09:08:40.801 6 340.4 -84.8 7402 7367 8 99.5% 100.0% 100.0% 99.5% 0.03 7.79 0.00 --
25850 2022:005:08:57:54.931 6 263.9 -221.4 6915 6910 6 99.9% 100.0% 100.0% 99.9% 0.02 7.78 0.00 --
26258 2022:005:16:53:50.955 5 296.5 -177.7 7145 7138 7 99.9% 100.0% 100.0% 99.9% 0.03 7.79 0.00 --
25853 2022:238:12:59:33.003 5 36.7 369.0 9836 9781 9 99.4% 100.0% 100.0% 99.4% 0.03 7.79 0.00 --
25854 2022:340:13:37:55.630 6 310.7 183.9 6282 6258 3 99.6% 100.0% 100.0% 99.6% 0.03 7.78 0.00 --
27595 2022:345:15:13:54.141 6 297.0 204.4 4295 4277 2 99.6% 100.0% 100.0% 99.6% 0.02 7.78 0.00 --
25848 2022:346:02:02:41.483 6 328.0 144.3 3697 3692 1 99.9% 100.0% 100.0% 99.9% 0.02 7.78 0.00 --
26259 2022:346:15:03:44.141 6 331.4 139.3 6615 6575 1 99.4% 100.0% 100.0% 99.4% 0.03 7.77 0.00 --
25852 2022:361:11:28:59.379 4 352.9 7.5 5388 5378 3 99.8% 100.0% 100.0% 99.8% 0.02 7.77 0.00 --
25847 2022:362:10:50:24.873 4 354.2 -11.9 5405 5355 1 99.1% 100.0% 100.0% 99.1% 0.03 7.80 0.00 --
27634 2022:362:21:16:37.727 4 352.4 -24.2 4415 4407 3 99.8% 100.0% 100.0% 99.8% 0.02 7.80 0.00 --
25125 2023:004:12:51:55.192 4 343.7 -80.2 5960 5929 2 99.5% 100.0% 100.0% 99.5% 0.03 7.79 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.