AGASC ID 24522960

Info

Last Obs. 2023:125:02:30
magcatalog 7.76 ± 0.10
mag3 arcsec 7.81 ± 0.01
mag5 arcsec 7.81 ± 0.01
Nobs 13 (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
4411 2003:342:08:33:58.773 5 -135.6 -21.1 23727 23720 10 100.0% 100.0% 100.0% 100.0% 0.01 7.81 0.00 --
5175 2004:347:11:05:54.118 5 133.0 -21.7 23019 23017 9 100.0% 100.0% 100.0% 100.0% 0.01 7.82 0.00 --
8908 2008:008:03:09:29.626 5 -208.2 -222.5 2529 2527 2 100.0% 100.0% 100.0% 100.0% 0.01 7.80 0.00 --
10994 2009:349:21:50:42.491 6 -23.2 -294.8 35186 35173 37 100.0% 100.0% 100.0% 100.0% 0.02 7.80 0.00 --
15701 2014:350:15:54:56.326 6 -25.0 -297.8 45985 45910 34 99.8% 100.0% 100.0% 99.8% 0.03 7.81 0.00 --
18304 2016:067:15:34:10.562 5 -176.9 278.4 4967 4962 3 99.9% 100.0% 100.0% 99.9% 0.01 7.80 0.00 --
18305 2016:251:02:30:21.667 6 164.5 -242.9 4961 4958 4 99.9% 100.0% 100.0% 99.9% 0.02 7.80 0.00 --
18307 2017:260:12:05:24.164 7 139.8 -258.7 4939 4933 3 99.9% 100.0% 100.0% 99.9% 0.02 7.80 0.00 --
18308 2018:047:00:14:08.802 7 -222.8 241.6 4936 4931 1 99.9% 100.0% 100.0% 99.9% 0.02 7.80 0.00 --
21578 2019:148:19:40:47.250 6 -43.1 322.1 2496 2485 4 99.6% 100.0% 100.0% 99.5% 0.02 7.80 0.00 --
21579 2020:019:13:36:49.899 6 -313.7 -40.9 2506 2493 4 99.5% 100.0% 100.0% 99.5% 0.02 7.82 0.00 --
21580 2021:095:17:01:13.279 6 -128.1 299.0 2516 2507 1 99.6% 100.0% 100.0% 99.6% 0.02 7.81 0.00 --
25503 2023:125:02:30:38.494 3 -88.7 313.6 937 936 0 100.0% 100.0% 100.0% 100.0% 0.02 7.80 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.