AGASC ID 157953216

Info

Last Obs. 2024:365:12:13
magcatalog 9.38 ± 0.02
mag3 arcsec 9.38 ± 0.02
mag5 arcsec 9.38 ± 0.02
Nobs 14 (0 bad)
fok 98.9%
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
4753 2003:324:04:04:06.951 5 -364.8 -76.4 2757 2693 1 100.0% 100.0% 100.0% 100.0% 0.04 9.39 0.00 --
54828 2012:057:20:56:41.152 5 112.4 200.9 968 894 3 97.4% 99.7% 100.0% 97.1% 0.02 9.35 0.00 --
14801 2013:233:15:24:27.037 5 323.2 172.1 5024 4911 7 99.3% 100.0% 100.0% 99.3% 0.04 9.36 0.00 --
53462 2013:233:18:45:57.193 5 323.2 172.1 561 511 0 99.0% 100.0% 100.0% 99.0% 0.03 9.36 0.00 --
16000 2013:264:06:25:50.572 6 305.0 205.7 19705 19342 17 98.6% 100.0% 100.0% 98.6% 0.06 9.36 0.00 --
16001 2013:280:23:36:29.790 4 268.4 255.6 7441 7259 8 99.3% 100.0% 100.0% 99.3% 0.04 9.38 0.00 --
16484 2013:283:14:12:30.277 4 268.4 255.6 7384 7135 13 97.8% 100.0% 100.0% 97.8% 0.04 9.39 0.00 --
16485 2013:284:10:53:41.891 4 268.4 255.6 4956 4733 4 98.3% 100.0% 100.0% 98.3% 0.04 9.38 0.00 --
16002 2013:318:19:47:01.269 5 -372.2 -56.3 19012 18939 25 99.9% 100.0% 100.0% 99.9% 0.03 9.38 0.00 --
16003 2013:349:15:36:04.966 6 -359.1 -105.9 20093 19706 13 98.4% 100.0% 100.0% 98.4% 0.05 9.40 0.00 --
53162 2013:350:03:39:04.881 4 -359.1 -105.9 575 528 0 99.2% 100.0% 100.0% 99.2% 0.03 9.41 0.00 --
21000 2018:273:20:16:41.142 6 253.6 272.3 5033 4900 5 98.5% 100.0% 100.0% 98.5% 0.06 9.39 0.00 --
20333 2018:308:10:42:10.074 7 -373.9 72.0 7976 7788 12 98.5% 100.0% 100.0% 98.4% 0.06 9.37 0.00 --
30486 2024:365:12:13:55.474 7 -375.1 42.6 3806 3766 0 99.9% 97.5% 100.0% 97.5% 0.12 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.