AGASC ID 500437816

Info

Last Obs. 2026:122:17:29
magcatalog 8.66 ± 0.02
mag3 arcsec 8.68 ± 0.01
mag5 arcsec 8.68 ± 0.01
Nobs 16 (0 bad)
fok 99.4%
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
7851 2006:361:16:06:04.026 5 -261.1 -465.2 2588 2531 10 99.7% 100.0% 100.0% 99.7% 0.01 8.68 0.00 --
12076 2010:017:12:35:14.703 6 102.0 -353.3 1652 1602 1 100.0% 100.0% 100.0% 100.0% 0.02 8.69 0.00 --
12077 2010:032:00:07:08.557 5 232.4 -284.5 1610 1557 2 99.9% 100.0% 100.0% 99.9% 0.02 8.69 0.00 --
12078 2010:049:06:10:03.646 6 337.2 -151.9 1611 1553 1 99.9% 100.0% 100.0% 99.9% 0.02 8.70 0.00 --
12080 2010:074:11:09:35.773 6 374.3 30.6 1610 1527 2 99.9% 100.0% 100.0% 99.9% 0.02 8.67 0.00 --
12081 2010:088:21:01:41.484 6 353.0 140.0 1612 1546 6 99.8% 100.0% 100.0% 99.8% 0.01 8.68 0.00 --
12082 2010:103:12:47:25.147 5 339.0 174.5 1611 1556 1 100.0% 100.0% 100.0% 100.0% 0.02 8.67 0.00 --
12083 2010:117:12:50:36.729 7 309.3 227.2 1615 1538 2 99.9% 100.0% 100.0% 99.9% 0.02 8.67 0.00 --
12084 2010:135:04:03:41.404 6 261.7 284.8 1612 1554 2 100.0% 100.0% 100.0% 100.0% 0.02 8.68 0.00 --
12085 2010:145:22:24:46.258 5 225.5 316.5 1613 1549 0 99.8% 100.0% 100.0% 99.8% 0.02 8.68 0.00 --
12086 2010:161:09:32:50.928 6 160.1 357.1 1766 1707 4 100.0% 100.0% 100.0% 100.0% 0.02 8.67 0.00 --
12087 2010:174:22:36:57.323 4 84.9 384.6 1612 1543 3 99.9% 100.0% 100.0% 99.9% 0.02 8.68 0.00 --
19307 2018:030:20:50:14.778 5 96.1 -406.6 26387 26131 19 99.3% 100.0% 100.0% 99.3% 0.06 8.67 0.00 --
20947 2018:032:02:56:55.900 5 95.7 -406.5 22100 21812 15 99.0% 100.0% 100.0% 99.0% 0.04 8.68 0.00 --
47918 2019:246:01:29:13.455 3 -88.1 81.8 1340 1255 0 98.4% 100.0% 100.0% 98.4% 0.03 8.66 0.00 --
31627 2026:122:17:29:12.403 7 422.0 41.0 7141 7071 0 100.0% 100.0% 100.0% 100.0% 0.10 8.69 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.