AGASC ID 374355168

Info

Last Obs. 2026:092:11:16
magcatalog 8.54 ± 0.02
mag3 arcsec 8.54 ± 0.02
mag5 arcsec 8.54 ± 0.02
Nobs 16 (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
5597 2004:358:05:33:26.453 5 -20.4 -378.7 12491 12429 12 99.9% 100.0% 100.0% 99.9% 0.02 8.54 0.00 --
5596 2005:085:07:30:58.729 6 273.1 -229.3 2584 2527 7 99.9% 100.0% 100.0% 99.9% 0.01 8.56 0.00 --
8473 2006:318:20:20:27.595 7 -468.4 -38.6 14776 14683 19 99.9% 100.0% 100.0% 99.9% 0.02 8.57 0.00 --
9097 2007:349:00:51:35.025 4 -149.8 -425.7 17217 17151 25 99.9% 100.0% 100.0% 99.9% 0.02 8.54 0.00 --
17281 2015:345:20:41:17.816 6 -41.5 -193.8 2586 2511 1 99.4% 100.0% 100.0% 99.3% 0.02 8.54 0.00 --
17282 2015:345:22:18:48.599 7 77.5 -55.8 2588 2526 2 99.8% 100.0% 100.0% 99.8% 0.02 8.58 0.00 --
17280 2015:345:23:50:38.599 5 -429.9 33.6 2578 2520 2 99.7% 100.0% 100.0% 99.7% 0.02 8.56 0.00 --
20522 2018:253:09:05:55.108 5 172.6 -138.9 4051 3963 4 99.8% 100.0% 100.0% 99.8% 0.03 8.56 0.00 --
21956 2018:323:18:49:31.206 6 -51.4 296.1 13319 13222 22 99.9% 100.0% 100.0% 99.9% 0.04 8.53 0.00 --
21969 2018:325:16:23:56.678 6 -52.0 296.4 6490 6396 9 99.6% 100.0% 100.0% 99.6% 0.03 8.53 0.00 --
21972 2018:331:12:48:19.898 6 -115.3 279.0 10875 10690 12 99.0% 100.0% 100.0% 99.0% 0.03 8.53 0.00 --
21973 2018:334:03:42:58.998 6 -116.1 279.4 7216 7101 9 99.3% 100.0% 100.0% 99.3% 0.02 8.53 0.00 --
21529 2018:334:10:20:21.511 6 -116.0 279.3 9415 9265 10 99.3% 100.0% 100.0% 99.3% 0.03 8.53 0.00 --
23702 2020:303:06:44:20.074 5 79.0 434.8 1330 1243 0 99.5% 100.0% 100.0% 99.5% 0.02 8.55 0.00 --
26219 2021:339:15:24:24.704 7 156.0 67.7 5682 5512 8 98.5% 100.0% 100.0% 98.5% 0.04 8.56 0.00 --
41579 2026:092:11:16:32.227 0 433.8 -2.8 1062 987 0 99.9% 100.0% 100.0% 99.9% 0.04 8.62 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.