AGASC ID 472665288

Info

Last Obs. 2024:161:21:00
magcatalog 5.95 ± 0.04
mag3 arcsec 5.95 ± 0.02
mag5 arcsec 5.95 ± 0.02
Nobs 25 (0 bad)
fok 100.0%
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 mag ⟩ 100s ⟨ mag ⟩ σmag Comments
25594 2023:157:19:51:55.332 3 457.1 -484.0 371 308 0 100.0% 100.0% 100.0% 100.0% 0.01 5.92 0.00 --
25595 2023:157:20:48:00.332 3 469.3 -471.9 334 291 0 100.0% 100.0% 100.0% 100.0% 0.01 5.92 0.00 --
25596 2023:157:21:13:10.332 3 481.7 -484.3 333 291 0 100.0% 100.0% 100.0% 100.0% 0.00 5.92 0.00 --
25597 2023:157:21:38:20.332 7 469.5 -496.5 338 291 0 100.0% 100.0% 100.0% 100.0% 0.01 5.92 0.00 --
25598 2023:157:22:03:30.332 3 452.0 -466.6 332 292 0 100.0% 100.0% 100.0% 100.0% 0.01 5.92 0.00 --
25599 2023:157:22:28:40.332 6 486.7 -467.1 337 289 0 100.0% 100.0% 100.0% 100.0% 0.01 5.92 0.00 --
25602 2023:158:07:35:07.375 7 420.7 -494.4 523 412 0 100.0% 100.0% 100.0% 100.0% 0.01 5.92 0.00 --
25603 2023:158:08:31:12.375 3 457.2 -457.8 335 290 0 100.0% 100.0% 100.0% 100.0% 0.01 5.92 0.00 --
25606 2023:158:09:46:42.375 3 422.9 -459.1 332 292 0 100.0% 100.0% 100.0% 100.0% 0.01 5.92 0.00 --
25610 2023:160:16:49:53.225 3 403.5 -480.4 441 384 0 100.0% 100.0% 100.0% 100.0% 0.01 5.93 0.00 --
25611 2023:160:17:48:58.225 3 476.4 -407.7 334 292 0 100.0% 100.0% 100.0% 100.0% 0.01 5.93 0.00 --
25587 2023:340:23:45:10.444 3 -462.9 482.6 323 292 0 100.0% 100.0% 100.0% 100.0% 0.01 5.97 0.00 --
25590 2023:341:01:00:40.444 3 -411.3 478.6 326 292 0 100.0% 100.0% 100.0% 100.0% 0.01 5.97 0.00 --
28384 2024:155:08:07:43.274 3 478.6 -476.1 1376 1316 0 100.0% 100.0% 100.0% 100.0% 0.01 5.95 0.00 --
28385 2024:158:23:53:56.869 3 470.2 -477.8 514 454 0 100.0% 100.0% 100.0% 100.0% 0.02 5.96 0.00 --
28386 2024:159:00:53:01.869 3 482.4 -465.6 332 292 0 100.0% 100.0% 100.0% 100.0% 0.01 5.96 0.00 --
28388 2024:159:01:43:21.869 3 482.6 -490.2 333 291 0 100.0% 100.0% 100.0% 100.0% 0.01 5.96 0.00 --
28389 2024:159:02:08:31.869 3 465.0 -460.4 332 292 0 100.0% 100.0% 100.0% 100.0% 0.01 5.96 0.00 --
28392 2024:159:03:24:01.869 3 465.4 -495.1 332 292 0 100.0% 100.0% 100.0% 100.0% 0.01 5.96 0.00 --
28393 2024:159:03:49:11.869 3 445.9 -477.5 330 292 0 100.0% 100.0% 100.0% 100.0% 0.01 5.96 0.00 --
28394 2024:159:04:14:21.869 3 482.3 -441.2 332 292 0 100.0% 100.0% 100.0% 100.0% 0.01 5.96 0.00 --
28470 2024:160:15:34:35.516 3 440.2 -448.6 332 292 1 100.0% 100.0% 100.0% 100.0% 0.01 5.96 0.00 --
28470 2024:160:17:15:15.516 3 402.1 -482.3 330 292 0 100.0% 100.0% 100.0% 100.0% 0.01 5.96 0.00 --
28470 2024:160:17:15:15.516 3 402.1 -482.3 330 292 0 100.0% 100.0% 100.0% 100.0% 0.01 5.96 0.00 --
28470 2024:160:17:40:25.516 3 475.0 -409.6 333 291 0 100.0% 100.0% 100.0% 100.0% 0.01 5.96 0.00 --
28470 2024:160:17:40:25.516 3 475.0 -409.6 333 291 0 100.0% 100.0% 100.0% 100.0% 0.01 5.96 0.00 --
62617 2024:161:21:00:17.948 3 484.0 -475.9 1471 1417 0 100.0% 100.0% 100.0% 100.0% 0.01 5.96 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.