AGASC ID 472655704

Info

Last Obs. 2024:179:23:01
magcatalog 9.50 ± 0.06
mag3 arcsec 9.48 ± 0.03
mag5 arcsec 9.48 ± 0.03
Nobs 34 (0 bad)
fok 99.6%
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
2614 2002:027:03:12:21.680 6 -138.6 -360.0 630 581 2 99.3% 99.8% 100.0% 99.1% 0.04 9.46 0.00 --
2622 2002:027:06:33:41.680 7 -258.8 -409.4 630 587 16 100.0% 100.0% 100.0% 100.0% 0.04 9.47 0.00 --
2653 2002:221:14:32:30.206 7 67.5 362.2 635 580 0 99.8% 100.0% 100.0% 99.8% 0.02 9.47 0.00 --
2656 2002:222:07:45:06.437 7 114.9 362.4 587 525 0 99.1% 100.0% 100.0% 99.1% 0.02 9.48 0.00 --
2658 2002:222:08:53:42.785 7 186.2 362.7 633 577 0 99.7% 100.0% 100.0% 99.7% 0.03 9.47 0.00 --
2661 2002:222:10:09:12.785 7 90.6 362.5 635 582 0 100.0% 100.0% 100.0% 100.0% 0.04 9.48 0.00 --
4333 2003:053:00:58:57.936 5 -60.3 -313.3 631 572 0 99.1% 100.0% 100.0% 99.1% 0.04 9.45 0.00 --
4335 2003:053:01:49:17.936 4 -36.1 -337.6 632 574 0 99.7% 100.0% 100.0% 99.7% 0.02 9.45 0.00 --
4336 2003:053:02:14:27.936 4 12.0 -313.4 633 577 1 99.7% 99.8% 100.0% 99.5% 0.07 9.51 0.00 --
4338 2003:053:03:04:47.936 4 36.2 -313.4 631 579 1 99.8% 100.0% 100.0% 99.8% 0.02 9.48 0.00 --
4340 2003:053:03:55:07.936 4 60.4 -337.7 631 579 0 100.0% 100.0% 100.0% 100.0% 0.03 9.50 0.00 --
4344 2003:053:05:35:47.936 5 132.8 -337.9 631 580 1 99.7% 100.0% 100.0% 99.7% 0.05 9.50 0.00 --
4346 2003:053:06:26:07.936 4 13.2 -337.5 632 578 1 99.8% 100.0% 100.0% 99.8% 0.02 9.49 0.00 --
4348 2003:053:07:16:27.936 4 -34.5 -313.2 628 577 1 99.5% 100.0% 100.0% 99.5% 0.04 9.44 0.00 --
4350 2003:053:08:06:47.936 4 -106.2 -337.4 635 570 62 97.9% 100.0% 100.0% 97.9% 0.08 9.45 0.00 --
4352 2003:053:08:57:07.936 4 37.9 -337.6 632 579 0 100.0% 100.0% 100.0% 100.0% 0.02 9.50 0.00 --
4300 2003:053:13:35:10.081 5 15.2 -361.7 630 579 11 99.8% 100.0% 100.0% 99.8% 0.08 9.51 0.00 --
4304 2003:053:15:15:50.081 4 15.7 -337.4 633 573 0 99.1% 100.0% 100.0% 99.1% 0.02 9.49 0.00 --
4306 2003:053:16:06:10.081 4 -32.0 -313.1 630 572 0 99.1% 100.0% 100.0% 99.1% 0.05 9.43 0.00 --
4307 2003:053:16:31:20.081 4 64.0 -313.2 629 580 0 100.0% 100.0% 100.0% 100.0% 0.03 9.47 0.00 --
4308 2003:053:16:56:30.081 6 -104.1 -434.5 631 576 0 100.0% 100.0% 100.0% 100.0% 0.05 9.45 0.00 --
4309 2003:053:17:21:40.081 5 136.2 -434.9 632 581 0 100.0% 100.0% 100.0% 100.0% 0.02 9.49 0.00 --
4322 2003:244:14:32:20.841 6 -185.3 366.5 631 580 1 99.8% 100.0% 100.0% 99.8% 0.02 9.47 0.00 --
13085 2011:262:13:44:52.195 7 -63.1 272.6 642 574 0 99.1% 100.0% 100.0% 99.1% 0.02 9.43 0.00 --
17370 2015:269:23:24:50.969 6 -344.9 389.0 626 560 0 96.2% 100.0% 100.0% 96.2% 0.05 9.44 0.00 --
27247 2023:151:11:51:46.224 7 303.7 122.6 2589 2526 1 99.9% 99.9% 100.0% 99.8% 0.09 9.49 0.00 --
25571 2023:337:22:33:22.459 7 -315.6 -106.5 1477 1421 1 99.9% 100.0% 100.0% 99.9% 0.11 9.54 0.00 --
25573 2023:338:01:04:17.459 7 -306.8 -98.4 335 292 0 100.0% 100.0% 100.0% 100.0% 0.03 9.52 0.00 --
25590 2023:341:01:00:40.444 7 -258.4 -171.5 345 291 0 100.0% 100.0% 100.0% 100.0% 0.08 9.49 0.00 --
28385 2024:158:23:53:56.869 7 275.8 162.0 510 455 0 100.0% 99.1% 100.0% 99.1% 0.08 9.49 0.00 --
28470 2024:160:17:40:25.516 7 288.9 231.4 336 291 0 100.0% 99.7% 100.0% 99.7% 0.09 9.53 0.00 --
28397 2024:179:20:05:17.327 6 205.6 263.5 330 291 0 100.0% 100.0% 100.0% 100.0% 0.06 9.55 0.00 --
28402 2024:179:22:11:07.327 7 240.1 301.9 330 291 0 100.0% 95.2% 100.0% 95.2% 0.06 9.55 0.00 --
28404 2024:179:23:01:27.327 7 239.6 157.1 330 289 0 99.7% 100.0% 100.0% 99.7% 0.08 9.55 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.