AGASC ID 4857864

Info

Last Obs. 2023:015:11:41
magcatalog 8.51 ± 0.11
mag3 arcsec 8.52 ± 0.02
mag5 arcsec 8.52 ± 0.02
Nobs 14 (0 bad)
fok 98.5%
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
4099 2003:238:02:43:52.786 4 -262.1 -221.8 1757 1756 0 100.0% 100.0% 100.0% 100.0% 0.02 8.52 0.00 --
9223 2008:169:19:13:45.756 3 -195.1 -284.0 2604 2146 0 100.0% 100.0% 100.0% 100.0% 0.02 8.50 0.00 --
17078 2014:322:07:01:19.601 7 421.0 490.6 14727 14636 13 99.4% 100.0% 100.0% 99.4% 0.04 8.54 0.00 --
25805 2022:292:14:56:54.366 6 -259.3 288.1 7400 7322 9 98.9% 100.0% 100.0% 98.9% 0.03 8.52 0.00 --
27515 2022:293:00:37:40.166 6 -260.3 288.7 7408 7249 6 97.9% 100.0% 100.0% 97.9% 0.03 8.54 0.00 --
25806 2022:293:11:06:05.692 6 -260.9 288.9 4948 4867 9 98.4% 100.0% 100.0% 98.3% 0.03 8.54 0.00 --
27520 2022:301:07:37:24.836 6 40.6 395.1 6981 6680 392 97.6% 99.5% 99.5% 97.1% 0.04 8.51 0.00 --
25237 2022:301:17:02:51.131 6 39.6 395.7 7388 7324 8 99.1% 100.0% 100.0% 99.1% 0.03 8.52 0.00 --
27485 2022:305:02:19:24.527 7 169.1 361.1 7499 7271 9 97.0% 100.0% 100.0% 96.9% 0.02 8.51 0.00 --
27533 2022:305:19:45:47.000 7 -0.0 396.8 6897 6742 8 97.8% 100.0% 100.0% 97.8% 0.03 8.54 0.00 --
27534 2022:306:14:41:25.180 7 138.6 373.6 6692 6646 5 99.3% 100.0% 100.0% 99.3% 0.05 8.51 0.00 --
25804 2022:307:20:15:33.514 7 249.4 311.3 4941 4884 2 98.8% 100.0% 100.0% 98.8% 0.04 8.50 0.00 --
25807 2022:312:08:15:11.129 7 237.2 320.2 2597 2573 2 99.1% 99.9% 100.0% 99.0% 0.02 8.52 0.00 --
27516 2023:015:11:41:23.019 7 366.1 157.4 3453 3395 4 98.3% 100.0% 100.0% 98.3% 0.05 8.51 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.