AGASC ID 340533352

Info

Last Obs. 2024:255:22:50
magcatalog 8.43 ± 0.02
mag3 arcsec 8.45 ± 0.02
mag5 arcsec 8.45 ± 0.02
Nobs 11 (0 bad)
fok 99.5%
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
2749 2002:125:09:59:17.235 7 307.1 343.1 24533 24468 21 100.0% 100.0% 100.0% 100.0% 0.01 8.44 0.00 --
2704 2002:186:17:32:25.678 4 -189.0 437.6 9197 9132 6 100.0% 100.0% 100.0% 100.0% 0.02 8.44 0.00 --
2705 2002:199:15:12:35.507 4 -274.1 390.7 9470 9302 5 100.0% 100.0% 100.0% 100.0% 0.02 8.44 0.00 --
4375 2002:307:06:56:06.380 5 -355.8 -284.8 9984 9930 4 99.9% 100.0% 100.0% 99.9% 0.02 8.45 0.00 --
3822 2003:343:23:34:10.180 3 -57.9 -441.8 14781 14699 10 100.0% 100.0% 100.0% 100.0% 0.02 8.44 0.00 --
6150 2004:336:08:43:01.462 4 -133.2 -424.1 11097 11030 16 99.9% 100.0% 100.0% 99.9% 0.01 8.44 0.00 --
23356 2020:225:05:18:01.338 4 -391.7 261.2 17213 16685 19 97.2% 100.0% 100.0% 97.2% 0.05 8.44 0.00 --
23360 2020:227:21:39:03.740 4 -392.0 261.3 7460 7301 13 98.5% 100.0% 100.0% 98.5% 0.02 8.44 0.00 --
28375 2023:224:22:38:45.621 6 -415.6 227.1 6181 6140 3 100.0% 100.0% 100.0% 100.0% 0.04 8.48 0.00 --
28768 2024:254:07:42:31.900 5 -461.1 86.8 5398 5353 0 99.9% 100.0% 100.0% 99.9% 0.04 8.50 0.00 --
29528 2024:255:22:50:10.956 5 -460.3 90.9 6790 6737 1 100.0% 100.0% 100.0% 99.9% 0.08 8.50 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.