AGASC ID 260979504

Info

Last Obs. 2023:065:13:48
magcatalog 6.01 ± 0.05
mag3 arcsec 6.04 ± 0.01
mag5 arcsec 6.04 ± 0.01
Nobs 12 (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
4772 2004:098:17:40:05.803 7 -201.8 187.8 2230 2230 1 100.0% 100.0% 100.0% 100.0% 0.01 6.04 0.00 --
4741 2005:034:11:55:02.433 7 204.5 450.4 19005 19005 2 100.0% 100.0% 100.0% 100.0% 0.01 6.04 0.00 --
7077 2006:075:13:55:30.981 7 -308.9 384.5 54502 54498 16 100.0% 100.0% 100.0% 100.0% 0.01 6.04 0.00 --
7108 2006:095:22:39:31.322 7 -477.1 385.4 1815 1347 0 100.0% 100.0% 100.0% 100.0% 0.01 6.06 0.00 --
7078 2006:206:09:56:54.746 7 -279.2 -374.8 26318 25849 4 100.0% 100.0% 100.0% 100.0% 0.01 6.04 0.00 --
7080 2007:110:12:28:15.175 7 -480.0 10.3 27696 27696 13 100.0% 100.0% 100.0% 100.0% 0.01 6.05 0.00 --
11269 2010:074:18:52:39.480 7 -324.0 366.0 40856 40854 10 100.0% 100.0% 100.0% 100.0% 0.01 6.03 0.00 --
12124 2010:079:15:27:57.661 7 -324.0 366.0 12772 12771 4 100.0% 100.0% 100.0% 100.0% 0.01 6.03 0.00 --
19561 2018:080:14:12:50.758 6 -102.6 255.8 15692 15692 2 100.0% 100.0% 100.0% 100.0% 0.01 6.03 0.00 --
21045 2018:081:09:22:52.840 7 -102.6 255.8 14369 14369 6 100.0% 100.0% 100.0% 100.0% 0.01 6.03 0.00 --
21046 2018:151:23:16:58.177 7 -269.6 25.0 18616 18616 2 100.0% 100.0% 100.0% 100.0% 0.01 6.04 0.00 --
25438 2023:065:13:48:06.354 3 346.9 342.5 1351 1351 0 100.0% 100.0% 100.0% 100.0% 0.01 6.03 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.