AGASC ID 818808880

Info

Last Obs. 2022:161:04:38
magcatalog 9.53 ± 0.10
mag3 arcsec 9.55 ± 0.02
mag5 arcsec 9.55 ± 0.02
Nobs 14 (0 bad)
fok 98.7%
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 mag100s ⟨ mag ⟩ σmag Comments
4650 2004:300:04:00:35.323 5 445.6 133.3 23741 22956 18 98.7% 100.0% 100.0% 98.7% 0.05 9.52 0.00 --
6714 2006:117:23:01:11.739 5 -421.4 -99.6 78758 78051 119 99.7% 100.0% 100.0% 99.7% 0.04 9.56 0.00 --
6716 2006:125:19:11:49.510 5 -420.2 -103.8 78801 77052 102 97.8% 100.0% 100.0% 97.8% 0.06 9.55 0.00 --
6717 2006:194:18:48:21.508 6 456.4 96.5 52775 52660 65 99.8% 100.0% 100.0% 99.8% 0.04 9.54 0.00 --
7366 2006:197:05:09:43.157 6 456.4 96.5 25455 25390 37 99.7% 100.0% 100.0% 99.7% 0.03 9.54 0.00 --
6718 2006:202:14:30:34.368 6 455.4 101.3 53304 52885 1402 99.2% 100.0% 100.0% 99.2% 0.08 9.55 0.00 --
6715 2006:215:16:26:22.866 7 454.0 108.2 79276 78655 109 99.8% 100.0% 100.0% 99.7% 0.04 9.55 0.00 --
16004 2014:133:17:30:07.787 4 -438.6 -133.1 51075 49797 43 97.5% 100.0% 100.0% 97.5% 0.08 9.55 0.00 --
16614 2014:136:08:16:00.868 4 -438.6 -133.1 18285 18008 10 98.5% 100.0% 100.0% 98.5% 0.05 9.57 0.00 --
15796 2015:039:10:45:33.979 6 419.8 -201.0 2533 2474 4 97.7% 100.0% 100.0% 97.7% 0.05 9.53 0.00 --
17901 2016:202:18:28:27.968 5 439.7 98.1 72967 71029 97 97.3% 100.0% 100.0% 97.3% 0.08 9.55 0.00 --
50834 2016:204:12:37:23.529 4 439.7 98.1 52 49 0 94.2% 100.0% 100.0% 94.2% 0.01 9.56 0.00 --
24245 2022:160:07:00:29.439 7 -304.2 -339.2 7823 7657 8 97.9% 99.9% 100.0% 97.8% 0.10 9.61 0.00 --
26385 2022:161:04:38:20.823 7 -303.0 -339.8 7797 7615 7 97.7% 99.5% 100.0% 97.2% 0.12 9.58 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.