AGASC ID 137102976

Info

Last Obs. 2024:201:11:30
magcatalog 8.54 ± 0.05
mag3 arcsec 8.54 ± 0.03
mag5 arcsec 8.54 ± 0.03
Nobs 14 (0 bad)
fok 99.7%
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
4589 2004:097:21:04:48.965 5 13.1 -264.8 14786 14696 18 99.9% 100.0% 100.0% 99.9% 0.02 8.53 0.00 --
6581 2005:337:16:09:11.596 5 -175.6 243.5 10141 10079 8 100.0% 100.0% 100.0% 100.0% 0.02 8.50 0.00 --
6586 2006:182:21:36:04.673 6 133.1 -235.2 14702 14582 15 99.6% 100.0% 100.0% 99.5% 0.03 8.53 0.00 --
58260 2007:229:14:26:48.749 0 -320.7 -469.1 88 40 0 100.0% 100.0% 100.0% 100.0% 0.01 8.53 0.00 --
12462 2011:172:04:21:13.813 4 224.8 -144.5 59414 59307 72 99.9% 100.0% 100.0% 99.9% 0.03 8.53 0.00 --
16709 2015:054:21:16:09.927 5 -135.6 -237.9 19656 19588 13 100.0% 100.0% 100.0% 100.0% 0.03 8.52 0.00 --
19717 2017:053:07:35:12.614 4 -140.3 -236.2 12375 12139 11 99.3% 100.0% 100.0% 99.3% 0.04 8.52 0.00 --
19719 2017:175:22:22:17.264 5 238.3 -121.4 12375 12243 14 99.4% 100.0% 100.0% 99.4% 0.02 8.54 0.00 --
22213 2019:120:04:31:38.036 5 53.5 -260.7 14793 14572 20 98.8% 100.0% 100.0% 98.8% 0.04 8.55 0.00 --
22885 2019:307:08:41:24.751 5 -75.9 285.2 14876 14762 14 99.6% 100.0% 100.0% 99.6% 0.04 8.54 0.00 --
23436 2021:320:05:59:34.795 5 -85.5 282.4 12341 12219 7 99.7% 100.0% 100.0% 99.7% 0.07 8.57 0.00 --
24664 2021:321:18:20:13.949 5 -87.0 283.1 12340 12184 18 99.4% 100.0% 100.0% 99.4% 0.04 8.57 0.00 --
65521 2024:134:23:39:09.095 7 -52.5 -268.6 7790 7742 5 100.0% 100.0% 100.0% 100.0% 0.06 8.59 0.00 --
27061 2024:201:11:30:48.544 6 264.3 -79.6 7171 7111 6 100.0% 99.9% 100.0% 99.9% 0.07 8.63 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.