AGASC ID 196482032

Info

Last Obs. 2024:216:19:57
magcatalog 8.23 ± 0.02
mag3 arcsec 8.26 ± 0.02
mag5 arcsec 8.26 ± 0.02
Nobs 13 (0 bad)
fok 99.8%
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
21023 2018:144:20:59:45.489 5 308.5 55.2 7465 7377 8 99.6% 100.0% 100.0% 99.6% 0.02 8.24 0.00 --
27230 2023:034:01:11:30.246 5 141.9 -435.7 2538 2446 4 98.6% 100.0% 100.0% 98.6% 0.04 8.26 0.00 --
27692 2023:035:23:02:41.975 5 149.1 -431.2 2537 2448 4 98.7% 100.0% 100.0% 98.7% 0.04 8.26 0.00 --
27691 2023:036:04:51:33.079 5 228.0 -393.9 2539 2469 2 99.5% 100.0% 100.0% 99.5% 0.04 8.27 0.00 --
27228 2024:019:07:09:37.253 4 81.2 -452.7 2622 2560 1 99.9% 100.0% 100.0% 99.9% 0.03 8.26 0.00 --
29202 2024:021:02:14:36.161 4 73.4 -453.9 2534 2465 1 99.9% 100.0% 100.0% 99.9% 0.05 8.26 0.00 --
29203 2024:021:11:00:23.692 4 67.9 -454.4 2530 2466 1 99.9% 100.0% 100.0% 99.9% 0.03 8.27 0.00 --
27226 2024:084:04:40:29.744 5 310.1 -336.1 7424 7300 7 99.9% 99.8% 99.9% 99.7% 0.04 8.28 0.00 --
27227 2024:094:22:17:54.985 6 393.0 -234.0 7406 7359 1 100.0% 100.0% 100.0% 100.0% 0.04 8.27 0.00 --
62617 2024:161:09:59:16.167 6 249.2 407.0 2536 2470 1 100.0% 100.0% 100.0% 100.0% 0.04 8.28 0.00 --
62617 2024:161:17:46:14.468 5 192.6 438.9 2536 2473 1 100.0% 100.0% 100.0% 100.0% 0.03 8.27 0.00 --
62617 2024:161:17:46:14.468 5 192.6 438.9 2536 2473 0 100.0% 100.0% 100.0% 100.0% 0.05 8.28 0.00 --
62617 2024:161:17:46:14.468 5 192.6 438.9 2536 2473 0 100.0% 100.0% 100.0% 100.0% 0.05 8.28 0.00 --
27229 2024:197:03:42:40.371 5 -52.8 482.5 9576 9534 0 99.9% 100.0% 100.0% 99.9% 0.10 8.27 0.00 --
27231 2024:216:19:57:30.997 5 -259.8 414.5 7400 7346 1 100.0% 100.0% 100.0% 100.0% 0.04 8.27 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.