AGASC ID 196480344

Info

Last Obs. 2024:245:23:12
magcatalog 8.81 ± 0.02
mag3 arcsec 8.84 ± 0.02
mag5 arcsec 8.84 ± 0.02
Nobs 15 (0 bad)
fok 99.7%
f3 arcsec 99.9%
f5 arcsec 99.9%

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
10242 2009:127:08:38:18.665 7 475.5 362.3 9174 9119 10 99.9% 100.0% 100.0% 99.9% 0.02 8.82 0.00 --
10908 2009:130:01:25:39.170 7 475.5 362.3 13656 13587 18 99.9% 100.0% 100.0% 99.9% 0.02 8.82 0.00 --
13331 2012:121:15:05:27.375 3 19.0 171.0 879 821 0 100.0% 100.0% 100.0% 100.0% 0.02 8.83 0.00 --
21023 2018:144:20:59:45.489 3 358.0 -403.9 7468 7296 10 98.5% 100.0% 100.0% 98.5% 0.03 8.83 0.00 --
27230 2023:034:01:11:30.246 7 -294.7 -287.7 2523 2476 1 99.9% 100.0% 100.0% 99.9% 0.06 8.82 0.00 --
27692 2023:035:23:02:41.975 7 -290.6 -292.6 2524 2470 1 99.6% 100.0% 100.0% 99.6% 0.06 8.82 0.00 --
27691 2023:036:04:51:33.079 7 -229.6 -338.3 2527 2474 2 99.7% 100.0% 100.0% 99.7% 0.05 8.83 0.00 --
27228 2024:019:07:09:37.253 6 -331.6 -247.4 2610 2562 2 100.0% 100.0% 100.0% 100.0% 0.07 8.85 0.00 --
29202 2024:021:02:14:36.161 6 -336.1 -242.1 2520 2464 1 99.9% 100.0% 100.0% 99.9% 0.07 8.84 0.00 --
29203 2024:021:11:00:23.692 6 -339.4 -238.4 2517 2467 1 100.0% 100.0% 100.0% 100.0% 0.05 8.85 0.00 --
27226 2024:084:04:40:29.744 7 -149.1 -376.8 7415 7302 3 99.9% 99.5% 99.5% 99.3% 0.09 8.84 0.00 --
62617 2024:161:17:46:14.468 7 401.3 27.9 2541 2474 1 100.0% 99.6% 100.0% 99.6% 0.10 8.86 0.00 --
27229 2024:197:03:42:40.371 6 336.2 235.0 9600 9534 1 99.9% 99.9% 100.0% 99.9% 0.15 8.85 0.00 --
27231 2024:216:19:57:30.997 7 199.0 366.4 7411 7341 5 99.9% 100.0% 100.0% 99.9% 0.07 8.85 0.00 --
29430 2024:245:23:12:43.474 7 153.5 389.7 2669 2617 2 100.0% 100.0% 100.0% 100.0% 0.06 8.88 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.