AGASC ID 44965328

Info

Last Obs. 2024:157:13:17
magcatalog 10.28 ± 0.14
mag3 arcsec 10.31 ± 0.07
mag5 arcsec 10.32 ± 0.07
Nobs 15 (0 bad)
fok 96.7%
f3 arcsec 96.8%
f5 arcsec 99.8%

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
4047 2003:138:11:06:05.553 6 412.4 169.7 1224 1159 51 100.0% 100.0% 100.0% 100.0% 0.09 10.16 0.00 --
60673 2003:182:08:03:13.097 0 -367.5 440.0 5187 5098 23 99.6% 99.5% 99.7% 99.1% 0.05 10.21 0.00 --
10437 2009:091:14:01:38.107 5 352.6 -412.1 2589 2521 8 99.7% 99.9% 100.0% 99.6% 0.05 10.31 0.00 --
25457 2022:130:12:49:13.001 6 432.2 29.7 10147 9580 25 94.9% 98.7% 99.8% 93.6% 0.11 10.30 0.00 --
45497 2022:131:09:36:37.980 7 -58.2 -203.3 335 252 1 97.3% 99.2% 100.0% 96.5% 0.05 10.32 0.00 --
26417 2022:131:10:31:29.781 6 431.9 29.8 9914 9363 17 95.0% 99.8% 99.9% 94.8% 0.13 10.26 0.00 --
25863 2022:135:05:35:23.422 6 430.0 60.5 7952 6996 9 88.6% 98.1% 100.0% 86.9% 0.19 10.35 0.00 --
27213 2024:108:19:16:47.268 6 274.4 -445.0 3454 3394 1 99.9% 81.2% 100.0% 81.1% 0.35 10.38 0.00 --
29376 2024:111:03:12:35.496 6 305.8 -424.4 3509 3435 0 99.4% 84.5% 98.4% 84.0% 0.53 10.37 0.00 --
27211 2024:139:09:39:42.606 7 437.1 317.8 4013 3933 5 99.5% 97.2% 100.0% 96.8% 0.30 10.36 0.00 --
29409 2024:139:19:45:10.411 7 440.0 313.8 3450 3319 9 99.7% 97.1% 99.3% 96.8% 0.26 10.35 0.00 --
27214 2024:142:20:37:14.180 7 437.1 317.8 4361 4301 3 99.8% 96.1% 100.0% 95.9% 0.31 10.36 0.00 --
29418 2024:143:08:12:51.300 7 437.7 317.5 2554 2509 1 99.9% 94.9% 100.0% 94.8% 0.29 10.33 0.00 --
26945 2024:155:23:34:32.751 7 441.0 310.6 4978 4906 3 99.9% 98.8% 100.0% 98.7% 0.25 10.33 0.00 --
29439 2024:157:13:17:04.699 7 440.6 310.8 2864 2797 2 100.0% 99.4% 100.0% 99.4% 0.21 10.36 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.