AGASC ID 56923480

Info

Last Obs. 2024:254:05:31
magcatalog 6.80 ± 0.02
mag3 arcsec 6.80 ± 0.01
mag5 arcsec 6.80 ± 0.01
Nobs 12 (0 bad)
fok 100.0%
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
4482 2004:201:22:45:13.498 5 -247.0 308.2 38569 38505 21 100.0% 100.0% 100.0% 100.0% 0.01 6.80 0.00 --
56164 2010:177:03:36:22.210 3 -74.2 370.3 2227 2182 0 100.0% 100.0% 100.0% 99.9% 0.02 6.79 0.00 --
22663 2020:041:00:23:08.553 5 317.5 -172.6 2586 2512 4 100.0% 100.0% 100.0% 100.0% 0.01 6.80 0.00 --
22664 2020:175:18:57:56.595 5 -10.0 385.3 2586 2508 0 100.0% 100.0% 100.0% 100.0% 0.01 6.80 0.00 --
25088 2021:195:05:05:51.902 6 171.3 108.3 5032 4945 2 100.0% 100.0% 100.0% 100.0% 0.02 6.80 0.00 --
22666 2021:218:23:58:56.628 5 -316.7 221.1 2582 2496 1 100.0% 100.0% 100.0% 100.0% 0.02 6.81 0.00 --
22665 2021:278:06:40:58.129 5 -377.8 38.7 2586 2509 1 100.0% 100.0% 100.0% 100.0% 0.02 6.82 0.00 --
22668 2023:115:21:20:07.469 4 365.3 16.0 1599 1537 0 100.0% 100.0% 100.0% 100.0% 0.01 6.79 0.00 --
22667 2023:160:19:04:28.225 4 217.0 310.2 1317 1254 0 100.0% 100.0% 100.0% 100.0% 0.01 6.79 0.00 --
27828 2023:260:00:37:48.505 4 -365.0 117.2 1321 1268 1 100.0% 100.0% 100.0% 100.0% 0.01 6.82 0.00 --
26968 2024:092:15:07:45.681 4 363.4 -15.1 1312 1254 0 100.0% 100.0% 100.0% 100.0% 0.02 6.83 0.00 --
26969 2024:254:05:31:46.900 4 -365.7 106.9 1565 1509 0 100.0% 100.0% 100.0% 100.0% 0.02 6.84 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.