AGASC ID 972689192

Info

Last Obs. 2025:211:01:35
magcatalog 8.90 ± 0.02
mag3 arcsec 8.92 ± 0.02
mag5 arcsec 8.92 ± 0.02
Nobs 14 (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
4356 2003:124:09:19:47.319 3 -440.6 69.1 286 213 0 100.0% 100.0% 100.0% 100.0% 0.01 8.93 0.00 --
60691 2003:166:10:40:35.769 0 -277.9 462.7 5159 5110 10 99.9% 99.9% 100.0% 99.8% 0.03 8.91 0.00 --
3499 2003:177:12:36:59.541 7 479.8 219.5 18690 18591 27 99.9% 100.0% 100.0% 99.9% 0.02 8.91 0.00 --
4475 2004:169:23:03:47.111 3 367.1 363.9 9899 9844 5 100.0% 100.0% 100.0% 100.0% 0.02 8.91 0.00 --
5402 2005:220:02:13:59.489 6 106.3 -475.7 7591 7451 13 99.1% 100.0% 100.0% 99.1% 0.02 8.94 0.00 --
5403 2005:221:02:14:53.388 6 100.0 -477.1 7464 7389 8 99.9% 100.0% 100.0% 99.9% 0.02 8.93 0.00 --
5404 2005:222:01:47:47.206 6 95.1 -478.2 7468 7398 11 99.9% 100.0% 100.0% 99.9% 0.02 8.93 0.00 --
5405 2005:224:02:57:26.834 6 83.9 -480.4 7459 7397 10 99.9% 100.0% 100.0% 99.9% 0.04 8.93 0.00 --
5406 2005:225:01:36:55.539 6 79.3 -481.2 7467 7401 6 99.9% 100.0% 100.0% 99.9% 0.03 8.93 0.00 --
13619 2012:232:13:16:56.274 4 51.3 292.0 5810 5656 4 98.3% 100.0% 100.0% 98.3% 0.04 8.91 0.00 --
26006 2023:194:14:23:17.037 7 280.5 -444.8 4006 3935 3 99.9% 100.0% 100.0% 99.9% 0.08 8.91 0.00 --
27947 2023:195:13:06:30.984 5 265.0 -454.8 4257 4186 7 99.9% 99.9% 100.0% 99.8% 0.07 8.91 0.00 --
27948 2023:196:15:26:51.453 7 272.5 -449.7 4109 4036 4 100.0% 100.0% 100.0% 99.9% 0.06 8.92 0.00 --
28764 2025:211:01:35:03.642 7 185.6 -469.0 4893 4842 1 100.0% 99.4% 100.0% 99.4% 0.14 8.97 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.