AGASC ID 688397848

Info

Last Obs. 2024:325:04:10
magcatalog 8.59 ± 0.02
mag3 arcsec 8.60 ± 0.02
mag5 arcsec 8.60 ± 0.02
Nobs 14 (0 bad)
fok 99.5%
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
61023 2002:266:18:31:42.714 2 -472.8 290.4 4839 4771 8 99.9% 99.9% 100.0% 99.8% 0.02 8.62 0.00 --
5786 2005:290:09:07:38.328 6 -290.7 -163.5 14778 14709 19 99.9% 100.0% 100.0% 99.9% 0.01 8.60 0.00 --
55958 2010:290:10:26:13.639 6 -55.3 -152.8 2292 2250 1 100.0% 100.0% 100.0% 100.0% 0.03 8.58 0.00 --
17490 2015:020:06:49:45.047 6 -270.0 -183.8 59118 58633 52 99.3% 100.0% 100.0% 99.3% 0.03 8.58 0.00 --
17170 2015:309:19:43:45.952 7 -308.6 -164.7 12703 12577 10 99.5% 100.0% 100.0% 99.5% 0.03 8.59 0.00 --
18702 2015:319:08:05:47.906 7 -308.6 -164.7 12335 12174 12 99.3% 100.0% 100.0% 99.3% 0.04 8.59 0.00 --
18703 2016:014:17:24:11.650 7 -299.9 -181.9 13171 13018 23 99.4% 100.0% 100.0% 99.3% 0.02 8.58 0.00 --
19559 2017:173:02:45:04.514 7 -312.9 -423.2 1847 1751 1 98.8% 100.0% 100.0% 98.8% 0.02 8.57 0.00 --
49455 2018:026:17:28:53.802 5 -427.4 -18.6 1826 1776 0 99.7% 100.0% 100.0% 99.7% 0.02 8.60 0.00 --
25361 2022:127:17:13:35.971 5 -309.4 499.4 2091 1984 6 98.1% 100.0% 100.0% 98.1% 0.03 8.61 0.00 --
43165 2024:254:23:35:46.707 3 -29.7 127.4 823 773 1 100.0% 99.4% 100.0% 99.4% 0.07 8.63 0.00 --
28673 2024:266:00:50:29.062 5 -283.7 457.5 3254 3200 0 99.9% 100.0% 100.0% 99.9% 0.04 8.64 0.00 --
30080 2024:266:21:08:18.573 5 -324.9 429.5 4229 4182 4 100.0% 100.0% 100.0% 100.0% 0.04 8.64 0.00 --
28303 2024:325:04:10:36.012 4 -476.2 252.5 10326 10279 1 99.9% 100.0% 100.0% 99.9% 0.09 8.66 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.