AGASC ID 1174293864

Info

Last Obs. 2023:198:02:48
magcatalog 7.48 ± 0.04
mag3 arcsec 7.47 ± 0.01
mag5 arcsec 7.47 ± 0.01
Nobs 30 (0 bad)
fok 99.9%
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
59535 2005:204:14:40:54.106 3 328.7 -391.5 1261 1260 0 99.9% 99.9% 99.9% 99.8% 0.02 7.48 0.00 --
7511 2007:255:10:56:30.400 5 -87.9 356.0 19911 19905 12 100.0% 100.0% 100.0% 100.0% 0.02 7.46 0.00 --
12328 2010:280:07:09:37.326 4 344.2 -303.7 82070 82045 62 100.0% 100.0% 100.0% 100.0% 0.02 7.47 0.00 --
12329 2010:288:12:34:32.086 4 286.9 -357.2 71816 71720 67 99.9% 100.0% 100.0% 99.9% 0.02 7.47 0.00 --
12330 2010:291:06:41:45.939 5 265.6 -373.0 42596 42580 38 100.0% 100.0% 100.0% 100.0% 0.02 7.47 0.00 --
13266 2011:308:08:09:47.879 4 114.7 -441.8 23818 23810 11 100.0% 100.0% 100.0% 100.0% 0.03 7.48 0.00 --
55080 2011:308:22:04:26.432 3 114.7 -441.8 47 47 1 100.0% 100.0% 100.0% 100.0% 0.01 7.48 0.00 --
50595 2016:302:10:14:59.763 3 -191.6 -199.4 90 90 0 100.0% 100.0% 100.0% 100.0% 0.01 7.45 0.00 --
21155 2019:272:17:34:32.137 5 371.2 -264.9 26424 26413 13 100.0% 100.0% 100.0% 100.0% 0.03 7.47 0.00 --
22861 2019:275:08:47:38.972 5 371.2 -264.9 34225 34206 24 99.9% 100.0% 100.0% 99.9% 0.02 7.47 0.00 --
22862 2019:278:12:24:27.668 5 371.4 -265.1 22010 21997 12 99.9% 100.0% 100.0% 99.9% 0.03 7.47 0.00 --
22422 2019:291:05:41:08.788 6 -105.8 -252.5 25941 25920 25 99.9% 100.0% 100.0% 99.9% 0.03 7.46 0.00 --
22877 2019:294:16:28:42.838 7 -113.4 -249.7 22023 22010 12 99.9% 100.0% 100.0% 99.9% 0.03 7.47 0.00 --
22883 2019:297:02:34:42.198 6 -113.4 -249.7 8837 8826 6 99.9% 100.0% 100.0% 99.9% 0.02 7.47 0.00 --
22884 2019:299:23:31:06.424 7 -114.6 -249.1 10169 10168 0 100.0% 100.0% 100.0% 100.0% 0.02 7.47 0.00 --
21156 2019:301:19:42:38.823 6 118.1 -440.2 10017 10013 7 100.0% 100.0% 100.0% 100.0% 0.03 7.47 0.00 --
22907 2019:303:01:37:08.347 5 119.7 -440.8 7418 7411 11 99.9% 100.0% 100.0% 99.9% 0.02 7.47 0.00 --
22908 2019:305:00:56:53.126 5 120.2 -441.0 10334 10329 8 100.0% 100.0% 100.0% 100.0% 0.03 7.47 0.00 --
22909 2019:305:16:47:19.271 5 120.8 -441.5 9830 9827 5 100.0% 100.0% 100.0% 100.0% 0.02 7.48 0.00 --
22910 2019:307:17:28:16.351 5 121.4 -441.7 7374 7370 4 100.0% 100.0% 100.0% 100.0% 0.02 7.48 0.00 --
22920 2019:325:14:19:54.395 6 -45.3 -457.6 22531 22506 21 99.9% 100.0% 100.0% 99.9% 0.03 7.46 0.00 --
23079 2019:326:21:57:48.808 5 -56.6 -456.8 6433 6418 3 99.8% 100.0% 100.0% 99.8% 0.02 7.46 0.00 --
23080 2019:328:15:37:18.751 5 -71.9 -454.9 10797 10795 4 100.0% 100.0% 100.0% 100.0% 0.03 7.46 0.00 --
26083 2022:301:03:53:10.091 5 202.2 292.1 5433 5433 2 100.0% 100.0% 100.0% 100.0% 0.01 7.47 0.00 --
27522 2022:330:18:14:32.045 5 322.1 130.5 2482 2480 3 99.9% 100.0% 100.0% 99.9% 0.02 7.47 0.00 --
27354 2023:037:09:22:59.661 4 211.0 -256.6 3907 3906 2 100.0% 100.0% 100.0% 100.0% 0.03 7.49 0.00 --
27704 2023:037:19:51:39.861 4 223.6 -246.0 2723 2720 1 99.9% 100.0% 100.0% 99.9% 0.03 7.49 0.00 --
27705 2023:041:23:42:05.055 4 192.1 -271.8 5650 5650 1 100.0% 100.0% 100.0% 100.0% 0.03 7.49 0.00 --
26512 2023:094:08:36:28.148 4 -96.4 -328.7 20523 20486 3 99.8% 100.0% 100.0% 99.8% 0.05 7.46 0.00 --
26007 2023:198:02:48:13.924 4 -290.1 224.4 10028 10027 5 100.0% 100.0% 100.0% 100.0% 0.03 7.48 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.