AGASC ID 1201019200

Info

Last Obs. 2024:176:20:41
magcatalog 9.55 ± 0.10
mag3 arcsec 9.46 ± 0.03
mag5 arcsec 9.46 ± 0.03
Nobs 53 (0 bad)
fok 99.0%
f3 arcsec 99.8%
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
2783 2002:302:18:27:57.789 5 -177.4 250.7 10168 10011 10 99.0% 100.0% 100.0% 99.0% 0.03 9.41 0.00 --
4614 2004:002:16:17:17.989 5 15.3 383.1 23174 23093 23 99.9% 100.0% 100.0% 99.9% 0.04 9.45 0.00 --
4640 2004:239:05:18:58.398 4 -346.8 -163.1 29033 28473 38 98.3% 100.0% 100.0% 98.3% 0.03 9.43 0.00 --
60080 2004:239:22:30:16.589 4 -296.5 -203.5 90 48 0 100.0% 100.0% 100.0% 100.0% 0.01 9.45 0.00 --
5362 2004:240:16:07:46.412 4 -346.8 -163.1 34301 34150 38 99.7% 100.0% 100.0% 99.7% 0.03 9.44 0.00 --
4641 2004:243:08:06:19.539 4 -346.8 -163.1 37007 36505 35 98.8% 100.0% 100.0% 98.8% 0.03 9.43 0.00 --
6099 2004:245:22:54:10.765 4 -346.8 -163.1 24767 24608 30 99.6% 100.0% 100.0% 99.6% 0.03 9.43 0.00 --
5363 2004:249:00:04:52.154 4 -346.8 -163.1 22241 21736 20 98.1% 100.0% 100.0% 98.0% 0.04 9.43 0.00 --
7590 2007:107:04:18:38.557 5 342.5 -98.0 17708 17621 23 99.8% 100.0% 100.0% 99.8% 0.05 9.46 0.00 --
9851 2008:119:03:22:57.090 5 297.2 -187.8 6488 6403 13 99.8% 100.0% 100.0% 99.8% 0.02 9.48 0.00 --
9085 2008:120:07:51:18.149 5 297.2 -187.8 16727 16652 31 99.9% 100.0% 100.0% 99.8% 0.03 9.48 0.00 --
10852 2009:012:12:12:02.380 4 104.3 363.0 5512 5452 4 99.9% 100.0% 100.0% 99.9% 0.03 9.46 0.00 --
10221 2009:013:10:18:40.767 4 104.3 363.0 9548 9419 14 99.2% 100.0% 100.0% 99.2% 0.03 9.45 0.00 --
10853 2009:015:07:19:40.101 4 104.3 363.0 5769 5646 6 98.9% 100.0% 100.0% 98.9% 0.03 9.46 0.00 --
10854 2009:017:03:05:33.752 4 104.3 363.0 6131 6013 15 98.9% 100.0% 100.0% 98.9% 0.03 9.46 0.00 --
10855 2009:018:16:58:53.130 4 104.3 363.0 9562 9479 18 99.7% 100.0% 100.0% 99.7% 0.04 9.46 0.00 --
10926 2009:251:09:32:06.296 3 -346.9 -128.5 17488 17243 32 99.0% 100.0% 100.0% 98.9% 0.02 9.44 0.00 --
56391 2010:076:06:02:14.263 2 356.1 61.0 146 27 0 100.0% 100.0% 100.0% 100.0% 0.01 9.47 0.00 --
11826 2010:230:03:26:11.557 6 -247.9 -261.8 16981 16540 38 97.7% 100.0% 100.0% 97.7% 0.06 9.44 0.00 --
55611 2011:065:14:54:44.031 2 347.9 109.7 90 45 0 97.8% 100.0% 100.0% 97.8% 0.02 9.44 0.00 --
52779 2014:133:05:08:37.483 4 14.9 -248.5 97 41 0 80.4% 100.0% 100.0% 80.4% 0.01 9.49 0.00 --
52774 2014:135:21:27:33.949 4 14.9 -248.5 86 48 0 100.0% 100.0% 100.0% 100.0% 0.01 9.48 0.00 --
52741 2014:151:18:19:55.511 3 -31.0 -248.1 88 45 1 100.0% 100.0% 100.0% 100.0% 0.01 9.43 0.00 --
52676 2014:178:04:07:04.678 4 -164.9 -195.5 104 62 0 100.0% 100.0% 100.0% 100.0% 0.01 9.45 0.00 --
52240 2014:355:09:06:14.067 4 154.6 221.5 94 47 0 100.0% 100.0% 100.0% 100.0% 0.02 9.44 0.00 --
51998 2015:085:13:17:22.055 5 208.2 -139.3 88 48 0 98.0% 100.0% 100.0% 98.0% 0.01 9.49 0.00 --
51988 2015:090:21:00:52.192 5 208.2 -139.3 92 47 0 100.0% 100.0% 100.0% 100.0% 0.02 9.49 0.00 --
51843 2015:159:15:14:58.936 7 -92.4 -234.6 98 42 0 93.3% 100.0% 100.0% 93.3% 0.01 9.42 0.00 --
51320 2016:022:01:23:19.548 4 227.2 130.9 104 59 0 100.0% 100.0% 100.0% 100.0% 0.01 9.45 0.00 --
50688 2016:267:23:55:18.419 2 -371.7 -63.8 226 82 0 100.0% 100.0% 100.0% 100.0% 0.01 9.45 0.00 --
17904 2017:123:14:21:00.211 5 171.6 -208.8 20094 19969 27 99.6% 100.0% 100.0% 99.6% 0.06 9.48 0.00 --
50107 2017:124:02:14:37.798 3 169.9 -208.1 229 90 1 97.8% 100.0% 100.0% 97.8% 0.03 9.46 0.00 --
19925 2017:132:16:55:27.238 5 198.7 -183.5 20496 19729 29 97.0% 100.0% 100.0% 97.0% 0.09 9.49 0.00 --
23163 2020:051:14:29:32.725 7 248.8 35.0 19179 18629 25 97.5% 100.0% 100.0% 97.4% 0.08 9.44 0.00 --
23198 2020:088:12:38:04.723 4 356.5 64.9 23567 23267 19 99.0% 100.0% 100.0% 99.0% 0.15 9.46 0.00 --
23534 2021:298:20:16:23.403 4 -345.1 156.4 13807 13480 21 98.1% 99.8% 99.9% 97.9% 0.11 9.46 0.00 --
24295 2021:300:15:22:55.780 4 -340.3 166.9 14780 14303 12 97.1% 99.8% 100.0% 96.9% 0.12 9.47 0.00 --
25514 2022:264:03:11:27.974 7 -371.6 -59.2 28922 28581 16 99.1% 100.0% 100.0% 99.0% 0.20 9.49 0.00 --
25511 2023:103:19:12:20.573 6 348.1 -82.2 3662 3543 2 98.5% 94.8% 100.0% 93.4% 0.12 9.48 0.00 --
27495 2023:110:18:54:26.559 6 333.5 -123.3 3806 3716 2 99.1% 95.5% 100.0% 94.7% 0.12 9.51 0.00 --
27807 2023:111:15:22:40.725 6 328.8 -127.0 3782 3652 2 98.0% 99.8% 100.0% 97.8% 0.09 9.51 0.00 --
28874 2023:244:03:27:46.987 7 -325.0 -173.4 2748 2697 1 100.0% 99.9% 100.0% 99.9% 0.16 9.51 0.00 --
27487 2023:270:13:39:58.046 7 -373.8 -17.6 3761 3701 2 100.0% 99.9% 100.0% 99.9% 0.13 9.52 0.00 --
28961 2023:284:19:42:20.970 6 -366.8 100.6 3849 3790 4 99.9% 100.0% 100.0% 99.9% 0.10 9.48 0.00 --
28980 2023:292:15:23:19.239 5 -388.7 278.5 3745 3696 5 99.8% 100.0% 100.0% 99.8% 0.07 9.47 0.00 --
28981 2023:293:00:13:59.677 5 -409.4 243.6 3745 3686 0 99.9% 99.8% 100.0% 99.7% 0.06 9.48 0.00 --
25513 2024:074:05:36:20.948 6 349.0 104.1 3461 3394 1 100.0% 98.9% 100.0% 98.8% 0.18 9.45 0.00 --
29324 2024:074:17:57:58.012 6 352.3 89.2 3380 3307 4 99.9% 99.1% 100.0% 99.0% 0.09 9.45 0.00 --
28756 2024:080:22:06:32.139 6 345.2 114.4 3679 3615 1 100.0% 97.6% 100.0% 97.6% 0.17 9.48 0.00 --
29215 2024:100:18:14:56.305 6 481.0 187.6 3760 3687 4 100.0% 98.9% 100.0% 98.9% 0.16 9.50 0.00 --
27070 2024:101:02:21:43.745 7 402.8 384.1 3368 3292 0 99.9% 99.2% 100.0% 99.1% 0.11 9.47 0.00 --
29367 2024:103:05:21:20.603 7 416.6 368.7 3836 3675 1 99.8% 99.6% 99.9% 99.4% 0.12 9.47 0.00 --
26553 2024:176:20:41:42.573 6 300.8 -401.7 10341 10267 2 99.9% 99.3% 100.0% 99.2% 0.20 9.54 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.