AGASC ID 440150048

Info

Last Obs. 2025:078:22:53
magcatalog 7.10 ± 0.02
mag3 arcsec 7.11 ± 0.03
mag5 arcsec 7.11 ± 0.03
Nobs 74 (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
2583 2002:119:17:37:19.697 3 270.7 127.7 13937 13876 15 100.0% 100.0% 100.0% 100.0% 0.01 7.16 0.00 --
3479 2002:279:09:50:08.954 4 -328.1 -17.5 14970 14876 5 100.0% 100.0% 100.0% 100.0% 0.01 7.11 0.00 --
5040 2004:254:22:08:42.782 6 -315.4 32.5 14378 14304 9 100.0% 100.0% 100.0% 100.0% 0.01 7.15 0.00 --
5041 2004:255:06:44:43.564 6 -347.8 32.6 14286 14237 9 100.0% 100.0% 100.0% 100.0% 0.01 7.15 0.00 --
5955 2005:087:13:02:04.973 5 290.7 42.8 14290 14214 10 100.0% 100.0% 100.0% 99.9% 0.01 7.15 0.00 --
5956 2005:090:07:55:50.456 4 294.1 48.9 14786 14718 15 100.0% 100.0% 100.0% 100.0% 0.01 7.13 0.00 --
6540 2005:340:15:38:55.565 5 -108.5 -270.1 2585 2531 1 100.0% 100.0% 100.0% 100.0% 0.01 7.10 0.00 --
6543 2005:340:17:49:22.089 6 -107.5 -270.4 2584 2534 3 100.0% 100.0% 100.0% 100.0% 0.01 7.10 0.00 --
6544 2005:340:19:21:12.089 6 -106.7 -270.7 2584 2530 1 100.0% 100.0% 100.0% 100.0% 0.01 7.10 0.00 --
6541 2005:341:20:45:01.348 6 -94.0 -274.7 2582 2532 1 100.0% 100.0% 100.0% 100.0% 0.01 7.10 0.00 --
6542 2005:341:22:36:29.184 5 -93.0 -275.0 2569 2517 3 100.0% 100.0% 100.0% 100.0% 0.01 7.10 0.00 --
6545 2005:353:21:49:11.712 4 98.3 -267.9 2583 2531 0 100.0% 100.0% 100.0% 100.0% 0.01 7.09 0.00 --
6546 2005:354:00:00:27.855 5 69.2 -277.2 2582 2533 0 100.0% 100.0% 100.0% 100.0% 0.01 7.09 0.00 --
6553 2005:354:01:36:31.441 6 70.1 -276.9 2583 2531 3 100.0% 100.0% 100.0% 100.0% 0.01 7.09 0.00 --
6547 2005:356:23:09:18.468 5 104.6 -265.5 2583 2532 1 100.0% 100.0% 100.0% 100.0% 0.01 7.09 0.00 --
6548 2005:357:00:57:03.102 5 105.5 -265.1 2590 2523 4 99.6% 100.0% 100.0% 99.6% 0.01 7.09 0.00 --
6554 2005:357:02:28:53.102 5 106.2 -264.9 2586 2532 2 100.0% 100.0% 100.0% 100.0% 0.01 7.09 0.00 --
6549 2005:359:04:53:45.157 3 128.6 -254.7 2584 2531 1 100.0% 100.0% 100.0% 100.0% 0.01 7.09 0.00 --
6550 2005:359:07:01:42.043 5 129.5 -254.2 2583 2533 3 99.9% 100.0% 100.0% 99.9% 0.01 7.09 0.00 --
6551 2005:359:08:33:32.043 5 130.2 -253.9 2584 2533 1 100.0% 100.0% 100.0% 100.0% 0.01 7.09 0.00 --
6552 2005:359:10:05:22.043 5 130.8 -253.6 2584 2535 2 100.0% 100.0% 100.0% 100.0% 0.01 7.09 0.00 --
6555 2006:010:09:27:16.904 5 234.1 -166.7 2586 2528 3 100.0% 100.0% 100.0% 100.0% 0.01 7.08 0.00 --
6556 2006:010:11:26:24.905 5 234.4 -166.3 2584 2533 1 100.0% 100.0% 100.0% 100.0% 0.01 7.08 0.00 --
6557 2006:010:12:58:14.905 5 234.6 -166.0 2583 2530 1 100.0% 100.0% 100.0% 100.0% 0.01 7.08 0.00 --
6558 2006:010:14:30:04.905 5 234.9 -165.7 2584 2532 1 100.0% 100.0% 100.0% 100.0% 0.01 7.08 0.00 --
6559 2006:010:16:01:54.905 5 235.1 -165.4 2584 2532 1 100.0% 100.0% 100.0% 100.0% 0.01 7.08 0.00 --
6472 2006:113:23:17:29.976 6 263.2 109.0 14784 14721 11 100.0% 100.0% 100.0% 100.0% 0.01 7.12 0.00 --
8345 2007:017:07:28:09.736 6 254.2 -136.5 2586 2528 2 100.0% 100.0% 100.0% 100.0% 0.01 7.09 0.00 --
8346 2007:017:09:22:23.309 6 254.4 -136.2 2585 2530 4 100.0% 100.0% 100.0% 100.0% 0.01 7.09 0.00 --
8347 2007:017:10:54:13.309 6 254.6 -135.9 2585 2531 2 100.0% 100.0% 100.0% 100.0% 0.01 7.09 0.00 --
8348 2007:017:12:26:03.309 6 254.8 -135.6 2584 2531 1 100.0% 100.0% 100.0% 100.0% 0.01 7.09 0.00 --
8349 2007:017:13:57:53.309 6 254.9 -135.3 2586 2530 1 100.0% 100.0% 100.0% 100.0% 0.01 7.09 0.00 --
8350 2007:017:15:29:43.309 6 255.1 -135.0 2585 2531 2 100.0% 100.0% 100.0% 100.0% 0.01 7.09 0.00 --
8351 2007:017:17:01:33.309 6 255.3 -134.7 2585 2528 4 99.9% 100.0% 100.0% 99.9% 0.01 7.09 0.00 --
8352 2007:017:18:33:23.309 6 255.4 -134.4 2586 2529 2 100.0% 100.0% 100.0% 100.0% 0.01 7.09 0.00 --
8353 2007:017:20:05:13.309 4 255.6 -134.1 2584 2529 1 100.0% 100.0% 100.0% 100.0% 0.01 7.08 0.00 --
8354 2007:017:21:37:03.309 4 255.8 -133.8 2584 2530 0 100.0% 100.0% 100.0% 100.0% 0.01 7.08 0.00 --
8355 2007:017:23:08:53.309 4 255.9 -133.5 2583 2531 1 100.0% 100.0% 100.0% 100.0% 0.01 7.08 0.00 --
8356 2007:020:18:53:07.170 6 262.1 -122.2 2584 2528 1 100.0% 100.0% 100.0% 100.0% 0.01 7.10 0.00 --
8357 2007:020:21:08:04.756 7 262.3 -121.8 2583 2532 4 100.0% 100.0% 100.0% 100.0% 0.01 7.10 0.00 --
8358 2007:020:22:39:54.756 7 262.4 -121.5 2586 2530 0 100.0% 100.0% 100.0% 100.0% 0.01 7.10 0.00 --
8359 2007:021:16:11:50.263 6 263.8 -118.8 2583 2530 3 100.0% 100.0% 100.0% 100.0% 0.01 7.09 0.00 --
8360 2007:021:18:12:30.342 6 263.9 -118.5 3169 3113 4 99.9% 100.0% 100.0% 99.9% 0.01 7.09 0.00 --
8319 2007:105:04:09:02.443 7 270.3 83.2 29418 29343 26 100.0% 100.0% 100.0% 100.0% 0.02 7.06 0.00 --
10600 2009:112:04:18:58.381 6 301.0 103.9 14677 14594 6 100.0% 100.0% 100.0% 100.0% 0.01 7.12 0.00 --
11931 2009:322:21:07:56.894 3 -251.6 -173.5 14935 14857 6 100.0% 100.0% 100.0% 100.0% 0.01 7.11 0.00 --
11932 2009:323:20:00:07.666 3 -243.5 -175.6 14999 14943 10 100.0% 100.0% 100.0% 100.0% 0.02 7.10 0.00 --
13090 2010:333:14:30:26.317 5 -175.6 -230.9 14779 14723 7 100.0% 100.0% 100.0% 100.0% 0.02 7.12 0.00 --
13089 2010:335:01:31:06.008 5 -176.1 -242.3 15107 15054 4 100.0% 100.0% 100.0% 100.0% 0.02 7.12 0.00 --
55833 2010:335:10:22:01.859 4 -176.1 -242.3 91 47 0 100.0% 100.0% 100.0% 100.0% 0.00 7.12 0.00 --
55824 2010:338:07:36:07.932 4 -40.8 -297.3 340 287 0 99.7% 100.0% 100.0% 99.7% 0.01 7.11 0.00 --
14240 2011:360:11:51:19.879 5 134.4 -252.0 14780 14723 9 100.0% 100.0% 100.0% 100.0% 0.01 7.13 0.00 --
14239 2011:363:14:36:35.158 4 156.6 -238.1 14780 14713 7 100.0% 100.0% 100.0% 100.0% 0.01 7.15 0.00 --
16418 2013:357:09:58:49.534 5 107.2 -267.9 14946 14891 9 100.0% 100.0% 100.0% 100.0% 0.01 7.15 0.00 --
17324 2014:335:03:12:54.700 5 -171.0 -244.7 14393 14221 3 99.2% 100.0% 100.0% 99.2% 0.02 7.16 0.00 --
18357 2016:208:12:26:23.895 4 -288.0 140.0 7547 7468 6 100.0% 100.0% 100.0% 100.0% 0.01 7.06 0.00 --
18358 2016:208:17:18:31.870 6 -306.5 139.2 5360 5310 2 100.0% 100.0% 100.0% 100.0% 0.01 7.06 0.00 --
18359 2016:208:20:29:25.470 6 -285.7 141.8 5018 4970 4 100.0% 100.0% 100.0% 100.0% 0.01 7.06 0.00 --
18360 2016:208:23:27:34.388 6 -306.9 138.3 5189 5140 2 100.0% 100.0% 100.0% 100.0% 0.01 7.06 0.00 --
18361 2016:209:02:32:52.388 5 -286.1 140.9 5021 4968 0 100.0% 100.0% 100.0% 100.0% 0.01 7.06 0.00 --
18364 2016:209:05:31:01.305 5 -289.1 137.5 7953 7905 5 100.0% 100.0% 100.0% 100.0% 0.01 7.06 0.00 --
18362 2016:254:00:49:40.950 5 -332.0 27.7 5018 4965 4 100.0% 100.0% 100.0% 100.0% 0.01 7.06 0.00 --
18363 2016:254:04:06:12.185 6 -314.5 31.2 5019 4969 1 100.0% 100.0% 100.0% 100.0% 0.01 7.06 0.00 --
19837 2016:362:05:50:09.747 5 107.7 -270.8 9659 9597 6 100.0% 100.0% 100.0% 100.0% 0.02 7.14 0.00 --
21786 2018:336:22:48:46.057 4 -140.6 -261.5 8925 8851 5 100.0% 100.0% 100.0% 100.0% 0.02 7.10 0.00 --
22003 2018:339:06:10:37.028 4 -140.6 -261.5 6072 5999 5 100.0% 100.0% 100.0% 100.0% 0.02 7.10 0.00 --
24839 2020:315:03:33:46.097 4 -274.4 -133.6 9899 9841 9 100.0% 100.0% 100.0% 100.0% 0.02 7.10 0.00 --
25616 2021:348:19:22:12.450 3 -4.6 -291.7 13802 13739 7 100.0% 100.0% 100.0% 100.0% 0.02 7.10 0.00 --
26463 2022:213:17:56:45.819 4 -289.2 119.3 4678 4589 6 99.9% 100.0% 100.0% 99.9% 0.02 7.18 0.00 --
29538 2025:049:02:18:49.115 4 293.3 -42.2 3842 3774 2 100.0% 100.0% 100.0% 100.0% 0.02 7.12 0.00 --
30806 2025:049:16:39:30.728 4 295.4 -46.3 3638 3574 0 100.0% 100.0% 100.0% 100.0% 0.02 7.12 0.00 --
29539 2025:076:02:17:39.711 4 300.3 8.6 2540 2478 0 100.0% 100.0% 100.0% 100.0% 0.02 7.14 0.00 --
30856 2025:078:01:03:28.797 4 298.1 4.3 2705 2639 0 100.0% 100.0% 100.0% 100.0% 0.05 7.14 0.00 --
30857 2025:078:22:53:47.870 4 299.4 3.7 2944 2878 0 100.0% 100.0% 100.0% 100.0% 0.06 7.15 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.