AGASC ID 374352808

Info

Last Obs. 2025:334:15:19
magcatalog 8.74 ± 0.02
mag3 arcsec 8.77 ± 0.02
mag5 arcsec 8.77 ± 0.02
Nobs 54 (3 bad)
fok 99.6%
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 mag ⟩ 100s ⟨ mag ⟩ σmag Comments
6139 2004:278:22:26:47.131 4 -403.8 -286.7 28087 28005 34 99.9% 100.0% 100.0% 99.9% 0.02 8.77 0.00 --
4946 2004:280:20:51:25.224 4 -397.1 -295.5 11767 11687 17 99.9% 100.0% 100.0% 99.9% 0.02 8.77 0.00 --
4948 2004:283:10:37:27.995 6 -385.2 -307.6 58677 58588 55 99.9% 100.0% 100.0% 99.9% 0.04 8.77 0.00 --
4949 2004:286:01:38:30.183 5 -374.1 -320.5 14773 14713 20 99.9% 100.0% 100.0% 99.9% 0.02 8.82 0.00 --
4950 2004:286:10:07:00.183 5 -370.5 -322.2 48345 48271 6 99.9% 100.0% 100.0% 99.9% 0.08 8.78 0.00 --
4952 2004:288:06:04:50.619 5 -359.4 -332.0 81230 81124 107 99.9% 100.0% 100.0% 99.9% 0.03 8.77 0.00 --
4951 2004:291:06:55:22.648 5 -345.4 -348.1 47559 47477 51 99.9% 100.0% 100.0% 99.9% 0.02 8.75 0.00 --
4953 2004:292:10:25:39.158 5 -336.8 -354.3 15132 15065 17 100.0% 100.0% 100.0% 100.0% 0.03 8.76 0.00 --
6146 2004:294:22:35:54.690 6 -324.7 -368.7 23548 23473 29 99.9% 100.0% 100.0% 99.9% 0.01 8.76 0.00 --
11716 2009:283:11:56:45.729 4 -436.8 -363.1 19650 19575 32 99.9% 100.0% 100.0% 99.9% 0.02 8.75 0.00 --
11715 2009:336:21:32:37.147 5 443.9 -340.0 36756 36653 71 99.9% 100.0% 100.0% 99.9% 0.02 8.76 0.00 --
12037 2009:339:17:51:13.756 7 443.9 -340.0 41920 41795 55 99.9% 100.0% 100.0% 99.9% 0.02 8.75 0.00 --
56615 2009:340:18:13:28.115 3 443.9 -340.0 151 28 0 100.0% 100.0% 100.0% 100.0% 0.01 8.76 0.00 --
11714 2009:341:18:07:00.005 5 386.4 -235.2 45527 45429 83 99.9% 100.0% 100.0% 99.9% 0.02 8.76 0.00 --
13989 2011:311:02:13:20.087 6 357.4 16.5 19019 18922 26 99.9% 100.0% 100.0% 99.9% 0.02 8.76 0.00 --
55075 2011:311:13:31:53.057 2 357.4 16.5 370 305 0 99.7% 100.0% 100.0% 99.7% 0.01 8.76 0.00 --
51466 2015:334:04:01:57.349 2 454.7 111.0 92 46 0 100.0% 100.0% 100.0% 100.0% 0.01 8.76 0.00 --
17280 2015:345:23:50:38.599 4 419.1 465.8 2587 2526 2 99.9% 100.0% 100.0% 99.9% 0.03 8.77 0.00 --
19568 2016:306:07:30:08.006 7 -219.4 -447.4 14837 14749 15 99.9% 100.0% 100.0% 99.9% 0.03 8.78 0.00 --
19913 2016:306:19:55:17.434 7 -219.6 -447.3 14593 14502 16 99.9% 100.0% 100.0% 99.9% 0.03 8.77 0.00 --
19914 2016:309:01:26:41.066 5 -218.6 -447.7 10569 10452 18 99.9% 100.0% 100.0% 99.9% 0.02 8.77 0.00 --
19915 2016:312:00:18:34.291 5 -217.9 -448.1 9407 9351 40 99.9% 100.0% 100.0% 99.9% 0.04 8.76 0.00 --
19565 2016:314:07:51:42.332 5 -356.6 -299.9 21613 21406 31 99.3% 100.0% 100.0% 99.3% 0.02 8.77 0.00 --
19938 2016:316:05:11:30.653 3 -358.2 -299.2 26619 26303 33 99.3% 100.0% 100.0% 99.3% 0.03 8.77 0.00 --
50492 2016:344:23:25:50.694 6 104.2 -488.3 1495 1397 0 97.6% 100.0% 100.0% 97.6% 0.03 8.79 0.00 --
20823 2017:297:12:19:23.807 5 -311.5 -392.6 26481 26103 17 98.8% 100.0% 100.0% 98.8% 0.06 8.75 0.00 --
20450 2017:300:01:10:05.439 5 -311.5 -392.6 14774 14569 12 99.1% 100.0% 100.0% 99.1% 0.06 8.76 0.00 --
20826 2017:301:22:47:41.110 5 -311.3 -392.7 14773 14521 16 98.6% 100.0% 100.0% 98.6% 0.06 8.76 0.00 --
20451 2017:302:23:51:49.602 7 -243.8 -435.4 18201 17964 24 99.1% 100.0% 100.0% 99.1% 0.04 8.74 0.00 --
20837 2017:304:14:35:41.397 7 -244.7 -435.0 17228 16985 18 99.1% 100.0% 100.0% 99.1% 0.04 8.75 0.00 --
20838 2017:305:09:44:32.996 7 -244.7 -435.0 12350 12099 17 98.5% 100.0% 100.0% 98.5% 0.04 8.75 0.00 --
20839 2017:307:15:04:52.402 4 -244.4 -435.2 10892 10611 20 98.0% 100.0% 100.0% 98.0% 0.04 8.76 0.00 --
20840 2017:308:12:39:11.164 7 -244.1 -435.3 10397 10161 13 98.6% 100.0% 100.0% 98.6% 0.04 8.76 0.00 --
20841 2017:313:07:17:26.228 7 -129.7 -478.8 26981 26427 35 98.2% 100.0% 100.0% 98.2% 0.05 8.79 0.00 --
20842 2017:314:06:36:48.894 7 -129.6 -478.9 9204 8972 16 98.2% 100.0% 100.0% 98.2% 0.03 8.80 0.00 --
20843 2017:315:04:07:29.382 7 -130.4 -478.5 11075 10915 10 99.3% 100.0% 100.0% 99.3% 0.03 8.80 0.00 --
20824 2017:336:08:03:23.720 6 323.4 -368.6 24536 24421 33 99.9% 100.0% 100.0% 99.9% 0.04 8.73 0.00 --
20827 2017:338:02:14:05.010 5 323.0 -368.4 8518 8432 12 99.9% 100.0% 100.0% 99.9% 0.04 8.73 0.00 --
20844 2017:339:02:34:53.901 5 323.0 -368.4 17225 17117 18 99.9% 100.0% 100.0% 99.9% 0.03 8.74 0.00 --
27864 2023:227:20:39:39.192 7 -457.3 -84.3 2516 2457 1 100.0% 100.0% 100.0% 100.0% 0.09 8.79 0.00 --
27866 2023:230:10:40:01.582 7 -457.8 -82.5 2500 2442 2 99.9% 100.0% 100.0% 99.9% 0.06 8.80 0.00 --
28474 2024:256:07:06:49.323 7 -418.0 -204.2 2539 2472 5 100.0% 100.0% 100.0% 100.0% 0.05 8.81 0.00 --
29635 2024:363:20:52:46.122 7 487.6 -118.0 4359 4293 2 100.0% 100.0% 100.0% 99.9% 0.07 8.85 0.00 --
30278 2025:056:15:49:04.557 7 485.3 128.5 3751 3684 3 99.9% 100.0% 100.0% 99.8% 0.06 8.80 0.00 --
30860 2025:080:21:19:14.054 7 429.9 273.2 2780 2711 0 100.0% 100.0% 100.0% 100.0% 0.06 8.79 0.00 --
30279 2025:091:02:09:36.629 7 415.6 295.6 3642 3564 3 100.0% 99.3% 100.0% 99.2% 0.08 8.80 0.00 --
30883 2025:091:09:39:30.345 7 414.8 295.9 4240 4176 2 100.0% 100.0% 100.0% 100.0% 0.08 8.81 0.00 --
31974 2025:308:16:18:36.629 7 -185.6 -458.9 3514 3455 2 100.0% 100.0% 100.0% 99.9% 0.06 8.76 0.00 --
29631 2025:315:06:14:54.850 7 -72.2 -487.2 3028 2956 0 100.0% 100.0% 100.0% 100.0% 0.04 8.77 0.00 --
30281 2025:328:10:34:40.070 7 216.6 -439.6 2528 2476 1 100.0% 100.0% 100.0% 100.0% 0.06 8.82 0.00 --
30317 2025:329:16:08:54.316 7 242.1 -427.3 2773 2710 0 99.9% 100.0% 100.0% 99.8% 0.07 8.80 0.00 --
32017 2025:334:01:21:08.298 7 207.2 -443.6 0 0 -1 0.0% 0.0% 0.0% 0.0% inf inf inf Error: No mica archive level 0 data.
31988 2025:334:08:25:36.862 7 246.3 -423.1 0 0 -1 0.0% 0.0% 0.0% 0.0% inf inf inf Error: No mica archive level 0 data.
31989 2025:334:15:19:43.680 7 207.4 -443.7 0 0 -1 0.0% 0.0% 0.0% 0.0% inf inf inf Error: No mica archive level 0 data.

  • 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.