AGASC ID 373817952

Info

Last Obs. 2024:264:00:45
magcatalog 8.73 ± 0.02
mag3 arcsec 8.74 ± 0.01
mag5 arcsec 8.74 ± 0.01
Nobs 74 (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
3209 2002:220:07:51:20.918 4 378.2 107.9 47463 47368 38 99.9% 100.0% 100.0% 99.9% 0.03 8.73 0.00 --
4289 2002:222:12:40:12.785 4 378.2 107.9 47229 47138 49 99.9% 100.0% 100.0% 99.9% 0.02 8.73 0.00 --
3404 2002:223:15:56:32.785 5 368.0 116.3 3140 3084 2 99.9% 100.0% 100.0% 99.9% 0.02 8.74 0.00 --
6139 2004:278:22:26:47.131 3 302.8 257.7 28092 28019 29 99.9% 100.0% 100.0% 99.9% 0.02 8.74 0.00 --
4946 2004:280:20:51:25.224 3 297.4 264.2 11774 11691 14 99.9% 100.0% 100.0% 99.9% 0.02 8.73 0.00 --
4948 2004:283:10:37:27.995 3 291.6 273.3 58683 58583 74 99.9% 100.0% 100.0% 99.9% 0.02 8.74 0.00 --
4947 2004:285:16:30:11.929 3 282.0 281.6 14782 14721 13 100.0% 100.0% 100.0% 100.0% 0.02 8.73 0.00 --
4949 2004:286:01:38:30.183 3 282.8 282.8 14780 14721 12 100.0% 100.0% 100.0% 100.0% 0.02 8.74 0.00 --
4950 2004:286:10:07:00.183 3 283.6 284.1 48351 48266 52 99.9% 100.0% 100.0% 99.9% 0.03 8.74 0.00 --
4952 2004:288:06:04:50.619 3 278.4 291.4 81236 81126 91 99.9% 100.0% 100.0% 99.9% 0.02 8.74 0.00 --
60004 2004:290:05:24:51.836 0 -15.1 49.8 3720 3680 2 99.9% 100.0% 100.0% 99.9% 0.02 8.73 0.00 --
4951 2004:291:06:55:22.648 3 263.8 303.3 47565 47476 60 99.9% 100.0% 100.0% 99.9% 0.03 8.74 0.00 --
4953 2004:292:10:25:39.158 3 260.7 307.9 15122 15063 16 99.9% 100.0% 100.0% 99.9% 0.02 8.74 0.00 --
6145 2004:293:22:05:23.988 3 247.1 314.2 42327 41133 35 97.4% 100.0% 100.0% 97.4% 0.02 8.74 0.00 --
6146 2004:294:22:35:54.690 3 243.9 318.4 23554 23475 31 99.9% 100.0% 100.0% 99.9% 0.02 8.74 0.00 --
5597 2004:358:05:33:26.453 3 -187.7 443.0 12489 12429 16 99.9% 100.0% 100.0% 99.9% 0.02 8.74 0.00 --
5596 2005:085:07:30:58.729 3 -434.9 220.1 2581 2528 1 100.0% 100.0% 100.0% 100.0% 0.01 8.75 0.00 --
8473 2006:318:20:20:27.595 3 285.6 329.6 14781 14672 34 99.8% 100.0% 100.0% 99.8% 0.02 8.74 0.00 --
9097 2007:349:00:51:35.025 6 -169.0 412.9 17225 17148 20 99.9% 100.0% 100.0% 99.9% 0.02 8.73 0.00 --
11716 2009:283:11:56:45.729 3 235.6 224.4 19656 19574 40 99.9% 100.0% 100.0% 99.9% 0.02 8.76 0.00 --
12025 2009:329:16:42:09.328 5 -226.4 431.4 8918 8853 16 99.9% 100.0% 100.0% 99.9% 0.03 8.73 0.00 --
12033 2009:331:08:57:27.714 5 -226.4 431.4 9410 9320 18 99.8% 100.0% 100.0% 99.8% 0.03 8.73 0.00 --
11715 2009:336:21:32:37.147 3 -257.9 210.9 36755 36467 60 99.3% 100.0% 100.0% 99.3% 0.03 8.74 0.00 --
12037 2009:339:17:51:13.756 3 -257.9 210.9 41917 41570 56 99.3% 100.0% 100.0% 99.3% 0.03 8.74 0.00 --
56615 2009:340:18:13:28.115 0 -257.9 210.9 140 28 0 100.0% 100.0% 100.0% 100.0% 0.00 8.74 0.00 --
11714 2009:341:18:07:00.005 3 -359.4 253.3 45519 45415 59 99.9% 100.0% 100.0% 99.9% 0.03 8.74 0.00 --
17065 2015:187:05:17:24.313 3 -64.9 345.1 4048 3984 3 99.7% 100.0% 100.0% 99.7% 0.02 8.73 0.00 --
17283 2015:279:11:21:16.366 3 143.0 69.3 2584 2446 2 97.3% 99.9% 99.9% 97.2% 0.02 8.76 0.00 --
17284 2015:279:13:19:15.611 3 67.9 286.7 2581 2531 2 99.9% 100.0% 100.0% 99.9% 0.03 8.75 0.00 --
17285 2015:279:14:51:05.611 3 178.2 477.2 2582 2516 8 99.5% 100.0% 100.0% 99.5% 0.02 8.76 0.00 --
17260 2015:335:09:02:21.059 3 79.6 79.8 2584 2516 3 99.7% 100.0% 100.0% 99.7% 0.02 8.75 0.00 --
17261 2015:335:21:44:35.377 3 -88.1 -15.0 2582 2516 2 99.5% 100.0% 100.0% 99.5% 0.02 8.76 0.00 --
17264 2015:335:23:45:30.906 3 -212.8 -152.0 2579 2518 2 99.6% 100.0% 100.0% 99.6% 0.02 8.74 0.00 --
17258 2015:337:20:40:01.246 3 373.1 145.4 2585 2513 3 99.2% 100.0% 100.0% 99.2% 0.02 8.72 0.00 --
17259 2015:337:22:39:33.124 3 202.5 223.4 2585 2524 5 99.8% 100.0% 100.0% 99.8% 0.02 8.75 0.00 --
17263 2015:338:00:11:23.124 3 150.0 -314.5 2586 2531 2 99.9% 100.0% 100.0% 99.9% 0.03 8.76 0.00 --
17266 2015:338:01:43:13.124 3 -438.2 -444.2 2578 2510 2 99.3% 100.0% 100.0% 99.3% 0.02 8.76 0.00 --
17265 2015:341:09:35:05.041 3 -322.6 -306.3 2580 2444 1 97.6% 100.0% 100.0% 97.6% 0.03 8.75 0.00 --
17262 2015:341:11:46:46.658 3 51.9 -160.3 2581 2495 3 98.7% 100.0% 100.0% 98.7% 0.02 8.77 0.00 --
17267 2015:346:01:23:00.009 3 -404.9 -189.4 3049 2982 3 99.3% 100.0% 100.0% 99.3% 0.03 8.74 0.00 --
19568 2016:306:07:30:08.006 3 138.3 369.7 14828 14744 23 99.9% 100.0% 100.0% 99.9% 0.03 8.75 0.00 --
19913 2016:306:19:55:17.434 3 138.0 369.8 14584 14503 19 99.9% 100.0% 100.0% 99.9% 0.03 8.75 0.00 --
19914 2016:309:01:26:41.066 3 139.0 369.3 10532 10444 13 99.8% 100.0% 100.0% 99.8% 0.02 8.75 0.00 --
19915 2016:312:00:18:34.291 3 139.7 369.0 9411 9333 31 99.7% 100.0% 100.0% 99.6% 0.04 8.74 0.00 --
50514 2016:336:18:24:07.764 7 -459.5 -205.5 6497 6345 23 98.4% 99.9% 100.0% 98.4% 0.04 8.75 0.00 --
20823 2017:297:12:19:23.807 3 214.5 327.7 26488 26132 34 99.0% 100.0% 100.0% 98.9% 0.04 8.72 0.00 --
20450 2017:300:01:10:05.439 3 214.5 327.7 14782 14703 24 100.0% 100.0% 100.0% 100.0% 0.03 8.72 0.00 --
20826 2017:301:22:47:41.110 3 214.7 327.6 14781 14578 16 99.0% 100.0% 100.0% 99.0% 0.03 8.72 0.00 --
20451 2017:302:23:51:49.602 3 163.0 358.3 18197 18027 22 99.4% 100.0% 100.0% 99.4% 0.03 8.73 0.00 --
20837 2017:304:14:35:41.397 3 162.2 358.7 17222 16988 19 99.1% 100.0% 100.0% 99.1% 0.03 8.73 0.00 --
20838 2017:305:09:44:32.996 3 162.1 358.7 12344 12237 17 99.6% 100.0% 100.0% 99.6% 0.03 8.73 0.00 --
20839 2017:307:15:04:52.402 3 162.5 358.6 10878 10743 16 99.3% 100.0% 100.0% 99.3% 0.04 8.73 0.00 --
20840 2017:308:12:39:11.164 3 162.7 358.4 10393 10196 16 98.9% 100.0% 100.0% 98.9% 0.03 8.72 0.00 --
20449 2017:310:16:12:34.676 3 73.5 389.4 22583 22329 35 99.1% 100.0% 100.0% 99.1% 0.03 8.73 0.00 --
20841 2017:313:07:17:26.228 3 73.0 389.6 26976 26624 37 99.0% 100.0% 100.0% 98.9% 0.04 8.73 0.00 --
20842 2017:314:06:36:48.894 3 73.2 389.6 9196 9046 18 99.0% 100.0% 100.0% 98.9% 0.03 8.73 0.00 --
20843 2017:315:04:07:29.382 3 72.3 390.0 11073 10920 17 99.3% 100.0% 100.0% 99.3% 0.03 8.73 0.00 --
20824 2017:336:08:03:23.720 3 -271.7 295.3 24533 24086 21 98.5% 100.0% 100.0% 98.5% 0.04 8.72 0.00 --
20827 2017:338:02:14:05.010 3 -272.1 295.5 8511 8246 17 97.7% 100.0% 100.0% 97.7% 0.03 8.72 0.00 --
20844 2017:339:02:34:53.901 3 -272.1 295.5 17214 16745 22 97.8% 100.0% 100.0% 97.7% 0.03 8.72 0.00 --
22644 2019:310:09:18:20.146 3 -127.7 183.0 12345 12059 19 98.2% 100.0% 100.0% 98.1% 0.05 8.75 0.00 --
23064 2019:311:11:36:50.487 3 -127.9 183.1 11969 11763 18 98.8% 100.0% 100.0% 98.8% 0.03 8.75 0.00 --
22888 2019:333:23:14:12.645 3 -214.6 -2.0 15263 14953 14 98.4% 100.0% 100.0% 98.4% 0.07 8.77 0.00 --
27864 2023:227:20:39:39.192 6 415.3 99.2 2518 2457 2 100.0% 100.0% 100.0% 100.0% 0.08 8.74 0.00 --
27865 2023:229:14:13:52.607 6 316.4 96.0 2533 2469 2 99.9% 100.0% 100.0% 99.9% 0.05 8.74 0.00 --
27866 2023:230:10:40:01.582 6 415.4 98.0 2516 2444 5 100.0% 100.0% 100.0% 100.0% 0.07 8.75 0.00 --
27867 2023:231:02:36:35.617 6 314.4 99.9 2639 2573 2 100.0% 100.0% 100.0% 100.0% 0.05 8.75 0.00 --
27868 2023:231:19:28:02.371 5 393.2 107.0 2541 2468 0 100.0% 100.0% 100.0% 100.0% 0.05 8.75 0.00 --
27869 2023:232:12:33:49.014 6 291.1 97.8 2535 2469 0 99.9% 100.0% 100.0% 99.9% 0.08 8.76 0.00 --
28475 2024:263:10:55:49.735 6 270.8 208.8 2532 2477 1 100.0% 99.9% 100.0% 99.9% 0.06 8.77 0.00 --
28476 2024:263:14:05:47.299 7 370.1 209.5 2524 2487 1 100.0% 100.0% 100.0% 100.0% 0.05 8.77 0.00 --
28477 2024:263:17:00:57.299 6 271.3 209.0 2709 2672 0 99.9% 100.0% 100.0% 99.9% 0.08 8.79 0.00 --
28478 2024:263:21:29:05.704 7 352.6 207.9 2537 2464 2 99.9% 100.0% 100.0% 99.9% 0.07 8.76 0.00 --
28479 2024:264:00:45:57.532 6 247.9 207.5 2522 2485 1 99.9% 100.0% 100.0% 99.9% 0.07 8.77 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.