AGASC ID 373826120

Info

Last Obs. 2023:232:12:33
magcatalog 8.94 ± 0.06
mag3 arcsec 8.90 ± 0.02
mag5 arcsec 8.90 ± 0.02
Nobs 57 (1 bad)
fok 99.4%
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
3404 2002:223:15:56:32.785 6 200.4 177.3 3137 3085 2 99.9% 100.0% 100.0% 99.9% 0.02 8.90 0.00 --
4948 2004:283:10:37:27.995 4 114.3 253.2 58688 58586 63 99.9% 100.0% 100.0% 99.9% 0.02 8.90 0.00 --
4947 2004:285:16:30:11.929 4 105.4 256.3 14780 14725 11 100.0% 100.0% 100.0% 100.0% 0.02 8.90 0.00 --
4949 2004:286:01:38:30.183 4 106.3 256.8 14778 14707 21 99.9% 100.0% 100.0% 99.9% 0.02 8.90 0.00 --
4950 2004:286:10:07:00.183 4 107.2 257.3 48350 48256 62 99.9% 100.0% 100.0% 99.9% 0.02 8.90 0.00 --
4952 2004:288:06:04:50.619 4 102.8 259.9 81235 81123 97 99.9% 100.0% 100.0% 99.9% 0.03 8.90 0.00 --
60004 2004:290:05:24:51.836 1 -189.5 15.3 3718 3679 5 99.9% 100.0% 100.0% 99.9% 0.02 8.90 0.00 --
4951 2004:291:06:55:22.648 4 89.8 263.9 47563 47469 63 99.9% 100.0% 100.0% 99.9% 0.02 8.91 0.00 --
4953 2004:292:10:25:39.158 4 87.3 265.4 15120 15059 17 99.9% 100.0% 100.0% 99.9% 0.02 8.91 0.00 --
6145 2004:293:22:05:23.988 4 74.9 267.4 42098 41988 48 99.9% 100.0% 100.0% 99.9% 0.03 8.90 0.00 --
6146 2004:294:22:35:54.690 4 72.6 268.6 23553 23478 33 99.9% 100.0% 100.0% 99.9% 0.02 8.90 0.00 --
5596 2005:085:07:30:58.729 4 -255.5 218.8 2583 2528 2 100.0% 100.0% 100.0% 100.0% 0.02 8.90 0.00 --
8473 2006:318:20:20:27.595 4 191.2 177.5 14780 14686 22 99.9% 100.0% 100.0% 99.9% 0.02 8.90 0.00 --
9097 2007:349:00:51:35.025 3 -70.3 263.4 17220 17152 30 99.9% 100.0% 100.0% 99.9% 0.02 8.89 0.00 --
12025 2009:329:16:42:09.328 3 -233.6 252.3 8917 8851 19 99.9% 100.0% 100.0% 99.8% 0.02 8.89 0.00 --
12033 2009:331:08:57:27.714 3 -233.6 252.3 9409 9323 17 99.9% 99.9% 100.0% 99.8% 0.02 8.89 0.00 --
11713 2009:333:18:55:38.103 3 -275.0 204.4 55510 55297 87 99.7% 100.0% 100.0% 99.7% 0.03 8.89 0.00 --
12036 2009:336:07:29:55.547 5 -275.0 204.4 23881 23757 35 99.7% 100.0% 100.0% 99.7% 0.03 8.89 0.00 --
11715 2009:336:21:32:37.147 4 -203.9 41.1 36752 36635 60 99.8% 100.0% 100.0% 99.8% 0.03 8.90 0.00 --
12037 2009:339:17:51:13.756 4 -203.9 41.1 41912 41767 79 99.8% 100.0% 100.0% 99.8% 0.03 8.90 0.00 --
56615 2009:340:18:13:28.115 2 -203.9 41.1 141 28 0 100.0% 100.0% 100.0% 100.0% 0.01 8.90 0.00 --
11714 2009:341:18:07:00.005 4 -290.5 88.2 45521 45412 79 99.9% 100.0% 100.0% 99.9% 0.02 8.90 0.00 --
17283 2015:279:11:21:16.366 4 -34.2 58.2 2580 2511 0 100.0% 100.0% 100.0% 100.0% 0.04 8.89 0.00 --
17284 2015:279:13:19:15.611 4 -109.7 275.8 2580 2525 1 99.6% 100.0% 100.0% 99.6% 0.03 8.89 0.00 --
17286 2015:279:16:22:55.611 6 233.6 483.5 2584 2515 2 99.4% 100.0% 100.0% 99.4% 0.03 8.92 0.00 --
17260 2015:335:09:02:21.059 4 96.3 -97.0 2583 2478 2 98.2% 100.0% 100.0% 98.2% 0.02 8.94 0.00 --
17261 2015:335:21:44:35.377 4 -56.4 -189.9 2584 2506 2 99.1% 100.0% 100.0% 99.1% 0.03 8.91 0.00 --
17264 2015:335:23:45:30.906 4 -158.7 -321.8 2581 2527 2 99.9% 100.0% 100.0% 99.9% 0.02 8.91 0.00 --
17258 2015:337:20:40:01.246 4 422.0 -25.9 2587 2530 2 99.9% 100.0% 100.0% 99.9% 0.03 8.93 0.00 --
17259 2015:337:22:39:33.124 4 250.0 52.0 2587 2525 3 99.9% 100.0% 100.0% 99.9% 0.02 8.92 0.00 --
17263 2015:338:00:11:23.124 7 198.4 -488.0 2590 2492 1 98.3% 100.0% 100.0% 98.3% 0.03 8.93 0.00 --
17265 2015:341:09:35:05.041 4 -259.6 -474.2 2581 2454 1 98.0% 100.0% 100.0% 98.0% 0.02 8.90 0.00 --
17262 2015:341:11:46:46.658 4 118.9 -325.7 2582 2489 2 98.5% 100.0% 100.0% 98.5% 0.04 8.93 0.00 --
17278 2015:344:03:15:48.893 3 -419.3 406.8 2579 2524 3 99.7% 100.0% 100.0% 99.7% 0.03 8.90 0.00 --
17281 2015:345:20:41:17.816 7 89.2 487.7 2586 2525 5 99.9% 100.0% 100.0% 99.9% 0.02 8.93 0.00 --
19568 2016:306:07:30:08.006 4 -12.8 274.7 14827 14733 15 99.8% 100.0% 100.0% 99.8% 0.08 8.90 0.00 --
19913 2016:306:19:55:17.434 4 -13.0 274.8 14583 14490 18 99.8% 100.0% 100.0% 99.8% 0.08 8.90 0.00 --
19914 2016:309:01:26:41.066 4 -12.1 274.3 10534 10432 6 99.7% 100.0% 100.0% 99.7% 0.08 8.89 0.00 --
19915 2016:312:00:18:34.291 4 -11.4 274.0 9410 9261 2 98.9% 100.0% 100.0% 98.9% 0.09 8.87 0.00 --
50514 2016:336:18:24:07.764 6 -427.5 -381.9 6495 6300 17 97.7% 99.9% 100.0% 97.6% 0.06 8.92 0.00 --
20823 2017:297:12:19:23.807 4 46.5 267.7 26486 26005 58 98.5% 100.0% 100.0% 98.5% 0.04 8.90 0.00 --
20450 2017:300:01:10:05.439 4 46.5 267.7 14779 14498 16 98.6% 100.0% 100.0% 98.6% 0.04 8.90 0.00 --
20826 2017:301:22:47:41.110 4 46.7 267.6 14778 14451 21 98.1% 100.0% 100.0% 98.1% 0.04 8.90 0.00 --
20449 2017:310:16:12:34.676 4 -57.7 268.5 22579 21976 25 97.5% 100.0% 100.0% 97.5% 0.04 8.88 0.00 --
20841 2017:313:07:17:26.228 4 -58.2 268.7 26975 26082 216 96.9% 100.0% 100.0% 96.9% 0.07 8.88 0.00 --
20842 2017:314:06:36:48.894 4 -58.1 268.6 9195 8920 354 97.6% 100.0% 100.0% 97.6% 0.07 8.88 0.00 --
20843 2017:315:04:07:29.382 4 -58.9 269.0 11069 10843 11 98.6% 100.0% 100.0% 98.6% 0.04 8.88 0.00 --
20824 2017:336:08:03:23.720 4 -247.8 118.4 24535 23994 29 98.1% 100.0% 100.0% 98.1% 0.04 8.90 0.00 --
20827 2017:338:02:14:05.010 4 -248.2 118.6 8510 8310 10 98.4% 100.0% 100.0% 98.4% 0.03 8.90 0.00 --
20844 2017:339:02:34:53.901 4 -248.2 118.6 17215 16833 13 98.3% 100.0% 100.0% 98.3% 0.03 8.89 0.00 --
20880 2017:340:00:33:32.160 7 -475.9 -193.5 13569 13429 45 99.5% 100.0% 100.0% 99.4% 0.06 8.95 0.00 --
19564 2017:341:15:12:59.346 7 -476.9 -193.0 9911 9764 12 99.2% 100.0% 100.0% 99.2% 0.06 8.95 0.00 --
20881 2017:342:08:03:22.265 7 -475.9 -193.5 19657 19320 22 98.6% 100.0% 100.0% 98.6% 0.07 8.96 0.00 --
22644 2019:310:09:18:20.146 4 -270.4 76.7 12334 12133 14 98.8% 100.0% 100.0% 98.8% 0.03 8.92 0.00 --
23064 2019:311:11:36:50.487 4 -270.7 76.8 11964 11617 20 97.5% 100.0% 100.0% 97.5% 0.04 8.91 0.00 --
23084 2019:334:17:24:42.563 3 -192.4 -185.0 15266 15171 22 99.9% 100.0% 100.0% 99.9% 0.05 8.91 0.00 --
27869 2023:232:12:33:49.014 7 126.5 165.6 0 0 -1 0.0% 0.0% 0.0% 0.0% inf inf inf Error: No 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.