AGASC ID 1091059112

Info

Last Obs. 2023:106:13:03
magcatalog 9.08 ± 0.11
mag3 arcsec 9.04 ± 0.02
mag5 arcsec 9.04 ± 0.02
Nobs 37 (0 bad)
fok 98.6%
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 mag100s ⟨ mag ⟩ σmag Comments
3515 2003:124:23:40:29.781 6 -342.3 -16.2 2649 2646 3 99.9% 100.0% 100.0% 99.9% 0.02 9.06 0.00 --
3516 2003:194:11:21:42.942 7 157.2 426.1 2764 2763 1 100.0% 100.0% 100.0% 100.0% 0.02 9.06 0.00 --
3517 2003:264:13:00:05.609 6 399.4 279.8 2640 2624 0 99.4% 100.0% 100.0% 99.4% 0.03 9.04 0.00 --
4596 2004:027:16:53:18.402 7 -97.3 -364.9 2523 2514 0 99.6% 100.0% 100.0% 99.6% 0.03 9.03 0.00 --
4597 2004:117:17:37:40.153 7 -334.0 -73.7 2387 2376 3 99.6% 100.0% 100.0% 99.5% 0.02 9.05 0.00 --
4598 2004:216:20:17:43.294 6 264.2 389.0 2529 2527 1 100.0% 100.0% 100.0% 100.0% 0.02 9.06 0.00 --
4599 2004:293:12:38:27.061 7 464.0 169.0 2511 2511 0 100.0% 100.0% 100.0% 100.0% 0.02 9.05 0.00 --
5592 2005:024:13:32:42.939 5 -86.3 -369.7 3443 2952 4 99.9% 100.0% 100.0% 99.9% 0.03 9.04 0.00 --
5593 2005:111:15:14:49.954 7 -324.8 -108.0 2531 2530 4 100.0% 100.0% 100.0% 100.0% 0.02 9.06 0.00 --
5472 2005:176:02:58:20.575 5 400.5 372.4 2529 2523 4 99.8% 100.0% 100.0% 99.8% 0.03 9.07 0.00 --
5594 2005:191:03:12:32.696 7 138.9 429.4 2530 2528 3 99.9% 100.0% 100.0% 99.9% 0.01 9.07 0.00 --
5595 2005:282:17:08:34.219 6 442.0 216.2 2286 2286 0 100.0% 100.0% 100.0% 100.0% 0.05 9.07 0.00 --
6684 2006:174:00:28:03.428 7 -156.5 377.7 29359 29316 56 99.9% 100.0% 100.0% 99.8% 0.02 9.06 0.00 --
8141 2007:172:02:27:53.358 7 -210.3 -436.5 1152 1149 3 99.7% 100.0% 100.0% 99.7% 0.02 9.06 0.00 --
57043 2009:166:05:34:46.426 6 -120.3 -462.7 25 25 0 100.0% 100.0% 100.0% 100.0% 0.01 9.04 0.00 --
11823 2010:152:05:00:06.000 6 -325.8 267.1 30938 30826 43 99.6% 100.0% 100.0% 99.6% 0.03 9.04 0.00 --
56227 2010:152:23:18:37.873 5 -325.8 267.1 61 61 0 100.0% 100.0% 100.0% 100.0% 0.01 9.03 0.00 --
56218 2010:154:02:30:39.895 7 -480.6 309.5 48 48 0 100.0% 100.0% 100.0% 100.0% 0.01 9.06 0.00 --
12224 2010:178:03:00:23.587 7 -56.5 418.6 9014 8999 17 99.8% 100.0% 100.0% 99.8% 0.02 9.03 0.00 --
12415 2011:284:04:59:14.980 7 -27.7 485.8 2529 2525 0 99.8% 100.0% 100.0% 99.8% 0.02 9.03 0.00 --
52740 2014:151:18:31:51.221 4 -413.1 253.9 1080 1073 0 99.4% 100.0% 100.0% 99.4% 0.02 9.04 0.00 --
17460 2015:013:14:11:52.011 4 -62.4 -395.8 12251 12014 16 98.1% 100.0% 100.0% 98.1% 0.03 9.04 0.00 --
51833 2015:164:22:05:38.381 3 34.1 209.9 1914 1898 3 99.2% 99.9% 100.0% 99.2% 0.03 9.06 0.00 --
51831 2015:165:08:30:34.210 5 37.1 209.5 2432 2423 4 99.6% 100.0% 100.0% 99.6% 0.03 9.05 0.00 --
16956 2015:169:13:57:04.167 7 -316.8 386.6 12282 11848 12 96.5% 100.0% 100.0% 96.5% 0.04 9.04 0.00 --
17676 2015:170:19:20:17.624 7 -316.8 386.6 16996 16239 23 95.5% 100.0% 100.0% 95.5% 0.03 9.04 0.00 --
18459 2016:144:07:22:45.312 7 -359.1 236.4 13094 12970 18 99.1% 100.0% 100.0% 99.1% 0.03 9.04 0.00 --
18854 2016:151:02:06:23.638 7 -359.1 236.4 6421 6312 6 98.3% 100.0% 100.0% 98.3% 0.03 9.04 0.00 --
18878 2016:177:09:12:08.024 6 -63.7 428.2 21558 21358 27 99.1% 100.0% 100.0% 99.1% 0.04 9.05 0.00 --
19724 2017:152:05:20:38.289 7 -284.9 325.0 23402 23157 26 99.0% 100.0% 100.0% 98.9% 0.05 9.01 0.00 --
19725 2018:011:11:28:36.289 6 -94.0 -397.3 23478 23282 17 99.2% 100.0% 100.0% 99.2% 0.07 9.03 0.00 --
20744 2018:159:18:48:10.113 5 -249.0 352.9 24872 24437 44 98.3% 100.0% 100.0% 98.2% 0.05 9.03 0.00 --
20746 2019:014:16:56:55.950 7 -113.7 -392.4 23530 23063 36 98.0% 100.0% 100.0% 98.0% 0.05 9.02 0.00 --
21692 2019:162:21:42:02.522 6 -217.7 375.0 25926 25156 38 97.0% 100.0% 100.0% 97.0% 0.06 9.05 0.00 --
24712 2021:145:17:48:53.836 5 -378.3 208.7 15207 14816 16 97.4% 100.0% 100.0% 97.4% 0.07 9.06 0.00 --
26017 2022:133:03:18:44.728 5 -413.3 116.4 13947 13881 10 99.5% 100.0% 100.0% 99.5% 0.10 9.09 0.00 --
27359 2023:106:13:03:15.581 6 -391.4 -161.8 7425 7375 6 99.3% 99.9% 100.0% 99.2% 0.13 9.05 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.