AGASC ID 896540888

Info

Last Obs. 2022:242:15:46
magcatalog 7.96 ± 0.11
mag3 arcsec 7.88 ± 0.01
mag5 arcsec 7.88 ± 0.01
Nobs 74 (0 bad)
fok 99.7%
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
6188 2005:156:01:25:11.127 5 -414.5 -186.4 2499 2495 9 99.9% 100.0% 100.0% 99.9% 0.03 7.90 0.00 --
5508 2005:157:23:36:36.873 7 471.0 -380.6 546 546 0 100.0% 100.0% 100.0% 100.0% 0.02 7.89 0.00 --
6189 2005:291:13:15:58.702 4 306.5 343.8 2139 2137 2 99.9% 100.0% 100.0% 99.9% 0.01 7.88 0.00 --
7044 2006:305:13:53:43.656 6 268.6 376.3 18716 18712 16 100.0% 100.0% 100.0% 100.0% 0.01 7.87 0.00 --
7048 2007:045:03:36:21.544 7 -458.5 -321.9 19549 19048 23 100.0% 100.0% 100.0% 100.0% 0.01 7.89 0.00 --
7045 2007:054:06:59:53.859 7 -188.4 -482.2 18301 18259 19 99.8% 100.0% 100.0% 99.8% 0.02 7.88 0.00 --
7498 2007:187:04:47:37.842 5 -116.8 247.4 579 579 0 100.0% 100.0% 100.0% 100.0% 0.01 7.86 0.00 --
7046 2007:200:09:57:19.214 4 293.9 305.2 18499 18491 17 100.0% 100.0% 100.0% 100.0% 0.02 7.87 0.00 --
8531 2007:205:09:29:48.526 7 241.4 395.7 2528 2526 2 99.9% 100.0% 100.0% 99.9% 0.01 7.87 0.00 --
9030 2008:131:15:56:39.059 5 -349.4 -283.3 2527 2526 1 100.0% 100.0% 100.0% 100.0% 0.02 7.87 0.00 --
9035 2008:197:20:40:38.243 6 223.6 407.0 2532 2529 4 99.9% 100.0% 100.0% 99.9% 0.02 7.87 0.00 --
11795 2010:201:23:39:49.155 6 85.9 236.8 48725 48710 49 100.0% 100.0% 100.0% 100.0% 0.02 7.87 0.00 --
56113 2010:203:03:48:47.795 4 85.9 236.8 99 99 0 100.0% 100.0% 100.0% 100.0% 0.01 7.87 0.00 --
14897 2013:219:16:35:33.300 6 419.5 442.4 25085 25060 16 99.9% 100.0% 100.0% 99.9% 0.01 7.89 0.00 --
17239 2015:231:17:07:43.996 5 446.0 464.8 39105 39074 52 99.9% 100.0% 100.0% 99.9% 0.03 7.90 0.00 --
18323 2016:197:05:45:38.383 5 386.0 340.9 1152 1152 0 100.0% 100.0% 100.0% 100.0% 0.01 7.88 0.00 --
18326 2016:197:08:00:08.383 5 163.2 433.9 1154 1153 1 99.9% 100.0% 100.0% 99.9% 0.01 7.88 0.00 --
18328 2016:197:09:29:48.383 6 211.9 301.6 1157 1155 2 99.9% 100.0% 100.0% 99.9% 0.01 7.88 0.00 --
18329 2016:197:10:14:38.383 4 40.1 457.6 1154 1153 0 100.0% 100.0% 100.0% 100.0% 0.01 7.89 0.00 --
21592 2019:183:19:22:23.337 5 -23.7 56.0 1073 1069 2 99.7% 100.0% 100.0% 99.7% 0.02 7.87 0.00 --
21593 2019:183:20:05:37.866 3 428.9 -167.4 1070 1065 4 99.6% 100.0% 100.0% 99.6% 0.01 7.88 0.00 --
21594 2019:183:20:47:27.866 5 224.1 194.3 1072 1053 1 98.3% 100.0% 100.0% 98.3% 0.02 7.87 0.00 --
21596 2019:183:22:11:07.866 4 441.3 21.3 1072 1070 0 99.8% 100.0% 100.0% 99.8% 0.01 7.86 0.00 --
21597 2019:183:22:52:57.866 4 362.6 289.4 1069 1064 0 99.5% 100.0% 100.0% 99.5% 0.01 7.87 0.00 --
21598 2019:183:23:34:47.866 4 298.3 -69.8 1071 1071 1 100.0% 100.0% 100.0% 100.0% 0.01 7.89 0.00 --
21600 2019:184:00:58:27.866 6 120.0 69.6 1070 1070 1 100.0% 100.0% 100.0% 100.0% 0.02 7.88 0.00 --
21602 2019:184:02:22:07.866 6 335.2 113.2 1070 1061 1 99.2% 100.0% 100.0% 99.2% 0.01 7.87 0.00 --
21618 2019:209:17:38:14.055 6 -192.0 482.7 1066 1066 0 100.0% 100.0% 100.0% 100.0% 0.02 7.87 0.00 --
21624 2019:209:21:49:14.055 7 -176.5 275.8 1067 1062 3 99.6% 100.0% 100.0% 99.6% 0.01 7.87 0.00 --
21626 2019:209:23:12:54.055 6 -278.1 432.8 1069 1068 0 99.9% 100.0% 100.0% 99.9% 0.02 7.87 0.00 --
23888 2021:183:01:56:28.737 5 238.4 64.7 2632 2629 3 99.9% 100.0% 100.0% 99.9% 0.02 7.88 0.00 --
26294 2022:035:05:33:55.153 6 -468.0 -419.2 7524 7520 2 99.9% 100.0% 100.0% 99.9% 0.02 7.88 0.00 --
24367 2022:036:07:31:37.366 7 -484.6 -401.8 8845 8824 8 99.8% 100.0% 100.0% 99.8% 0.03 7.89 0.00 --
26295 2022:036:17:59:54.998 7 -489.3 -396.8 5924 5916 4 99.9% 100.0% 100.0% 99.9% 0.02 7.89 0.00 --
24822 2022:041:07:42:02.250 6 -476.5 -406.9 8855 8805 7 99.4% 100.0% 100.0% 99.4% 0.02 7.89 0.00 --
26304 2022:041:18:16:21.577 6 -476.7 -406.7 5921 5894 6 99.5% 100.0% 100.0% 99.5% 0.02 7.89 0.00 --
24189 2022:071:11:48:03.575 4 277.4 -7.0 2208 2203 1 99.8% 100.0% 100.0% 99.8% 0.02 7.91 0.00 --
24190 2022:071:13:09:17.654 5 238.1 -200.9 2208 2200 2 99.6% 100.0% 100.0% 99.6% 0.02 7.90 0.00 --
24191 2022:071:14:30:00.987 5 197.1 -399.6 2205 2197 1 99.6% 100.0% 100.0% 99.6% 0.01 7.89 0.00 --
24198 2022:076:12:27:36.770 6 475.4 -156.0 2201 2176 3 98.9% 100.0% 100.0% 98.9% 0.02 7.88 0.00 --
24360 2022:090:06:30:58.802 6 -465.8 -418.4 15187 15090 15 99.4% 100.0% 100.0% 99.4% 0.04 7.89 0.00 --
23902 2022:092:21:41:03.279 5 -417.6 3.4 2667 2642 3 99.1% 100.0% 100.0% 99.1% 0.03 7.92 0.00 --
24132 2022:103:15:26:29.283 3 356.7 -5.9 2209 2208 0 100.0% 100.0% 100.0% 100.0% 0.02 7.91 0.00 --
24133 2022:103:16:50:44.093 4 340.1 -204.2 2206 2199 1 99.7% 100.0% 100.0% 99.7% 0.02 7.88 0.00 --
24134 2022:103:18:11:27.426 5 218.4 -403.6 2206 2173 5 98.5% 100.0% 100.0% 98.5% 0.02 7.88 0.00 --
24135 2022:103:19:32:10.759 4 377.6 195.7 2206 2167 0 98.3% 100.0% 100.0% 98.3% 0.03 7.87 0.00 --
24136 2022:103:20:52:54.092 6 399.5 401.0 2210 2205 4 99.8% 100.0% 100.0% 99.8% 0.02 7.87 0.00 --
24222 2022:104:07:42:09.748 4 66.1 -169.7 2213 2192 2 99.1% 100.0% 100.0% 99.1% 0.02 7.90 0.00 --
24224 2022:106:22:22:47.864 4 -119.9 127.0 2210 2201 2 99.6% 100.0% 100.0% 99.6% 0.02 7.91 0.00 --
24225 2022:107:16:13:31.617 5 -98.1 331.6 2182 2176 2 99.7% 100.0% 100.0% 99.7% 0.02 7.90 0.00 --
24370 2022:107:20:41:04.263 7 -479.7 -401.8 14726 14665 10 99.6% 100.0% 100.0% 99.6% 0.04 7.89 0.00 --
23890 2022:116:07:57:51.134 4 -254.0 245.4 2838 2817 4 99.3% 100.0% 100.0% 99.3% 0.02 7.90 0.00 --
24061 2022:145:16:34:28.943 4 154.7 2.7 2203 2200 1 99.9% 100.0% 100.0% 99.9% 0.05 7.90 0.00 --
24062 2022:146:09:58:41.259 5 156.5 -172.9 2170 2170 2 100.0% 100.0% 100.0% 100.0% 0.02 7.91 0.00 --
24063 2022:146:11:53:36.850 4 165.5 205.2 2209 2205 2 99.9% 100.0% 100.0% 99.9% 0.02 7.89 0.00 --
24064 2022:146:13:14:20.183 5 249.5 368.9 2205 2191 5 99.4% 100.0% 100.0% 99.4% 0.02 7.88 0.00 --
23898 2022:151:21:03:58.893 4 -278.7 369.3 2653 2643 1 99.6% 100.0% 100.0% 99.6% 0.02 7.89 0.00 --
24067 2022:166:15:55:39.769 3 22.8 77.6 2208 2204 2 99.8% 100.0% 100.0% 99.8% 0.02 7.90 0.00 --
24068 2022:166:17:17:25.089 5 354.2 312.4 2208 2207 2 100.0% 100.0% 100.0% 100.0% 0.02 7.87 0.00 --
24192 2022:181:16:08:57.101 4 -256.1 -264.5 2417 2409 6 99.7% 100.0% 100.0% 99.7% 0.02 7.88 0.00 --
24197 2022:181:17:37:22.986 6 -455.4 -193.0 2418 2409 3 99.7% 100.0% 100.0% 99.7% 0.02 7.89 0.00 --
23905 2022:185:21:57:30.396 4 353.4 -348.9 2669 2641 1 99.0% 100.0% 100.0% 99.0% 0.04 7.90 0.00 --
23906 2022:185:23:36:57.902 4 461.1 -286.4 2668 2654 2 99.5% 100.0% 100.0% 99.5% 0.02 7.89 0.00 --
23902 2022:194:16:40:48.381 5 393.6 117.2 2664 2622 0 98.4% 100.0% 100.0% 98.4% 0.03 7.88 0.00 --
24069 2022:201:10:36:23.125 5 58.6 -248.2 2211 2198 2 99.4% 100.0% 100.0% 99.4% 0.02 7.91 0.00 --
24218 2022:205:08:49:30.792 3 -86.5 -19.2 2174 2168 3 99.7% 100.0% 100.0% 99.7% 0.02 7.91 0.00 --
24219 2022:205:10:35:02.838 4 -73.7 -215.7 2207 2203 2 99.8% 100.0% 100.0% 99.8% 0.02 7.89 0.00 --
24220 2022:205:11:55:46.171 5 -61.3 -421.4 2210 2200 0 99.6% 100.0% 100.0% 99.6% 0.02 7.88 0.00 --
24822 2022:211:00:23:54.573 6 441.2 457.1 8865 8825 4 99.5% 100.0% 100.0% 99.5% 0.02 7.88 0.00 --
24372 2022:214:13:29:27.756 6 424.5 475.1 16171 16042 6 99.2% 100.0% 100.0% 99.2% 0.03 7.88 0.00 --
26304 2022:218:20:25:29.379 6 452.1 446.1 5922 5912 6 99.8% 100.0% 100.0% 99.8% 0.03 7.89 0.00 --
24364 2022:219:00:22:03.931 7 404.2 445.2 5311 5297 4 99.7% 100.0% 100.0% 99.7% 0.02 7.88 0.00 --
24375 2022:219:14:20:10.719 6 454.7 444.5 13737 13538 10 98.6% 100.0% 100.0% 98.6% 0.03 7.88 0.00 --
24750 2022:242:15:46:14.585 6 454.3 445.1 5431 5378 0 99.0% 100.0% 100.0% 99.0% 0.03 7.87 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.