AGASC ID 261505808

Info

Last Obs. 2022:185:04:57
magcatalog 9.09 ± 0.15
mag3 arcsec 9.38 ± 0.03
mag5 arcsec 9.38 ± 0.03
Nobs 37 (0 bad)
fok 98.4%
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 mag ⟩ 100s ⟨ mag ⟩ σmag Comments
58136 2007:312:17:50:38.304 2 -320.3 -317.8 3557 3549 13 99.8% 99.8% 100.0% 99.6% 0.03 9.38 0.00 --
11391 2010:062:15:48:12.581 7 -132.2 -181.5 12333 12280 20 99.6% 100.0% 100.0% 99.5% 0.03 9.38 0.00 --
56419 2010:062:23:15:38.221 6 -132.2 -181.5 26 26 0 100.0% 100.0% 100.0% 100.0% 0.01 9.38 0.00 --
11975 2010:065:00:37:21.380 5 68.3 -368.9 22507 22478 37 99.9% 100.0% 100.0% 99.9% 0.03 9.44 0.00 --
16600 2014:070:06:47:37.220 6 -72.5 -207.2 48160 47750 47 99.1% 100.0% 100.0% 99.1% 0.05 9.38 0.00 --
16599 2014:072:21:37:13.351 6 -72.5 -207.2 14488 14249 16 98.4% 100.0% 100.0% 98.3% 0.04 9.38 0.00 --
15023 2014:074:12:52:31.653 6 -72.5 -207.2 21531 21342 25 99.1% 100.0% 100.0% 99.1% 0.04 9.38 0.00 --
52925 2014:075:01:40:29.372 5 -72.5 -207.2 1065 1055 2 99.1% 99.9% 100.0% 99.0% 0.04 9.39 0.00 --
15024 2014:075:13:33:07.771 6 -72.5 -207.2 10105 10059 8 99.5% 100.0% 100.0% 99.5% 0.03 9.38 0.00 --
18275 2016:076:01:50:33.356 6 -456.8 431.6 24617 23776 15 96.6% 100.0% 100.0% 96.6% 0.09 9.36 0.00 --
18795 2016:077:05:07:01.937 6 -456.8 431.6 13946 13409 10 96.1% 100.0% 100.0% 96.1% 0.08 9.36 0.00 --
51180 2016:077:13:20:06.149 6 -456.8 431.6 45 45 0 100.0% 100.0% 100.0% 100.0% 0.02 9.33 0.00 --
18796 2016:078:11:26:32.859 6 -456.8 431.6 19719 19087 14 96.8% 100.0% 100.0% 96.8% 0.10 9.37 0.00 --
18797 2016:079:06:16:11.059 6 -456.8 431.6 27037 25967 28 96.0% 100.0% 100.0% 96.0% 0.10 9.35 0.00 --
18798 2016:080:19:18:33.965 6 -456.8 431.6 6688 6572 5 98.3% 100.0% 100.0% 98.2% 0.09 9.35 0.00 --
50800 2016:215:14:46:32.927 4 -392.8 20.8 900 899 1 99.9% 99.9% 99.9% 99.8% 0.05 9.37 0.00 --
19998 2017:072:12:44:42.085 7 -401.7 482.9 15709 15546 22 99.0% 100.0% 100.0% 99.0% 0.06 9.40 0.00 --
18271 2017:074:10:54:18.618 7 -400.9 482.5 27207 26822 45 98.6% 100.0% 100.0% 98.6% 0.06 9.38 0.00 --
20037 2017:075:19:05:03.571 7 -400.2 482.3 8349 8242 16 98.7% 100.0% 100.0% 98.7% 0.04 9.37 0.00 --
20038 2017:077:02:55:03.385 7 -401.3 482.7 25035 24959 31 99.7% 100.0% 100.0% 99.7% 0.06 9.38 0.00 --
20039 2017:078:10:28:28.083 7 -400.7 482.5 10859 10677 11 98.3% 100.0% 100.0% 98.3% 0.07 9.39 0.00 --
18234 2017:087:23:59:14.786 4 -437.7 383.2 10013 9870 18 98.6% 100.0% 100.0% 98.6% 0.04 9.37 0.00 --
20049 2017:088:09:24:12.986 4 -437.5 383.2 10011 9958 7 99.5% 100.0% 100.0% 99.5% 0.06 9.37 0.00 --
20050 2017:088:23:08:56.473 4 -437.3 383.0 6919 6747 6 97.5% 100.0% 100.0% 97.5% 0.06 9.38 0.00 --
20051 2017:090:07:41:45.787 4 -437.9 383.4 7760 7657 13 98.7% 100.0% 100.0% 98.7% 0.04 9.38 0.00 --
49342 2018:095:12:43:51.911 5 -388.4 33.7 559 536 2 95.9% 99.8% 100.0% 95.7% 0.05 9.39 0.00 --
49341 2018:095:22:16:09.744 5 -388.8 29.3 275 270 0 98.5% 100.0% 100.0% 98.5% 0.04 9.39 0.00 --
49340 2018:096:05:31:23.003 5 -389.0 25.9 274 269 0 98.2% 99.6% 99.6% 97.8% 0.03 9.38 0.00 --
49339 2018:096:15:54:54.430 5 -389.2 21.4 274 265 0 96.7% 100.0% 100.0% 96.7% 0.04 9.37 0.00 --
22648 2020:063:16:27:39.861 7 -482.1 166.3 16162 15990 25 98.9% 99.9% 100.0% 98.9% 0.08 9.40 0.00 --
22649 2020:064:07:44:29.812 7 -481.7 166.1 16920 16740 19 98.9% 100.0% 100.0% 98.9% 0.12 9.39 0.00 --
23182 2020:064:22:10:58.565 7 -481.5 166.1 15203 14866 24 97.8% 100.0% 100.0% 97.8% 0.07 9.40 0.00 --
22930 2020:224:02:12:41.204 7 333.1 -320.2 18341 18122 32 98.8% 99.9% 99.9% 98.7% 0.10 9.42 0.00 --
23361 2020:307:18:29:37.534 7 148.1 460.9 9347 9300 22 99.5% 99.9% 100.0% 99.4% 0.06 9.37 0.00 --
24853 2020:308:16:00:08.218 7 140.2 463.5 13234 12989 7 98.1% 100.0% 100.0% 98.1% 0.14 9.39 0.00 --
24854 2020:313:01:32:16.378 7 122.9 469.0 4248 4189 8 98.6% 100.0% 100.0% 98.6% 0.04 9.35 0.00 --
23779 2022:185:04:57:28.762 7 -82.0 -467.3 25773 25400 13 98.6% 99.9% 100.0% 98.5% 0.19 9.37 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.