CameraObs.Time(UTC)FieldPreviewStatusLogPointing.Offset(°)mag.lim.FWHM(pix)Candidates(new/total)Comments
TTUQ2b1x120.10.2026 05:16:03.663 Aql-02-Q2b1x1 OKlog0.020314.32.10/0
TTUQ2b1x120.10.2026 05:17:33.317 Aql-01-Q2b1x1 ERRORlog0.05272.10/0ERROR: large change in astrometric-star counts between the two new images (q4: 378 -> 259, 31.481% > 20%; fd_Aql-01-Q2b1x1_2026-10-20_00-16-43_20.00sec_0.00C_LIGHT_0003.fits vs fd_Aql-01-Q2b1x1_2026-10-20_00-17-33_20.00sec_-0.00C_LIGHT_0004.fits) - usually a bad plate solution on one of them, sometimes stars crossing a quadrant boundary when the two images are widely offset, rarely a transparency change; continuing processing
TTUQ2b1x120.10.2026 05:19:15.896 Vul-01-Q2b1x1 ERRORlog0.10032.20/0ERROR: large change in astrometric-star counts between the two new images (q2: 676 -> 526, 22.189% > 20%; fd_Vul-01-Q2b1x1_2026-10-20_00-18-12_20.00sec_-0.00C_LIGHT_0005.fits vs fd_Vul-01-Q2b1x1_2026-10-20_00-19-15_20.00sec_-0.00C_LIGHT_0006.fits) - usually a bad plate solution on one of them, sometimes stars crossing a quadrant boundary when the two images are widely offset, rarely a transparency change; continuing processing
TTUQ2b1x120.10.2026 05:21:21.461 Vul-02-Q2b1x1 ERRORlog0.01622.50/0ERROR: large change in astrometric-star counts between the two new images (q3: 1377 -> 913, 33.696% > 20%; fd_Vul-02-Q2b1x1_2026-10-20_00-20-13_20.00sec_-0.00C_LIGHT_0007.fits vs fd_Vul-02-Q2b1x1_2026-10-20_00-21-21_20.00sec_-0.00C_LIGHT_0008.fits) - usually a bad plate solution on one of them, sometimes stars crossing a quadrant boundary when the two images are widely offset, rarely a transparency change; continuing processing
TTUQ2b1x120.10.2026 05:22:56.806 Cyg-08-Q2b1x1 OKlog0.068414.82.40/0
TTUQ2b1x120.10.2026 05:24:47.224 Cyg-05-Q2b1x1 OKlog0.016914.82.20/0
TTUQ2b1x120.10.2026 05:26:29.093 Cyg-06-Q2b1x1 OKlog0.011815.02.40/0
TTUQ2b1x120.10.2026 05:27:59.928 Cyg-06-Q2b1x1 OKlog0.016115.02.40/0
TTUQ2b1x120.10.2026 05:29:30.858 Cyg-03-Q2b1x1 OKlog0.062215.12.40/0
TTUQ2b1x120.10.2026 05:30:45.719 Cyg-03-Q2b1x1 OKlog0.061515.12.40/0
TTUQ2b1x120.10.2026 05:32:56.024 Cyg-04-Q2b1x1 OKlog0.010715.22.40/0
TTUQ2b1x120.10.2026 05:36:01.526 Cyg-02-Q2b1x1 OKlog0.018515.22.50/0
TTUQ2b1x120.10.2026 05:34:28.612 Cyg-04-Q2b1x1 OKlog0.012915.22.40/0
TTUQ2b1x120.10.2026 05:42:08.825 Cep-06-Q2b1x1 OKlog0.023115.22.40/0
TTUQ2b1x120.10.2026 05:37:20.494 Cyg-02-Q2b1x1 OKlog0.024015.22.50/0
TTUQ2b1x120.10.2026 05:39:08.586 Lac-01-Q2b1x1 OKlog0.018715.32.40/0
TTUQ2b1x120.10.2026 05:43:41.256 Cep-06-Q2b1x1 OKlog0.023715.22.40/0
TTUQ2b1x120.10.2026 05:40:21.087 Lac-01-Q2b1x1 OKlog0.019315.22.40/0
TTUQ2b1x120.10.2026 05:49:08.957 Cep-03-Q2b1x1 OKlog0.015815.32.30/0
TTUQ2b1x120.10.2026 05:52:26.134 Cas-01-Q2b1x1 OKlog0.026815.42.20/0
TTUQ2b1x120.10.2026 05:46:01.155 Cas-04-Q2b1x1 OKlog0.016215.42.30/0
TTUQ2b1x120.10.2026 05:56:24.221 Cas-02-Q2b1x1 ERRORlog0.01292.60/1ERROR: large change in astrometric-star counts between the two new images (q2: 765 -> 583, 23.791% > 20%; fd_Cas-02-Q2b1x1_2026-10-20_00-55-18_20.00sec_-0.00C_LIGHT_0049.fits vs fd_Cas-02-Q2b1x1_2026-10-20_00-56-24_20.00sec_-0.00C_LIGHT_0050.fits) - usually a bad plate solution on one of them, sometimes stars crossing a quadrant boundary when the two images are widely offset, rarely a transparency change; continuing processing
TTUQ2b1x120.10.2026 05:50:16.544 Cep-03-Q2b1x1 OKlog0.019915.32.30/0
TTUQ2b1x120.10.2026 05:54:01.178 Cas-01-Q2b1x1 OKlog0.034215.32.20/0
TTUQ2b1x120.10.2026 05:47:30.124 Cas-04-Q2b1x1 OKlog0.010415.42.30/0
TTUQ2b1x120.10.2026 05:56:49.805 Cas-02-Q2b1x1 ERRORlog0.00902.70/1ERROR: large change in astrometric-star counts between the two new images (q2: 337 -> 258, 23.442% > 20%; fd_Cas-02-Q2b1x1_2026-10-20_00-56-49_20.00sec_-0.00C_LIGHT_0051.fits vs fd_Cas-02-Q2b1x1_2026-10-20_00-57-37_20.00sec_0.00C_LIGHT_0052.fits) - usually a bad plate solution on one of them, sometimes stars crossing a quadrant boundary when the two images are widely offset, rarely a transparency change; continuing processing
TTUQ2b1x120.10.2026 05:59:46.935 Cas-03-Q2b1x1 ERRORlog0.01392.30/0ERROR: large change in astrometric-star counts between the two new images (q3: 607 -> 475, 21.746% > 20%; fd_Cas-03-Q2b1x1_2026-10-20_00-58-54_20.00sec_-0.00C_LIGHT_0053.fits vs fd_Cas-03-Q2b1x1_2026-10-20_00-59-46_20.00sec_0.00C_LIGHT_0054.fits) - usually a bad plate solution on one of them, sometimes stars crossing a quadrant boundary when the two images are widely offset, rarely a transparency change; continuing processing
TTUQ2b1x120.10.2026 06:02:49.274 Cam-08-Q2b1x1 ERRORlog0.02022.40/0ERROR: large change in astrometric-star counts between the two new images (q3: 803 -> 1006, 20.179% > 20%; fd_Cam-08-Q2b1x1_2026-10-20_01-01-54_20.00sec_-0.00C_LIGHT_0057.fits vs fd_Cam-08-Q2b1x1_2026-10-20_01-02-49_20.00sec_-0.00C_LIGHT_0058.fits) - usually a bad plate solution on one of them, sometimes stars crossing a quadrant boundary when the two images are widely offset, rarely a transparency change; continuing processing
TTUQ2b1x120.10.2026 06:06:02.419 Cas-05-Q2b1x1 OKlog0.029315.52.30/0
TTUQ2b1x120.10.2026 06:09:10.987 Per-01-Q2b1x1 OKlog0.031015.42.30/0
TTUQ2b1x120.10.2026 06:12:26.056 Cam-11-Q2b1x1 OKlog0.009515.32.40/0
TTUQ2b1x120.10.2026 06:00:58.589 Cas-03-Q2b1x1 ERRORlog0.01442.40/0ERROR: large change in astrometric-star counts between the two new images (q3: 499 -> 923, 45.937% > 20%; fd_Cas-03-Q2b1x1_2026-10-20_01-00-13_20.00sec_-0.00C_LIGHT_0055.fits vs fd_Cas-03-Q2b1x1_2026-10-20_01-00-58_20.00sec_-0.00C_LIGHT_0056.fits) - usually a bad plate solution on one of them, sometimes stars crossing a quadrant boundary when the two images are widely offset, rarely a transparency change; continuing processing
TTUQ2b1x120.10.2026 06:04:04.878 Cam-08-Q2b1x1 ERRORlog0.02322.40/0ERROR: large change in astrometric-star counts between the two new images (q2: 1033 -> 807, 21.878% > 20%; fd_Cam-08-Q2b1x1_2026-10-20_01-03-15_20.00sec_-0.00C_LIGHT_0059.fits vs fd_Cam-08-Q2b1x1_2026-10-20_01-04-04_20.00sec_-0.00C_LIGHT_0060.fits) - usually a bad plate solution on one of them, sometimes stars crossing a quadrant boundary when the two images are widely offset, rarely a transparency change; continuing processing
TTUQ2b1x120.10.2026 06:07:24.723 Cas-05-Q2b1x1 OKlog0.030515.52.20/0
TTUQ2b1x120.10.2026 06:10:25.604 Per-01-Q2b1x1 OKlog0.037415.42.30/0
TTUQ2b1x120.10.2026 06:14:02.586 Cam-11-Q2b1x1 OKlog0.009615.32.40/0
TTUQ2b1x120.10.2026 06:18:18.775 Per-02-Q2b1x1 OKlog0.020215.32.40/0
TTUQ2b1x120.10.2026 06:21:19.308 Per-03-Q2b1x1 OKlog0.003815.22.52/2
TTUQ2b1x120.10.2026 06:24:11.746 Per-05-Q2b1x1 ERRORlog0.01382.50/0ERROR: large change in astrometric-star counts between the two new images (q1: 1703 -> 1031, 39.460% > 20%; fd_Per-05-Q2b1x1_2026-10-20_01-23-26_20.00sec_0.00C_LIGHT_0081.fits vs fd_Per-05-Q2b1x1_2026-10-20_01-24-11_20.00sec_-0.00C_LIGHT_0082.fits) - usually a bad plate solution on one of them, sometimes stars crossing a quadrant boundary when the two images are widely offset, rarely a transparency change; continuing processing
TTUQ2b1x120.10.2026 06:26:50.789 Aur-03-Q2b1x1 ERRORlog0.00462.50/2ERROR: large change in astrometric-star counts between the two new images (q4: 869 -> 582, 33.026% > 20%; fd_Aur-03-Q2b1x1_2026-10-20_01-26-12_20.00sec_-0.00C_LIGHT_0085.fits vs fd_Aur-03-Q2b1x1_2026-10-20_01-26-50_20.00sec_-0.00C_LIGHT_0086.fits) - usually a bad plate solution on one of them, sometimes stars crossing a quadrant boundary when the two images are widely offset, rarely a transparency change; continuing processing
TTUQ2b1x120.10.2026 06:19:42.585 Per-02-Q2b1x1 OKlog0.025015.22.30/0
TTUQ2b1x120.10.2026 06:22:33.651 Per-03-Q2b1x1 ERRORlog0.01142.70/0ERROR: large change in astrometric-star counts between the two new images (q3: 984 -> 646, 34.350% > 20%; fd_Per-03-Q2b1x1_2026-10-20_01-21-46_20.00sec_-0.00C_LIGHT_0079.fits vs fd_Per-03-Q2b1x1_2026-10-20_01-22-33_20.00sec_-0.00C_LIGHT_0080.fits) - usually a bad plate solution on one of them, sometimes stars crossing a quadrant boundary when the two images are widely offset, rarely a transparency change; continuing processing
TTUQ2b1x120.10.2026 06:24:37.498 Per-05-Q2b1x1 ERRORlog0.01220/0***** IMAGE PROCESSING ERROR (less than 4 images processed) *****
TTUQ2b1x120.10.2026 06:27:58.489 Aur-03-Q2b1x1 ERRORlog0.01172.50/1ERROR: large change in astrometric-star counts between the two new images (q1: 1487 -> 922, 37.996% > 20%; fd_Aur-03-Q2b1x1_2026-10-20_01-27-16_20.00sec_-0.00C_LIGHT_0087.fits vs fd_Aur-03-Q2b1x1_2026-10-20_01-27-58_20.00sec_-0.00C_LIGHT_0088.fits) - usually a bad plate solution on one of them, sometimes stars crossing a quadrant boundary when the two images are widely offset, rarely a transparency change; continuing processing
TTUQ2b1x120.10.2026 06:45:02.509 Aur-05-Q2b1x1 ERRORlogERROR0/0***** IMAGE PROCESSING ERROR (less than 4 images processed) *****
TTUQ2b1x120.10.2026 06:46:34.219 Aur-05-Q2b1x1 ERRORlogERROR0/0***** IMAGE PROCESSING ERROR (less than 4 images processed) *****
TTUQ2b1x120.10.2026 06:48:13.801 Aur-06-Q2b1x1 ERRORlog0.07222.40/1ERROR: large change in astrometric-star counts between the two new images (q1: 1248 -> 337, 72.997% > 20%; fd_Aur-06-Q2b1x1_2026-10-20_01-47-14_20.00sec_-0.00C_LIGHT_0093.fits vs fd_Aur-06-Q2b1x1_2026-10-20_01-48-13_20.00sec_-0.00C_LIGHT_0094.fits) - usually a bad plate solution on one of them, sometimes stars crossing a quadrant boundary when the two images are widely offset, rarely a transparency change; continuing processing
TTUQ2b1x120.10.2026 06:49:22.836 Aur-06-Q2b1x1 ERRORlog0.07212.50/1ERROR: large change in astrometric-star counts between the two new images (q1: 663 -> 1290, 48.605% > 20%; fd_Aur-06-Q2b1x1_2026-10-20_01-48-39_20.00sec_-0.00C_LIGHT_0095.fits vs fd_Aur-06-Q2b1x1_2026-10-20_01-49-22_20.00sec_0.00C_LIGHT_0096.fits) - usually a bad plate solution on one of them, sometimes stars crossing a quadrant boundary when the two images are widely offset, rarely a transparency change; continuing processing
TTUQ2b1x120.10.2026 06:50:56.656 Tau-04-Q2b1x1 ERRORlog0.10172.90/0ERROR: large change in astrometric-star counts between the two new images (q1: 604 -> 478, 20.861% > 20%; fd_Tau-04-Q2b1x1_2026-10-20_01-50-01_20.00sec_-0.00C_LIGHT_0097.fits vs fd_Tau-04-Q2b1x1_2026-10-20_01-50-56_20.00sec_0.00C_LIGHT_0098.fits) - usually a bad plate solution on one of them, sometimes stars crossing a quadrant boundary when the two images are widely offset, rarely a transparency change; continuing processing
TTUQ2b1x120.10.2026 06:51:22.171 Tau-04-Q2b1x1 ERRORlogERROR0/0ERROR: passing clouds (SD ratio=0.271 hard threshold=0.18)
TTUQ2b1x120.10.2026 06:54:37.756 Gem-03-Q2b1x1 ERRORlog0.02072.40/4ERROR: large change in astrometric-star counts between the two new images (q2: 660 -> 868, 23.963% > 20%; fd_Gem-03-Q2b1x1_2026-10-20_01-53-28_20.00sec_-0.00C_LIGHT_0101.fits vs fd_Gem-03-Q2b1x1_2026-10-20_01-54-37_20.00sec_-0.00C_LIGHT_0102.fits) - usually a bad plate solution on one of them, sometimes stars crossing a quadrant boundary when the two images are widely offset, rarely a transparency change; continuing processing
TTUQ2b1x120.10.2026 06:56:05.857 Ori-02-Q2b1x1 ERRORlog0.06172.40/2ERROR: large change in astrometric-star counts between the two new images (q4: 964 -> 674, 30.083% > 20%; fd_Ori-02-Q2b1x1_2026-10-20_01-55-16_20.00sec_-0.00C_LIGHT_0103.fits vs fd_Ori-02-Q2b1x1_2026-10-20_01-56-05_20.00sec_-0.00C_LIGHT_0104.fits) - usually a bad plate solution on one of them, sometimes stars crossing a quadrant boundary when the two images are widely offset, rarely a transparency change; continuing processing
TTUQ2b1x120.10.2026 06:57:37.971 Gem-05-Q2b1x1 OKlog0.068714.62.40/1
TTUQ2b1x120.10.2026 06:59:26.825 Ori-04-Q2b1x1 ERRORlog0.01602.50/0ERROR: large change in astrometric-star counts between the two new images (q1: 1038 -> 759, 26.879% > 20%; fd_Ori-04-Q2b1x1_2026-10-20_01-58-32_20.00sec_-0.00C_LIGHT_0107.fits vs fd_Ori-04-Q2b1x1_2026-10-20_01-59-26_20.00sec_0.00C_LIGHT_0108.fits) - usually a bad plate solution on one of them, sometimes stars crossing a quadrant boundary when the two images are widely offset, rarely a transparency change; continuing processing
TTUQ2b1x120.10.2026 07:00:48.575 Mon-01-Q2b1x1 OKlog0.040014.52.40/0
TTUQ2b1x120.10.2026 07:05:06.843 Mon-02-Q2b1x1 OKlog0.101314.42.30/0
TTUQ2b1x120.10.2026 07:03:01.691 Aqr-07-Q2b1x1 OKlog0.021114.62.50/4
TTUQ2b1x120.10.2026 07:09:03.290 Peg-08-Q2b1x1 OKlog0.049314.92.40/0
TTUQ2b1x120.10.2026 07:07:28.762 Equ-01-Q2b1x1 OKlog0.015414.72.40/0
TTUQ2b1x120.10.2026 07:10:34.216 Aqr-05-Q2b1x1 ERRORlog0.13752.30/4ERROR: large change in astrometric-star counts between the two new images (q2: 361 -> 190, 47.368% > 20%; fd_Aqr-05-Q2b1x1_2026-10-20_02-09-45_20.00sec_-0.00C_LIGHT_0119.fits vs fd_Aqr-05-Q2b1x1_2026-10-20_02-10-34_20.00sec_0.00C_LIGHT_0120.fits) - usually a bad plate solution on one of them, sometimes stars crossing a quadrant boundary when the two images are widely offset, rarely a transparency change; continuing processing
TTUQ2b1x120.10.2026 07:15:50.772 For-01-Q2b1x1 ERRORlog0.02732.80/0ERROR: large change in astrometric-star counts between the two new images (q1: 99 -> 152, 34.868% > 20%; fd_For-01-Q2b1x1_2026-10-20_02-14-59_20.00sec_-0.00C_LIGHT_0121.fits vs fd_For-01-Q2b1x1_2026-10-20_02-15-50_20.00sec_0.00C_LIGHT_0122.fits) - usually a bad plate solution on one of them, sometimes stars crossing a quadrant boundary when the two images are widely offset, rarely a transparency change; continuing processing
TTUQ2b1x120.10.2026 07:17:40.162 Vul-03-Q2b1x1 OKlog0.011515.02.50/0
TTUQ2b1x120.10.2026 07:21:34.804 Aqr-02-Q2b1x1 OKlog0.011914.92.30/1
TTUQ2b1x120.10.2026 07:24:16.268 For-03-Q2b1x1   —  ERRORlogERROR0/0ERROR: too few refereence images for the field For-03-Q2b1x1
TTUQ2b1x120.10.2026 07:23:06.052 Cyg-09-Q2b1x1 OKlog0.046215.02.50/0
TTUQ2b1x120.10.2026 07:26:56.447 Dra-08-Q2b1x1 OKlog0.014414.92.50/1
TTUQ2b1x120.10.2026 07:29:00.496 Mon-05-Q2b1x1 ERRORlog0.02532.90/0ERROR: large change in astrometric-star counts between the two new images (q2: 67 -> 115, 41.739% > 20%; fd_Mon-05-Q2b1x1_2026-10-20_02-28-13_20.00sec_-0.00C_LIGHT_0133.fits vs fd_Mon-05-Q2b1x1_2026-10-20_02-29-00_20.00sec_-0.00C_LIGHT_0134.fits) - usually a bad plate solution on one of them, sometimes stars crossing a quadrant boundary when the two images are widely offset, rarely a transparency change; continuing processing
TTUQ2b1x120.10.2026 07:31:00.339 Cyg-01-Q2b1x1 OKlog0.018314.92.60/0
TTUQ2b1x120.10.2026 07:32:43.719 Dra-04-Q2b1x1 OKlog0.023714.82.40/0
TTUQ2b1x120.10.2026 07:34:14.849 Peg-11-Q2b1x1 OKlog0.052815.12.40/2
TTUQ2b1x120.10.2026 07:36:01.341 Cet-09-Q2b1x1 ERRORlog0.02422.60/0ERROR: large change in astrometric-star counts between the two new images (q4: 156 -> 197, 20.812% > 20%; fd_Cet-09-Q2b1x1_2026-10-20_02-35-15_20.00sec_-0.00C_LIGHT_0141.fits vs fd_Cet-09-Q2b1x1_2026-10-20_02-36-01_20.00sec_-0.00C_LIGHT_0142.fits) - usually a bad plate solution on one of them, sometimes stars crossing a quadrant boundary when the two images are widely offset, rarely a transparency change; continuing processing
TTUQ2b1x120.10.2026 07:37:25.777 Peg-09-Q2b1x1 ERRORlog0.07332.50/0ERROR: large change in astrometric-star counts between the two new images (q2: 461 -> 292, 36.659% > 20%; fd_Peg-09-Q2b1x1_2026-10-20_02-36-44_20.00sec_-0.00C_LIGHT_0143.fits vs fd_Peg-09-Q2b1x1_2026-10-20_02-37-25_20.00sec_-0.00C_LIGHT_0144.fits) - usually a bad plate solution on one of them, sometimes stars crossing a quadrant boundary when the two images are widely offset, rarely a transparency change; continuing processing
TTUQ2b1x120.10.2026 07:40:33.231 Psc-09-Q2b1x1 OKlog0.016815.12.40/7
TTUQ2b1x120.10.2026 07:38:53.788 Cet-05-Q2b1x1 ERRORlog0.08772.90/2ERROR: large change in astrometric-star counts between the two new images (q4: 340 -> 243, 28.529% > 20%; fd_Cet-05-Q2b1x1_2026-10-20_02-38-08_20.00sec_-0.00C_LIGHT_0145.fits vs fd_Cet-05-Q2b1x1_2026-10-20_02-38-53_20.00sec_-0.00C_LIGHT_0146.fits) - usually a bad plate solution on one of them, sometimes stars crossing a quadrant boundary when the two images are widely offset, rarely a transparency change; continuing processing
TTUQ2b1x120.10.2026 07:42:09.031 Peg-05-Q2b1x1 OKlog0.004615.22.50/0
TTUQ2b1x120.10.2026 07:44:48.894 For-02-Q2b1x1 ERRORlog0.03972.80/0ERROR: large change in astrometric-star counts between the two new images (q1: 285 -> 368, 22.554% > 20%; fd_For-02-Q2b1x1_2026-10-20_02-43-38_20.00sec_-0.00C_LIGHT_0151.fits vs fd_For-02-Q2b1x1_2026-10-20_02-44-48_20.00sec_0.00C_LIGHT_0152.fits) - usually a bad plate solution on one of them, sometimes stars crossing a quadrant boundary when the two images are widely offset, rarely a transparency change; continuing processing
TTUQ2b1x120.10.2026 07:47:10.734 Peg-02-Q2b1x1 ERRORlog0.04492.80/0ERROR: large change in astrometric-star counts between the two new images (q2: 1033 -> 788, 23.717% > 20%; fd_Peg-02-Q2b1x1_2026-10-20_02-45-55_20.00sec_-0.00C_LIGHT_0153.fits vs fd_Peg-02-Q2b1x1_2026-10-20_02-47-10_20.00sec_-0.00C_LIGHT_0154.fits) - usually a bad plate solution on one of them, sometimes stars crossing a quadrant boundary when the two images are widely offset, rarely a transparency change; continuing processing
TTUQ2b1x120.10.2026 07:48:47.326 Psc-07-Q2b1x1 OKlog0.100015.22.50/4
TTUQ2b1x120.10.2026 07:51:05.436 For-04-Q2b1x1 ERRORlog0.00972.70/0ERROR: large change in astrometric-star counts between the two new images (q1: 94 -> 58, 38.298% > 20%; fd_For-04-Q2b1x1_2026-10-20_02-50-21_20.00sec_-0.00C_LIGHT_0157.fits vs fd_For-04-Q2b1x1_2026-10-20_02-51-05_20.00sec_-0.00C_LIGHT_0158.fits) - usually a bad plate solution on one of them, sometimes stars crossing a quadrant boundary when the two images are widely offset, rarely a transparency change; continuing processing
TTUQ2b1x120.10.2026 07:52:36.625 Cet-10-Q2b1x1 ERRORlogERROR0/0ERROR: passing clouds (SD ratio=0.230 hard threshold=0.18)
TTUQ2b1x120.10.2026 07:54:56.046 Cyg-07-Q2b1x1 ERRORlog0.10352.90/0ERROR: large change in astrometric-star counts between the two new images (q2: 9 -> 104, 91.346% > 20%; fd_Cyg-07-Q2b1x1_2026-10-20_02-54-08_20.00sec_-0.00C_LIGHT_0161.fits vs fd_Cyg-07-Q2b1x1_2026-10-20_02-54-56_20.00sec_0.00C_LIGHT_0162.fits) - usually a bad plate solution on one of them, sometimes stars crossing a quadrant boundary when the two images are widely offset, rarely a transparency change; continuing processing
TTUQ2b1x120.10.2026 07:56:35.983 Peg-10-Q2b1x1 OKlog0.015215.32.30/2
TTUQ2b1x120.10.2026 07:59:34.532 Psc-08-Q2b1x1 ERRORlogERROR0/0***** IMAGE PROCESSING ERROR (less than 4 images processed) *****
TTUQ2b1x120.10.2026 07:58:26.118 Cet-06-Q2b1x1 ERRORlog0.01802.70/2ERROR: large change in astrometric-star counts between the two new images (q1: 439 -> 190, 56.720% > 20%; fd_Cet-06-Q2b1x1_2026-10-20_02-57-32_20.00sec_-0.00C_LIGHT_0165.fits vs fd_Cet-06-Q2b1x1_2026-10-20_02-58-26_20.00sec_-0.00C_LIGHT_0166.fits) - usually a bad plate solution on one of them, sometimes stars crossing a quadrant boundary when the two images are widely offset, rarely a transparency change; continuing processing
TTUQ2b1x120.10.2026 08:04:16 Eri-08-Q2b1x1 ERRORlog0.01003.20/0ERROR: large change in astrometric-star counts between the two new images (q2: 196 -> 311, 36.977% > 20%; fd_Eri-08-Q2b1x1_2026-10-20_03-03-19_20.00sec_-0.00C_LIGHT_0171.fits vs fd_Eri-08-Q2b1x1_2026-10-20_03-04-16_20.00sec_-0.00C_LIGHT_0172.fits) - usually a bad plate solution on one of them, sometimes stars crossing a quadrant boundary when the two images are widely offset, rarely a transparency change; continuing processing
TTUQ2b1x120.10.2026 08:01:54.069 Peg-06-Q2b1x1 ERRORlog0.07002.40/3ERROR: large change in astrometric-star counts between the two new images (q2: 851 -> 633, 25.617% > 20%; fd_Peg-06-Q2b1x1_2026-10-20_03-01-03_20.00sec_-0.00C_LIGHT_0169.fits vs fd_Peg-06-Q2b1x1_2026-10-20_03-01-54_20.00sec_-0.00C_LIGHT_0170.fits) - usually a bad plate solution on one of them, sometimes stars crossing a quadrant boundary when the two images are widely offset, rarely a transparency change; continuing processing
TTUQ2b1x120.10.2026 08:08:59.755 Cep-05-Q2b1x1 ERRORlog0.01872.30/0ERROR: large change in astrometric-star counts between the two new images (q3: 1175 -> 688, 41.447% > 20%; fd_Cep-05-Q2b1x1_2026-10-20_03-07-44_20.00sec_-0.00C_LIGHT_0173.fits vs fd_Cep-05-Q2b1x1_2026-10-20_03-08-59_20.00sec_0.00C_LIGHT_0174.fits) - usually a bad plate solution on one of them, sometimes stars crossing a quadrant boundary when the two images are widely offset, rarely a transparency change; continuing processing
TTUQ2b1x120.10.2026 08:10:38.406 Psc-04-Q2b1x1 ERRORlog0.07272.30/3ERROR: large change in astrometric-star counts between the two new images (q1: 387 -> 636, 39.151% > 20%; fd_Psc-04-Q2b1x1_2026-10-20_03-09-46_20.00sec_-0.00C_LIGHT_0175.fits vs fd_Psc-04-Q2b1x1_2026-10-20_03-10-38_20.00sec_0.00C_LIGHT_0176.fits) - usually a bad plate solution on one of them, sometimes stars crossing a quadrant boundary when the two images are widely offset, rarely a transparency change; continuing processing
TTUQ2b1x120.10.2026 08:12:58.564 Peg-03-Q2b1x1 OKlog0.026715.42.40/0
TTUQ2b1x120.10.2026 08:22:09.353 CMa-02-Q2b1x1 ERRORlogERROR0/0***** IMAGE PROCESSING ERROR (less than 4 images processed) *****
TTUQ2b1x120.10.2026 08:26:41.857 Mon-06-Q2b1x1 ERRORlog0.05712.40/0***** IMAGE PROCESSING ERROR (less than 4 images processed) *****
TTUQ2b1x120.10.2026 08:28:57.523 Cet-11-Q2b1x1 ERRORlog0.01602.40/0ERROR: large change in astrometric-star counts between the two new images (q3: 211 -> 122, 42.180% > 20%; fd_Cet-11-Q2b1x1_2026-10-20_03-28-08_20.00sec_-0.00C_LIGHT_0183.fits vs fd_Cet-11-Q2b1x1_2026-10-20_03-28-57_20.00sec_-0.00C_LIGHT_0184.fits) - usually a bad plate solution on one of them, sometimes stars crossing a quadrant boundary when the two images are widely offset, rarely a transparency change; continuing processing
TTUQ2b1x120.10.2026 08:31:18.607 Eri-10-Q2b1x1 ERRORlog0.01132.40/0ERROR: large change in astrometric-star counts between the two new images (q2: 227 -> 288, 21.181% > 20%; fd_Eri-10-Q2b1x1_2026-10-20_03-30-34_20.00sec_-0.00C_LIGHT_0185.fits vs fd_Eri-10-Q2b1x1_2026-10-20_03-31-18_20.00sec_0.00C_LIGHT_0186.fits) - usually a bad plate solution on one of them, sometimes stars crossing a quadrant boundary when the two images are widely offset, rarely a transparency change; continuing processing
TTUQ2b1x120.10.2026 08:37:01.855 Lac-03-Q2b1x1 ERRORlog0.10232.70/0ERROR: large change in astrometric-star counts between the two new images (q1: 534 -> 1375, 61.164% > 20%; fd_Lac-03-Q2b1x1_2026-10-20_03-36-08_20.00sec_0.00C_LIGHT_0187.fits vs fd_Lac-03-Q2b1x1_2026-10-20_03-37-01_20.00sec_-0.00C_LIGHT_0188.fits) - usually a bad plate solution on one of them, sometimes stars crossing a quadrant boundary when the two images are widely offset, rarely a transparency change; continuing processing
TTUQ2b1x120.10.2026 09:11:12.823 Peg-07-Q2b1x1 OKlog0.069615.22.30/3
TTUQ2b1x120.10.2026 09:17:33.646 Pup-01-Q2b1x1 OKlog0.045014.12.40/1
TTUQ2b1x120.10.2026 09:19:40.733 Cet-07-Q2b1x1 OKlog0.021215.12.30/5
TTUQ2b1x120.10.2026 09:21:25.944 Cet-02-Q2b1x1 OKlog0.007015.02.30/8
TTUQ2b1x120.10.2026 09:23:26.042 Dra-05-Q2b1x1 OKlog0.025614.92.20/0
TTUQ2b1x120.10.2026 09:27:14.542 Lac-02-Q2b1x1 ERRORlog0.04142.40/0ERROR: large change in astrometric-star counts between the two new images (q1: 1665 -> 1230, 26.126% > 20%; fd_Lac-02-Q2b1x1_2026-10-20_04-26-30_20.00sec_-0.00C_LIGHT_0201.fits vs fd_Lac-02-Q2b1x1_2026-10-20_04-27-14_20.00sec_-0.00C_LIGHT_0202.fits) - usually a bad plate solution on one of them, sometimes stars crossing a quadrant boundary when the two images are widely offset, rarely a transparency change; continuing processing
TTUQ2b1x120.10.2026 09:25:25.788 Pup-02-Q2b1x1 OKlog0.059213.92.30/0
TTUQ2b1x120.10.2026 09:28:41.666 Peg-04-Q2b1x1 ERRORlog0.01712.50/0ERROR: large change in astrometric-star counts between the two new images (q3: 736 -> 566, 23.098% > 20%; fd_Peg-04-Q2b1x1_2026-10-20_04-27-56_20.00sec_-0.00C_LIGHT_0203.fits vs fd_Peg-04-Q2b1x1_2026-10-20_04-28-41_20.00sec_-0.00C_LIGHT_0204.fits) - usually a bad plate solution on one of them, sometimes stars crossing a quadrant boundary when the two images are widely offset, rarely a transparency change; continuing processing
TTUQ2b1x120.10.2026 09:30:05.876 Eri-09-Q2b1x1 ERRORlogERROR0/0ERROR: passing clouds (SD ratio=0.226 hard threshold=0.18)
TTUQ2b1x120.10.2026 09:49:17.881 Psc-05-Q2b1x1 ERRORlog0.09642.50/0ERROR: large change in astrometric-star counts between the two new images (q1: 292 -> 495, 41.010% > 20%; fd_Psc-05-Q2b1x1_2026-10-20_04-48-19_20.00sec_-0.00C_LIGHT_0207.fits vs fd_Psc-05-Q2b1x1_2026-10-20_04-49-17_20.00sec_-0.00C_LIGHT_0208.fits) - usually a bad plate solution on one of them, sometimes stars crossing a quadrant boundary when the two images are widely offset, rarely a transparency change; continuing processing
TTUQ2b1x120.10.2026 09:51:35.120 Cet-12-Q2b1x1 ERRORlog0.02002.50/0ERROR: large change in astrometric-star counts between the two new images (q2: 23 -> 79, 70.886% > 20%; fd_Cet-12-Q2b1x1_2026-10-20_04-50-43_20.00sec_-0.00C_LIGHT_0209.fits vs fd_Cet-12-Q2b1x1_2026-10-20_04-51-35_20.00sec_-0.00C_LIGHT_0210.fits) - usually a bad plate solution on one of them, sometimes stars crossing a quadrant boundary when the two images are widely offset, rarely a transparency change; continuing processing
TTUQ2b1x120.10.2026 09:53:16.324 Peg-01-Q2b1x1 ERRORlog0.05972.40/0ERROR: large change in astrometric-star counts between the two new images (q4: 588 -> 239, 59.354% > 20%; fd_Peg-01-Q2b1x1_2026-10-20_04-52-20_20.00sec_-0.00C_LIGHT_0211.fits vs fd_Peg-01-Q2b1x1_2026-10-20_04-53-16_20.00sec_-0.00C_LIGHT_0212.fits) - usually a bad plate solution on one of them, sometimes stars crossing a quadrant boundary when the two images are widely offset, rarely a transparency change; continuing processing
TTUQ2b1x120.10.2026 09:55:37.225 Pup-03-Q2b1x1 ERRORlog0.01702.50/0ERROR: large change in astrometric-star counts between the two new images (q3: 196 -> 252, 22.222% > 20%; fd_Pup-03-Q2b1x1_2026-10-20_04-54-43_20.00sec_-0.00C_LIGHT_0213.fits vs fd_Pup-03-Q2b1x1_2026-10-20_04-55-37_20.00sec_0.00C_LIGHT_0214.fits) - usually a bad plate solution on one of them, sometimes stars crossing a quadrant boundary when the two images are widely offset, rarely a transparency change; continuing processing
TTUQ2b1x120.10.2026 09:57:54.009 Psc-02-Q2b1x1 OKlog0.012315.32.30/2
TTUQ2b1x120.10.2026 10:00:20.647 Col-01-Q2b1x1 ERRORlog0.01372.30/0ERROR: large change in astrometric-star counts between the two new images (q1: 85 -> 114, 25.439% > 20%; fd_Col-01-Q2b1x1_2026-10-20_04-59-24_20.00sec_-0.00C_LIGHT_0217.fits vs fd_Col-01-Q2b1x1_2026-10-20_05-00-20_20.00sec_0.00C_LIGHT_0218.fits) - usually a bad plate solution on one of them, sometimes stars crossing a quadrant boundary when the two images are widely offset, rarely a transparency change; continuing processing
TTUQ2b1x120.10.2026 10:02:22.792 Cet-08-Q2b1x1 OKlog0.022915.22.30/1
TTUQ2b1x120.10.2026 10:04:17.048 Cet-03-Q2b1x1 OKlog0.051715.12.30/3
TTUQ2b1x120.10.2026 10:06:01.828 And-04-Q2b1x1 OKlog0.080615.32.40/0
TTUQ2b1x120.10.2026 10:07:50.369 And-07-Q2b1x1 OKlog0.056015.32.30/7
TTUQ2b1x120.10.2026 10:09:32.745 Psc-06-Q2b1x1 OKlog0.070315.22.30/4
TTUQ2b1x120.10.2026 10:14:19.020 Lep-02-Q2b1x1 OKlog0.010314.82.40/0
TTUQ2b1x120.10.2026 10:15:34.656 Eri-06-Q2b1x1 ERRORlogERROR0/0ERROR: passing clouds (SD ratio=0.262 hard threshold=0.18)
TTUQ2b1x120.10.2026 10:21:42.629 And-01-Q2b1x1 OKlog0.079015.32.40/0
TTUQ2b1x120.10.2026 10:26:23.394 Pyx-01-Q2b1x1 ERRORlog0.01832.80/0ERROR: large change in astrometric-star counts between the two new images (q1: 226 -> 101, 55.310% > 20%; fd_Pyx-01-Q2b1x1_2026-10-20_05-25-19_20.00sec_-0.00C_LIGHT_0235.fits vs fd_Pyx-01-Q2b1x1_2026-10-20_05-26-23_20.00sec_-0.00C_LIGHT_0236.fits) - usually a bad plate solution on one of them, sometimes stars crossing a quadrant boundary when the two images are widely offset, rarely a transparency change; continuing processing
TTUQ2b1x120.10.2026 10:28:18.011 Psc-01-Q2b1x1 OKlog0.041515.32.50/1
TTUQ2b1x120.10.2026 10:30:04.985 Psc-03-Q2b1x1 OKlog0.014915.22.40/5
TTUQ2b1x120.10.2026 10:30:46.973 Eri-03-Q2b1x1 ERRORlogERROR0/0ERROR: passing clouds (SD ratio=0.199 hard threshold=0.18)
TTUQ2b1x120.10.2026 10:34:09.026 Cet-04-Q2b1x1 OKlog0.014214.82.40/4
TTUQ2b1x120.10.2026 10:45:58.487 Col-02-Q2b1x1 ERRORlog0.02592.50/0ERROR: large change in astrometric-star counts between the two new images (q4: 43 -> 94, 54.255% > 20%; fd_Col-02-Q2b1x1_2026-10-20_05-42-00_20.00sec_-0.00C_LIGHT_0245.fits vs fd_Col-02-Q2b1x1_2026-10-20_05-45-58_20.00sec_-0.00C_LIGHT_0246.fits) - usually a bad plate solution on one of them, sometimes stars crossing a quadrant boundary when the two images are widely offset, rarely a transparency change; continuing processing
TTUQ2b1x120.10.2026 10:47:04.829 And-05-Q2b1x1 ERRORlogERROR0/0***** IMAGE PROCESSING ERROR (less than 4 images processed) *****
TTUQ2b1x120.10.2026 10:49:27.485 Ari-02-Q2b1x1 ERRORlog0.08103.31/5ERROR: large change in astrometric-star counts between the two new images (q2: 678 -> 495, 26.991% > 20%; fd_Ari-02-Q2b1x1_2026-10-20_05-48-34_20.00sec_-0.00C_LIGHT_0249.fits vs fd_Ari-02-Q2b1x1_2026-10-20_05-49-27_20.00sec_0.00C_LIGHT_0250.fits) - usually a bad plate solution on one of them, sometimes stars crossing a quadrant boundary when the two images are widely offset, rarely a transparency change; continuing processing
TTUQ2b1x120.10.2026 10:50:07.003 Cet-01-Q2b1x1 ERRORlogERROR0/0ERROR: passing clouds (SD ratio=0.192 hard threshold=0.18)
TTUQ2b1x120.10.2026 11:50:20.433 CMa-03-Q2b1x1 ERRORlog0.02622.30/0ERROR: large change in astrometric-star counts between the two new images (q3: 480 -> 202, 57.917% > 20%; fd_CMa-03-Q2b1x1_2026-10-20_06-49-26_20.00sec_-0.00C_LIGHT_0253.fits vs fd_CMa-03-Q2b1x1_2026-10-20_06-50-20_20.00sec_-0.00C_LIGHT_0254.fits) - usually a bad plate solution on one of them, sometimes stars crossing a quadrant boundary when the two images are widely offset, rarely a transparency change; continuing processing
TTUQ2b1x120.10.2026 11:52:44.451 Pup-04-Q2b1x1 ERRORlog0.01462.50/0ERROR: large change in astrometric-star counts between the two new images (q1: 286 -> 211, 26.224% > 20%; fd_Pup-04-Q2b1x1_2026-10-20_06-51-55_20.00sec_-0.00C_LIGHT_0255.fits vs fd_Pup-04-Q2b1x1_2026-10-20_06-52-44_20.00sec_-0.00C_LIGHT_0256.fits) - usually a bad plate solution on one of them, sometimes stars crossing a quadrant boundary when the two images are widely offset, rarely a transparency change; continuing processing
TTUQ2b1x120.10.2026 12:14:10.098 Eri-07-Q2b1x1 ERRORlog0.01022.40/0ERROR: large change in astrometric-star counts between the two new images (q4: 121 -> 90, 25.620% > 20%; fd_Eri-07-Q2b1x1_2026-10-20_07-13-26_20.00sec_-0.00C_LIGHT_0257.fits vs fd_Eri-07-Q2b1x1_2026-10-20_07-14-10_20.00sec_-0.00C_LIGHT_0258.fits) - usually a bad plate solution on one of them, sometimes stars crossing a quadrant boundary when the two images are widely offset, rarely a transparency change; continuing processing
TTUQ2b1x120.10.2026 12:15:29.047 Eri-04-Q2b1x1 ERRORlog0.11832.40/0ERROR: passing clouds (SD ratio=0.166 soft threshold=0.12)