ePESSTO+ Year 3+4 - Final SOFI Imaging reduction

Summary:

The reductions of the SOFI imaging resulted in 603 images (248 J-band, 235 H-band, 120 K-band).

2021-10-04:

The SN2021jad J and H-band reduced images had some sky subtraction residuals in the default PESSTO pipeline reduction. The images were re-reduced without the illumination correction step, which appeared to improve the image quality.

2021-10-14:

The SN2021uds H-band reduced image had some sky subtraction residuals in the default PESSTO pipeline reduction. The image was re-reduced without the illumination correction step, which appeared to improve the image quality.

2021-10-14:

The SN2021zzu H-band reduced image had some sky subtraction residuals in the default PESSTO pipeline reduction. The image was re-reduced without the illumination correction step, which appeared to improve the image quality.

2021-10-25:

2021-10-26:

2021-11-06:

SN2020znr K-band imaging sequence has only 3 frames.

2021-11-11:

SN2021adcr J-band imaging sequence has only 2 frames, and the resulting reduction has major quality issues.

2021-11-11:

SN2021zny J-band imaging sequence had 2 frames followed by later during the night a full set of 4 frames, which the PESSTO pipeline originally merged together. The image was re-reduced using only the latter set, which resulted in an improved image quality.

2021-12-14:

SN2021afuq H-band reduced image had some sky subtraction residuals in the default PESSTO pipeline reduction. The image was re-reduced without the illumination correction step, which appeared to improve the image quality.

2021-12-14:

SN2021afuq J-band reduced image had some major quality issues in the first 2 exposures of the sequence of 4 frames was poor quality. The image was re-reduced with the remaining 2 frames and without illumination correction.

SOFI.2021-12-15T07:01:06.018.fits

SOFI.2021-12-15T07:01:25.725.fits

2022-01-11:

SN2018hi H-band reduced image had some sky subtraction residuals in the default PESSTO pipeline reduction. The image was re-reduced without the illumination correction step, which appeared to improve the image quality.

2022-01-11:

SN2018hle H-band reduced image had some sky subtraction residuals in the default PESSTO pipeline reduction. The image was re-reduced without the illumination correction step, which appeared to improve the image quality.

2022-01-11:

SN2021aapa H-band reduced image had some sky subtraction residuals in the default PESSTO pipeline reduction. The image was re-reduced without the illumination correction step, which appeared to improve the image quality.

2022-01-12:

SN2021jad H-band reduced image had some sky subtraction residuals in the default PESSTO pipeline reduction. The image was re-reduced without the illumination correction step, which appeared to improve the image quality.

2022-03-30:

SN2022qh JHKs-band image reductions have a major quality issue due to the raw images having every source seen in double. The observers note in the nightlog that: "TO indicated a problem with the images, but LOEM failure meant we could not inspect to comment or correct."

SOFI.2022-03-31T08:36:29.612.fits

SOFI.2022-03-31T08:36:49.281.fits

SOFI.2022-03-31T08:37:08.760.fits

SOFI.2022-03-31T08:37:28.081.fits

SOFI.2022-03-31T08:38:06.317.fits

SOFI.2022-03-31T08:38:49.661.fits

SOFI.2022-03-31T08:39:32.817.fits

SOFI.2022-03-31T08:40:16.089.fits

SOFI.2022-03-31T08:41:17.911.fits

SOFI.2022-03-31T08:42:06.659.fits

SOFI.2022-03-31T08:42:55.312.fits

SOFI.2022-03-31T08:43:43.628.fits

2022-04-21:

SN2022fie Ks-band imaging sequence has only 1 frame; therefore, this data was not reduced.

SOFI.2022-04-22T02:09:07.071.fits

2022-04-21:

SN2022esa Ks-band imaging sequence has only 1 frame; therefore, this data was not reduced.

SOFI.2022-04-22T09:31:44.218.fits

2022-04-21:

SN2022zi H-band reduced image had some sky subtraction residuals in the default PESSTO pipeline reduction. The image was re-reduced without the illumination correction step, which appeared to improve the image quality.

2022-04-22:

SN2022gor J-band imaging was obtained in two sets of frames, which resulted in two reduced images.

2022-04-22:

SN2021afuq H and J-band reduced images had some sky subtraction residuals in the default PESSTO pipeline reduction. The images were re-reduced without the illumination correction step, which appeared to improve the image quality.

2022-04-22:

SN2022fqn H-band reduced image had some sky subtraction residuals in the default PESSTO pipeline reduction. The image was re-reduced without the illumination correction step, which appeared to improve the image quality.

2022-04-22:

SN2022frl H and J-band reduced images had some sky subtraction residuals in the default PESSTO pipeline reduction. The images were re-reduced without the illumination correction step, which appeared to improve the image quality.

2022-04-23:

SN2021tkm H-band reduced image had some sky subtraction residuals in the default PESSTO pipeline reduction. The image was re-reduced without the illumination correction step, which appeared to improve the image quality.

2022-04-23:

SN2022gks H-band reduced image had some sky subtraction residuals in the default PESSTO pipeline reduction. The image was re-reduced without the illumination correction step, which appeared to improve the image quality.

2022-04-23:

SN2022gtw H-band reduced image had some sky subtraction residuals in the default PESSTO pipeline reduction. The image was re-reduced without the illumination correction step, which appeared to improve the image quality.

2022-05-22:

SN2022idx H-band reduced image had some sky subtraction residuals in the default PESSTO pipeline reduction. The image was re-reduced without the illumination correction step, which appeared to improve the image quality.

2022-05-22:

SN2022ihz H-band reduced image had some sky subtraction residuals in the default PESSTO pipeline reduction. The image was re-reduced without the illumination correction step, which appeared to improve the image quality.

2022-08-19:

SN2022qiw J-band imaging sequence has additional 2 frames before the full sequence, which cause problems for the PESSTO pipeline and were removed from the reductions.

SOFI.2022-08-20T06:36:28.201.fits

SOFI.2022-08-20T06:38:05.100.fits

2022-08-20:

SN2022qjh J-band imaging sequence of 12 exposures has a set of exposures from 6th to 10th that are very poor quality, and the image was re-reduced without the following files:

SOFI.2022-08-21T04:05:45.662.fits

SOFI.2022-08-21T04:07:22.578.fits

SOFI.2022-08-21T04:08:59.435.fits

SOFI.2022-08-21T04:10:39.480.fits

SOFI.2022-08-21T04:12:16.281.fits

2022-08-24:

SN2022qsn J-band imaging sequence has only 1 frame; therefore, this data was not reduced.

SOFI.2022-08-25T09:16:29.300.fits

2022-08-24:

SN2021aefx H-band reduced image had some sky subtraction residuals in the default PESSTO pipeline reduction. The image was re-reduced without the illumination correction step, which appeared to improve the image quality.

2022-09-02:

SN2022rld H-band reduced image had some sky subtraction residuals in the default PESSTO pipeline reduction. The image was re-reduced without the illumination correction step, which appeared to improve the image quality.

2022-09-02:

SN2022rsb H-band reduced image had some sky subtraction residuals in the default PESSTO pipeline reduction. The image was re-reduced without the illumination correction step, which appeared to improve the image quality.

2022-09-15:

All SOFI imaging observations from the night 2022-09-15 are affected by seeing all the sources in double in the raw data. The following reductions are affected:

AM0702601N_20220915_H_merge_60555_1.fits

AM0702601N_20220915_J_merge_60555_1.fits

AM0702601N_20220915_Ks_merge_60555_1.fits

AT2022dsb_20220915_J_merge_60555_1.fits

AT2022dsb_20220915_Ks_merge_60555_1.fits

AT2022rmk_20220915_H_merge_60555_1.fits

AT2022rmk_20220915_J_merge_60555_1.fits

AT2022rmk_20220915_Ks_merge_60555_1.fits

SN2021aefx_20220915_H_merge_60555_1.fits

SN2021aefx_20220915_J_merge_60555_1.fits

SN2021jad_20220915_H_merge_60555_1.fits

SN2021jad_20220915_J_merge_60555_1.fits

SN2021jad_20220915_Ks_merge_60555_1.fits

SN2022ryi_20220915_H_merge_60555_1.fits

SN2022ryi_20220915_J_merge_60555_1.fits

SN2022ryi_20220915_Ks_merge_60555_1.fits

SN2022ssj_20220915_H_merge_60555_1.fits

SN2022ssj_20220915_J_merge_60555_1.fits

SN2022ssk_20220915_H_merge_60555_1.fits

SN2022ssk_20220915_J_merge_60555_1.fits

SN2022syq_20220915_H_merge_60555_1.fits

SN2022syq_20220915_J_merge_60555_1.fits

SN2022szg_20220915_H_merge_60555_1.fits

SN2022szg_20220915_J_merge_60555_1.fits

SN2022zi_20220915_H_merge_60555_1.fits

SN2022zi_20220915_J_merge_60555_1.fits

SN2022zi_20220915_Ks_merge_60555_1.fits

2022-09-21:

SN2022ryi Ks-band reduced image had some sky subtraction residuals in the default PESSTO pipeline reduction. The image was re-reduced without the illumination correction step, which appeared to improve the image quality.

2022-10-01:

SN2021aefx J, H, and Ks-band observations have been obtained with a space in the object name of 'SN 2021aefx' in the used OB, which would cause a pipeline crash; the headers of the following raw frames were modified to remove the space:

SOFI.2022-10-02T06:35:57.032.fits

SOFI.2022-10-02T06:37:33.530.fits

SOFI.2022-10-02T06:39:10.337.fits

SOFI.2022-10-02T06:40:46.832.fits

SOFI.2022-10-02T06:42:26.027.fits

SOFI.2022-10-02T06:44:02.570.fits

SOFI.2022-10-02T06:45:39.029.fits

SOFI.2022-10-02T06:47:15.528.fits

SOFI.2022-10-02T06:48:54.979.fits

SOFI.2022-10-02T06:50:31.559.fits

SOFI.2022-10-02T06:52:08.079.fits

SOFI.2022-10-02T06:53:44.585.fits

SOFI.2022-10-02T06:55:38.931.fits

SOFI.2022-10-02T06:57:49.326.fits

SOFI.2022-10-02T07:00:00.137.fits

SOFI.2022-10-02T07:02:10.571.fits

SOFI.2022-10-02T07:04:23.881.fits

SOFI.2022-10-02T07:06:34.620.fits

SOFI.2022-10-02T07:08:45.178.fits

SOFI.2022-10-02T07:10:55.622.fits

SOFI.2022-10-02T07:13:09.029.fits

SOFI.2022-10-02T07:15:19.473.fits

SOFI.2022-10-02T07:17:29.979.fits

SOFI.2022-10-02T07:19:40.671.fits

SOFI.2022-10-02T07:22:09.279.fits

SOFI.2022-10-02T07:23:53.670.fits

SOFI.2022-10-02T07:25:38.479.fits

SOFI.2022-10-02T07:27:22.819.fits

SOFI.2022-10-02T07:29:09.278.fits

SOFI.2022-10-02T07:30:53.723.fits

SOFI.2022-10-02T07:32:38.180.fits

SOFI.2022-10-02T07:34:22.571.fits

SOFI.2022-10-02T07:36:10.128.fits

SOFI.2022-10-02T07:37:54.572.fits

SOFI.2022-10-02T07:39:39.079.fits

SOFI.2022-10-02T07:41:23.490.fits

SOFI.2022-10-02T07:43:10.429.fits

SOFI.2022-10-02T07:44:54.923.fits

SOFI.2022-10-02T07:46:39.732.fits

SOFI.2022-10-02T07:48:24.120.fits

2022-10-16:

SN2022vqz H-band imaging sequence has only 1 frame; therefore, this data was not reduced.

SOFI.2022-10-17T04:56:12.801.fits

2022-11-17:

AT2022ryi H-band reduced image had some sky subtraction residuals in the default PESSTO pipeline reduction. The image was re-reduced without the illumination correction step, which appeared to improve the image quality.

2022-11-17:

SN2022yuw H-band reduced image had some sky subtraction residuals in the default PESSTO pipeline reduction. The image was re-reduced without the illumination correction step, which appeared to improve the image quality.

2022-11-17:

SN2022ywc H-band reduced image had some sky subtraction residuals in the default PESSTO pipeline reduction. The image was re-reduced without the illumination correction step, which appeared to improve the image quality.

2022-12-20:

SN2022abdu H-band reduced image had some sky subtraction residuals in the default PESSTO pipeline reduction. The image was re-reduced without the illumination correction step, which appeared to improve the image quality.

2022-12-20:

SN2022xkq H and J-band reduced images had some sky subtraction residuals in the default PESSTO pipeline reductions. The images were re-reduced without the illumination correction step, which appeared to improve the image quality.

2022-12-28:

2022-12-20:

SN2022adcy H-band reduced image had some sky subtraction residuals in the default PESSTO pipeline reduction. The image was re-reduced without the illumination correction step, which appeared to improve the image quality.

2023-01-14:

SN2023Q J-band ON-OFF observations had 3 additional ON images in the beginning of the sequence, which were removed from the reductions to have the PESSTO pipeline function correctly.

SOFI.2023-01-15T01:23:09.280.fits

SOFI.2023-01-15T01:24:01.380.fits

SOFI.2023-01-15T01:24:53.393.fits

2023-01-14:

SN2022xxf J-band observations resulted in two reductions

SN2022xxf_20230114_J_merge_60556_1.fits

SN2022xxf_20230114_J_merge_60556_2.fits

2023-01-14:

SN2023E J-band sequence of 4 frames has prominent aircraft stripe in the following last image of the set affecting the reductions and the final image was re-reduced without it.

SOFI.2023-01-15T02:09:11.684.fits

2023-01-14:

SN2022aebc H-band reduced image had some sky subtraction residuals in the default PESSTO pipeline reduction. The image was re-reduced without the illumination correction step, which appeared to improve the image quality.

2023-01-14:

SN2023E H-band reduced image had some sky subtraction residuals in the default PESSTO pipeline reduction. The image was re-reduced without the illumination correction step, which appeared to improve the image quality.

2023-01-14:

SN2022pul H-band reduced image had some sky subtraction residuals in the default PESSTO pipeline reduction. The image was re-reduced without the illumination correction step, which appeared to improve the image quality.

2023-02-18:

SN2022qh H and J-band reduced images had some sky subtraction residuals in the default PESSTO pipeline reductions. The images were re-reduced without the illumination correction step, which appeared to improve the image quality.

2023-02-27:

SN2022eadm H-band reduced image had some sky subtraction residuals in the default PESSTO pipeline reduction. The image was re-reduced without the illumination correction step, which appeared to improve the image quality.

2023-02-27:

SN2023cjd H-band reduced image had some sky subtraction residuals in the default PESSTO pipeline reduction. The image was re-reduced without the illumination correction step, which appeared to improve the image quality.

2023-02-27:

SN2023cmf H-band reduced image had some sky subtraction residuals in the default PESSTO pipeline reduction. The image was re-reduced without the illumination correction step, which appeared to improve the image quality.

2023-04-16:

SN2022pul J, H, and Ks-band observations have been obtained with a space in the object name of 'SN 2022pul' in the used OB, which would cause a pipeline crash; the headers of the following raw frames were modified to remove the space:

SOFI.2023-04-17T02:06:19.310.fits

SOFI.2023-04-17T02:08:08.764.fits

SOFI.2023-04-17T02:09:58.052.fits

SOFI.2023-04-17T02:11:47.428.fits

SOFI.2023-04-17T02:13:53.964.fits

SOFI.2023-04-17T02:15:34.611.fits

SOFI.2023-04-17T02:17:15.203.fits

SOFI.2023-04-17T02:18:55.818.fits

SOFI.2023-04-17T02:20:53.761.fits

SOFI.2023-04-17T02:22:38.324.fits

SOFI.2023-04-17T02:24:23.107.fits

SOFI.2023-04-17T02:26:07.716.fits

SOFI.2023-04-17T02:27:53.964.fits

SOFI.2023-04-17T02:29:38.859.fits

SOFI.2023-04-17T02:31:23.352.fits

SOFI.2023-04-17T02:33:07.963.fits

2023-04-18:

SN2023cj J, H, and Ks-band observations have been obtained with a space in the object name of 'SN 2023cj' in the used OB, which would cause a pipeline crash; the headers of the following raw frames were modified to remove the space:

SOFI.2023-04-19T04:13:18.462.fits

SOFI.2023-04-19T04:14:55.363.fits

SOFI.2023-04-19T04:16:32.549.fits

SOFI.2023-04-19T04:18:09.510.fits

SOFI.2023-04-19T04:19:59.912.fits

SOFI.2023-04-19T04:21:41.700.fits

SOFI.2023-04-19T04:23:23.948.fits

SOFI.2023-04-19T04:25:06.201.fits

SOFI.2023-04-19T04:26:56.760.fits

SOFI.2023-04-19T04:28:33.810.fits

SOFI.2023-04-19T04:30:11.548.fits

SOFI.2023-04-19T04:31:48.613.fits

SOFI.2023-04-19T04:33:38.601.fits

SOFI.2023-04-19T04:35:20.551.fits

SOFI.2023-04-19T04:37:02.952.fits

SOFI.2023-04-19T04:38:45.199.fits

SOFI.2023-04-19T04:40:36.206.fits

SOFI.2023-04-19T04:42:13.261.fits

SOFI.2023-04-19T04:43:50.555.fits

SOFI.2023-04-19T04:45:27.620.fits

SOFI.2023-04-19T04:47:17.548.fits

SOFI.2023-04-19T04:48:58.902.fits

SOFI.2023-04-19T04:50:41.302.fits

SOFI.2023-04-19T04:52:24.054.fits

SOFI.2023-04-19T04:54:22.399.fits

SOFI.2023-04-19T04:57:33.670.fits

SOFI.2023-04-19T05:00:44.900.fits

SOFI.2023-04-19T05:03:55.810.fits

SOFI.2023-04-19T05:07:19.955.fits

SOFI.2023-04-19T05:10:35.200.fits

SOFI.2023-04-19T05:13:51.150.fits

SOFI.2023-04-19T05:17:07.348.fits

SOFI.2023-04-19T05:20:32.057.fits

SOFI.2023-04-19T05:23:43.111.fits

SOFI.2023-04-19T05:26:54.650.fits

SOFI.2023-04-19T05:30:05.749.fits

SOFI.2023-04-19T05:33:30.013.fits

SOFI.2023-04-19T05:36:45.460.fits

SOFI.2023-04-19T05:40:01.564.fits

SOFI.2023-04-19T05:43:17.561.fits

SOFI.2023-04-19T05:46:42.452.fits

SOFI.2023-04-19T05:49:53.462.fits

SOFI.2023-04-19T05:53:04.851.fits

SOFI.2023-04-19T05:56:16.162.fits

SOFI.2023-04-19T05:59:40.775.fits

SOFI.2023-04-19T06:02:56.359.fits

SOFI.2023-04-19T06:06:12.710.fits

SOFI.2023-04-19T06:09:28.758.fits

SOFI.2023-04-19T06:12:59.401.fits

SOFI.2023-04-19T06:14:44.199.fits

SOFI.2023-04-19T06:16:29.352.fits

SOFI.2023-04-19T06:18:14.259.fits

SOFI.2023-04-19T06:20:12.864.fits

SOFI.2023-04-19T06:22:02.164.fits

SOFI.2023-04-19T06:23:51.957.fits

SOFI.2023-04-19T06:25:42.160.fits

SOFI.2023-04-19T06:27:41.250.fits

SOFI.2023-04-19T06:29:26.811.fits

SOFI.2023-04-19T06:31:12.023.fits

SOFI.2023-04-19T06:32:56.848.fits

SOFI.2023-04-19T06:34:56.162.fits

SOFI.2023-04-19T06:36:46.459.fits

SOFI.2023-04-19T06:38:37.157.fits

SOFI.2023-04-19T06:40:27.862.fits

SOFI.2023-04-19T06:42:27.050.fits

SOFI.2023-04-19T06:44:12.100.fits

SOFI.2023-04-19T06:45:57.104.fits

SOFI.2023-04-19T06:47:42.150.fits

SOFI.2023-04-19T06:49:41.258.fits

SOFI.2023-04-19T06:51:31.510.fits

SOFI.2023-04-19T06:53:22.459.fits

SOFI.2023-04-19T06:55:17.000.fits

SOFI.2023-04-19T06:57:16.049.fits

SOFI.2023-04-19T06:59:01.300.fits

SOFI.2023-04-19T07:00:46.257.fits

SOFI.2023-04-19T07:02:31.101.fits

SOFI.2023-04-19T07:04:29.809.fits

SOFI.2023-04-19T07:06:19.812.fits

SOFI.2023-04-19T07:08:11.458.fits

SOFI.2023-04-19T07:10:02.162.fits

SOFI.2023-04-19T07:12:00.900.fits

SOFI.2023-04-19T07:13:46.462.fits

SOFI.2023-04-19T07:15:31.512.fits

SOFI.2023-04-19T07:17:16.552.fits

SOFI.2023-04-19T07:19:15.562.fits

SOFI.2023-04-19T07:21:04.761.fits

SOFI.2023-04-19T07:22:55.562.fits

SOFI.2023-04-19T07:24:45.457.fits

SOFI.2023-04-19T07:26:44.048.fits

SOFI.2023-04-19T07:28:29.481.fits

SOFI.2023-04-19T07:30:14.305.fits

SOFI.2023-04-19T07:32:00.305.fits

SOFI.2023-04-19T07:33:58.464.fits

SOFI.2023-04-19T07:35:47.961.fits

SOFI.2023-04-19T07:37:39.509.fits

SOFI.2023-04-19T07:39:29.459.fits

2023-04-18:

SN2018hfp J, and H-band observations have been obtained with a space in the object name of 'SN 2018hfp' in the used OB, which would cause a pipeline crash; the headers of the following raw frames were modified to remove the space:

SOFI.2023-04-19T07:43:21.912.fits

SOFI.2023-04-19T07:44:58.800.fits

SOFI.2023-04-19T07:46:35.311.fits

SOFI.2023-04-19T07:48:12.249.fits

SOFI.2023-04-19T07:49:52.514.fits

SOFI.2023-04-19T07:51:29.199.fits

SOFI.2023-04-19T07:53:05.821.fits

SOFI.2023-04-19T07:54:43.110.fits

SOFI.2023-04-19T07:56:23.110.fits

SOFI.2023-04-19T07:57:59.753.fits

SOFI.2023-04-19T07:59:36.361.fits

SOFI.2023-04-19T08:01:13.506.fits

SOFI.2023-04-19T08:03:09.068.fits

SOFI.2023-04-19T08:05:19.600.fits

SOFI.2023-04-19T08:07:30.112.fits

SOFI.2023-04-19T08:09:40.600.fits

SOFI.2023-04-19T08:11:54.061.fits

SOFI.2023-04-19T08:14:04.651.fits

SOFI.2023-04-19T08:16:15.160.fits

SOFI.2023-04-19T08:18:25.961.fits

SOFI.2023-04-19T08:20:39.911.fits

SOFI.2023-04-19T08:22:50.501.fits

SOFI.2023-04-19T08:25:01.172.fits

SOFI.2023-04-19T08:27:11.751.fits

2023-04-16:

AT2023bfb J-band ON-OFF imaging sequence got incorrectly merged with SN2022pul J-band sequence by the PESSTO pipeline, resulted in reducing AT2023bfb JHKs bands in a separate list.

2023-04-16:

AT2023bfb H and J-band raw images suffer from notable instrumental noise, resulting in poor quality reductions.

2023-04-16:

SN2022pul H and J-band raw images suffer from notable instrumental noise, resulting in poor quality reductions.

2023-04-18:

SN2023cj J-band raw images suffer from notable instrumental noise, resulting in a poor quality reduction.

2023-04-18:

AT2018ebu J-band reduced image had some sky subtraction residuals in the default PESSTO pipeline reduction. The image was re-reduced without the illumination correction step, which appeared to improve the image quality.

2023-04-18:

SN2018exb J-band reduced image had some sky subtraction residuals in the default PESSTO pipeline reduction. The image was re-reduced without the illumination correction step, which appeared to improve the image quality.

2023-05-19:

SOFI.2023-05-20T03:25:11.002.fits

SOFI.2023-05-20T03:27:00.221.fits

SOFI.2023-05-20T03:28:49.500.fits

SOFI.2023-05-20T03:30:38.721.fits

SOFI.2023-05-20T03:32:46.064.fits

SOFI.2023-05-20T03:34:26.473.fits

SOFI.2023-05-20T03:36:07.054.fits

SOFI.2023-05-20T03:37:47.592.fits

SOFI.2023-05-20T03:39:46.257.fits

SOFI.2023-05-20T03:41:30.628.fits

SOFI.2023-05-20T03:43:15.152.fits

SOFI.2023-05-20T03:45:00.018.fits

SOFI.2023-05-20T03:46:47.003.fits

SOFI.2023-05-20T03:48:31.372.fits

SOFI.2023-05-20T03:50:15.902.fits

SOFI.2023-05-20T03:52:00.415.fits

2023-05-19:

AT2021lwx J-band imaging sequence has only 3 frames.

2023-05-19:

AT2021lwx J-band reduced image had some sky subtraction residuals in the default PESSTO pipeline reduction. The image was re-reduced without the illumination correction step, which appeared to improve the image quality.

2023-05-19:

SN2023cj H-band reduced image had some sky subtraction residuals in the default PESSTO pipeline reduction. The image was re-reduced without the illumination correction step, which appeared to improve the image quality.

Astrometry:

Astrometry of the following reduced 70 SOFI images was re-done with the PESSTOASTRO task:

AT2021adxl_20220227_Ks_merge_60551_1.fits

AT2022jzy_20220901_J_merge_60555_1.fits

AT2022jzy_20221014_H_merge_60555_1.fits

AT2022jzy_20221014_J_merge_60555_1.fits

AT2023bfb_20230416_H_merge_60557_1.fits

AT2023bfb_20230416_J_merge_60557_1.fits

SN2018hle_20220111_H_merge_60551_1.fits

SN2021aapa_20220310_H_merge_60551_1.fits

SN2021aapa_20220310_J_merge_60551_1.fits

SN2021aapa_20220310_Ks_merge_60551_1.fits

SN2021acnz_20211228_H_merge_60551_1.fits

SN2021acnz_20211228_J_merge_60551_1.fits

SN2021aefx_20220301_H_merge_60551_1.fits

SN2021aefx_20220301_Ks_merge_60551_1.fits

SN2021aefx_20220310_H_merge_60551_1.fits

SN2021aefx_20220310_J_merge_60551_1.fits

SN2021aefx_20220310_Ks_merge_60551_1.fits

SN2021aefx_20220322_J_merge_60551_1.fits

SN2021aess_20220301_H_merge_60551_1.fits

SN2021aess_20220301_J_merge_60551_1.fits

SN2021aess_20220311_Ks_merge_60551_1.fits

SN2021afuq_20211214_J_merge_60551_1.fits

SN2021afuq_20220112_H_merge_60551_1.fits

SN2021afuq_20220422_H_merge_60552_1.fits

SN2021afuq_20220422_J_merge_60552_1.fits

SN2021afuq_20220422_Ks_merge_60552_1.fits

SN2021pit_20211025_Ks_merge_60550_1.fits

SN2021pit_20211111_Ks_merge_60550_1.fits

SN2021pit_20211127_H_merge_60550_1.fits

SN2021pit_20211127_Ks_merge_60550_1.fits

SN2021pit_20211228_H_merge_60551_1.fits

SN2021pit_20220111_J_merge_60551_1.fits

SN2021pit_20220820_J_merge_60555_1.fits

SN2021pit_20220824_H_merge_60555_1.fits

SN2021xju_20220321_J_merge_60551_1.fits

SN2022adpu_20221229_H_merge_60556_1.fits

SN2022an_20220227_J_merge_60551_1.fits

SN2022an_20220310_J_merge_60551_1.fits

SN2022bqg_20220310_J_merge_60551_1.fits

SN2022buw_20220221_J_merge_60551_1.fits

SN2022buw_20220221_Ks_merge_60551_1.fits

SN2022cei_20220227_H_merge_60551_1.fits

SN2022cmd_20220227_J_merge_60551_1.fits

SN2022cme_20220227_J_merge_60551_1.fits

SN2022dtv_20220330_J_merge_60551_1.fits

SN2022esa_20220330_H_merge_60551_1.fits

SN2022esa_20220330_J_merge_60551_1.fits

SN2022fw_20220310_H_merge_60551_1.fits

SN2022fw_20220310_Ks_merge_60551_1.fits

SN2022idx_20220522_Ks_merge_60552_1.fits

SN2022pdq_20220820_J_merge_60555_1.fits

SN2022pul_20230416_J_merge_60557_1.fits

SN2022qh_20220330_H_merge_60551_1.fits

SN2022qzr_20221101_J_merge_60556_1.fits

SN2022qzr_20221101_Ks_merge_60556_1.fits

SN2022ssk_20220915_J_merge_60555_1.fits

SN2022szg_20220915_H_merge_60555_1.fits

SN2022szg_20220915_J_merge_60555_1.fits

SN2022wiv_20221015_H_merge_60555_1.fits

SN2022wiv_20221015_J_merge_60555_1.fits

SN2022xxf_20230114_J_merge_60556_1.fits

SN2022xxf_20230114_J_merge_60556_2.fits

SN2022zi_20220208_Ks_merge_60551_1.fits

SN2022zi_20220227_J_merge_60551_1.fits

SN2022zi_20220227_Ks_merge_60551_1.fits

SN2022zi_20220322_J_merge_60551_1.fits

SN2023Q_20230114_J_merge_60556_1.fits

SN2023cj_20230218_H_merge_60556_1.fits

SN2023cj_20230218_Ks_merge_60556_1.fits

Sn2021aclv_20211111_J_merge_60550_1.fits

Astrometry of the following image of SN2021adcr could not be improved with the PESSTO pipeline due of very poor quality of the image.

SN2021adcr_20211111_J_merge_60550_1.fits