PESSTO Year 3+4 - Final SOFI imaging reduction


Summary:
SOFI images reduced with PESSTO pipeline version 2.2.10.

411 total reduced SOFI images (140 J + 137 H + 134 Ks-band).
11 from the total are OB repeats (ftom these 1 JHK OB initially with wrong coordinates) during the same night (4 J + 3 H + 4 Ks-band).
21 from the total are photometric standard star observations (7 J + 7 H + 7 Ks-band).
3 from the total are obtained with wrong coordinates (1 J + 1 H + 1 Ks-band).
->
376 epochs of science target data (128 J + 126 H + 122 Ks-band).


2014-09-03:
NGC772-OT1 and SN2009ip reduced images have ghosts from the host galaxy.

CSS140424-133007-212728 Ks-band pipeline reduction results in two final frames.
CSS140424-133007-212728_20140903_Ks_merge_57620_1.fits
CSS140424-133007-212728_20140903_Ks_merge_57620_2.fits

2014-09-22:
SN2009ip reduced J-band image has ghosts from the host galaxy.

2014-09-29:
SN2013fc reduced J and H-band images have ghosts from the host galaxy.

NGC772-OT1 J-band beamswitch sequence has 36 ON and only 12 OFF frames.

2014-10-03:
NGC7552-OT H and J-band beamswitch sequences have 6 ON and 8 OFF frames.

NGC772-OT1 H-band beamswitch sequence has 7 ON and 8 OFF frames.

NGC772-OT1 J-band beamswitch sequence has 6 ON and 8 OFF frames.

2014-11-02:
LSQ14fxj reduced H-band image has vertical noise pattern.

2014-11-14:
ASASSN-14il has a JHKs sequence with incorrect coordinates (00:00:00.0 +00:00:00.0). This was also noted in the nightlog. The reduction of these files resulted in files
ASASSN-14il_20141114_H_merge_57621_1.fits
ASASSN-14il_20141114_J_merge_57621_1.fits 
ASASSN-14il_20141114_Ks_merge_57621_1.fits
Another sequence was obtained with correct pointing resulting in files
ASASSN-14il_20141114_H_merge_57621_2.fits
ASASSN-14il_20141114_J_merge_57621_2.fits
ASASSN-14il_20141114_Ks_merge_57621_2.fits

2014-12-14:
PESSTOESO154-G10 reduced Ks-band image has negative residuals.

2014-12-29:
SN2013hx reduced Ks-band image has alignment problems.

2015-01-27:
SN2013fc reduced JHKs images have ghosts from the host galaxy.

2015-03-13:
PSNJ07361576-6930230 reduced J-band image has horizontal noise pattern.

2015-03-20:
PS15ae has only one image in Ks-band
SOFI.2015-03-21T04:46:02.697.fits
DATA NOT REDUCED!!!

PSNJ07361576-6930230 J-band OB restarted after 2 frames. These images were not used in the reductions
SOFI.2015-03-21T00:42:46.425.fits
SOFI.2015-03-21T00:43:00.927.fits

PSNJ07361576-6930230 JHK data pipeline reduction resulted in two sets of final frames
PSNJ07361576-6930230_20150320_H_merge_57622_1.fits
PSNJ07361576-6930230_20150320_J_merge_57622_1.fits
PSNJ07361576-6930230_20150320_Ks_merge_57622_1.fits
PSNJ07361576-6930230_20150320_H_merge_57622_2.fits
PSNJ07361576-6930230_20150320_J_merge_57622_2.fits
PSNJ07361576-6930230_20150320_Ks_merge_57622_2.fits
The second set is not very deep.

2015-04-09:
SN2015D reduced JHKs images have ghosts from the host galaxy.

2015-04-18:
LSQ15adm JHKs data observed with a non-standard 3 point dither sequence.

P9181 photometric standard field observed in JHKs.

2015-04-27:
P9129 and P9181 photometric standard fields observed in JHKs. Pipeline reduction naming convention not logical
STD_20150427_H_merge_57622_1.fits  -  P9181
STD_20150427_J_merge_57622_1.fits  -  P9129
STD_20150427_Ks_merge_57622_1.fits -  P9181
STD_20150427_H_merge_57622_2.fits  -  P9129
STD_20150427_J_merge_57622_2.fits  -  P9181
STD_20150427_Ks_merge_57622_2.fits -  P9129

2015-08-14:
LSQ15adm reduced J-band image has very prominent horizontal noise pattern.

2015-09-04:
ASASSN-15oz reduced H-band image has vertical noise pattern.

SN2013fc reduced JHKs images have ghosts from the host galaxy.

2015-10-04:
ASASSN-15oz reduced H-band image has negative residuals.

PSNJ02051332+0606084 reduced Ks-band image is very low quality.

2015-10-11:
LSQ15adm reduced H-band image has negative residuals.

ASASSN-15qc reduced H-band image has ghosts from the host galaxy.

2015-11-21:
ASASSN-15oz JHKs data observed with a non-standard single cycle 5 point dither sequence.

2015-12-05:
SN2015F observed without beamswitching and reduced JHKs images have residual from the host galaxy.

P9119 and P9129 photometric standard fields observed in JHKs.

SN2013hx JHKs images obtained with a typo in declination coordinates. The centered coordinates should be roughly 01:35:35.3 -57:57:30.6, but are instead around 01:35:35.3 -57:05:30.6. The observed field does not cover SN2013hx.

2015-12-17:
SN2015F observed without beamswitching and reduced JHKs images have residual from the host galaxy.

P9119 and P9129 photometric standard fields observed in JHKs.

2016-01-02:
SN2015F JHKs observations have a non-standard beamswitch sequence. Pipeline reduced final images from the complete data set are not properly aligned. Using only 4 ON and 4 OFF images. This is 8/24 J, 8/28 H, and 8/34 Ks-band images.

2016-01-16:
SN2016B reduced H-band image has an artifact in the field.

2016-01-17:
SN2015F JH observations have a non-standard beamswitch sequence. Pipeline reduced final images from the complete data set are not properly aligned. Using only 4 ON and 4 OFF images. This is 8/24 J, and 8/28 H-band images.

2016-01-26:
OGLE15xl has a second sequence with only one image in Ks-band
SOFI.2016-01-27T07:23:44.238.fits
Nightlog reports that an OB was aborted. DATA NOT REDUCED!!!

ASASSN-14ko J-band OB aborted after 10 exposures. This is also reported in the nightlog.

ASASSN-14ko J-band pipeline reduction resulted in two final frames
ASASSN-14ko_20160126_J_merge_57622_1.fits
ASASSN-14ko_20160126_J_merge_57622_2.fits
The latter is of poor quality.

PS15dpn reduced H-band image has negative residuals.

OGLE15xl reduced Ks-band image is of low quality. Clouds reported in the nightlog.

2016-02-06:
ASASSN14lp JHKs observations have a non-standard beamswitch sequence. Pipeline reduced final images from the complete data set are not properly aligned. Using only 4 ON and 4 OFF images. This is 8/26 J, 8/30 H, and 8/46 Ks-band images. Ks-band image has artifacts in the field.

2016-02-14:
SN2015F J and H-band observations have a non-standard beamswitch sequence. Pipeline reduced final images from the complete data set are not properly aligned. Using only 4 ON and 4 OFF images. This is 8/24 J, and 8/28 H-band images.

SN2016adj JHK pipeline reduction resulted in two sets of final frames
SN2016adj_20160214_H_merge_57623_1.fits
SN2016adj_20160214_J_merge_57623_1.fits
SN2016adj_20160214_Ks_merge_57623_1.fits
SN2016adj_20160214_H_merge_57623_2.fits
SN2016adj_20160214_J_merge_57623_2.fits
SN2016adj_20160214_Ks_merge_57623_2.fits

2016-02-17:
SN2015F Ks-band observations have a non-standard beamswitch sequence.

2016-02-23:
SN2016adj H-band beamswitch sequence has 5 ON and 4 OFF frames.

SN2016X reduced JHKs images have artifacts in the field.

2016-02-25:
ASASSN-15og H-band sequence has 7 frames.

2016-03-07:
SN2016adj reduced J-band images has horizontal noise pattern.

2016-04-12:
SN2016aiy reduced H-band image has negative residuals.

2016-04-13:
PS15ae J and H-band sequence has a non-standard 6 point dither sequence.

ASASSN14lp J-band observations have a non-standard beamswitch sequence.

2016-04-14:
ASASSN14lp H-band observations have a non-standard beamswitch sequence. Pipeline reduced final image from the complete data set is not properly aligned. Using only 4 ON and 4 OFF images. This is 8/40 H-band images.

SN2015F J and H-band observations have a non-standard beamswitch sequence. Pipeline reduced final images from the complete data set are not properly aligned. Using only 4 ON and 4 OFF images. This is 8/34 J, and 8/40 H-band images.




The astrometry of the following 56 reduced images were corrected with PESSTOASTRO:

ASASSN-14ha_20140922_J_merge_57620_1.fits
ASASSN-14ha_20141013_H_merge_57620_1.fits
ASASSN-14ha_20141013_J_merge_57620_1.fits
ASASSN-14il_20141114_J_merge_57621_2.fits
ASASSN-14ko_20150119_H_merge_57621_1.fits
ASASSN-14ko_20151121_J_merge_57622_1.fits
ASASSN-14ko_20160414_H_merge_57624_1.fits
ASASSN-15fz_20150409_Ks_merge_57622_1.fits
ASASSN-15ga_20150411_H_merge_57622_1.fits
ASASSN-15ga_20150411_J_merge_57622_1.fits
ASASSN-15ga_20150411_Ks_merge_57622_1.fits
ASASSN14lp_20160414_H_merge_57624_1.fits
ASASSN_15oz_20151004_J_merge_57622_1.fits
LSQ15adm_20150427_H_merge_57622_1.fits
LSQ15adm_20150427_J_merge_57622_1.fits
LSQ15adm_20150427_Ks_merge_57622_1.fits
MASTERJ003918.04+035659.6_20151121_J_merge_57622_1.fits
MASTERJ003918.04+035659.6_20151121_Ks_merge_57622_1.fits
NGC772-OT1_20140903_Ks_merge_57620_1.fits
OGLE-2015-SN-073_20150214_Ks_merge_57621_1.fits
OGLE15xl_20160126_Ks_merge_57622_1.fits
PS15ae_20150427_Ks_merge_57622_1.fits
PSNJ02051332+0606084_20151004_Ks_merge_57622_1.fits
PSNJ07361576-6930230_20150311_J_merge_57621_1.fits
PSNJ07361576-6930230_20150312_Ks_merge_57621_1.fits
PSNJ07361576-6930230_20150313_Ks_merge_57621_1.fits
PSNJ07361576-6930230_20150320_J_merge_57622_1.fits
PSNJ07361576-6930230_20150320_Ks_merge_57622_1.fits
PSNJ07361576-6930230_20150320_Ks_merge_57622_2.fits
PSNJ23002463+0137368_20150814_J_merge_57622_1.fits
SN2009ip_20140903_H_merge_57620_1.fits
SN2013fc_20140929_H_merge_57620_1.fits
SN2013fc_20140929_J_merge_57620_1.fits
SN2013fc_20150127_J_merge_57621_1.fits
SN2013fc_20150904_H_merge_57622_1.fits
SN2014cx_20141023_H_merge_57620_1.fits
SN2014cx_20141023_J_merge_57620_1.fits
SN2014cx_20141023_Ks_merge_57620_1.fits
SN2015D_20150209_H_merge_57621_1.fits
SN2015D_20150209_Ks_merge_57621_1.fits
SN2015D_20150311_J_merge_57621_1.fits
SN2015F_20150411_J_merge_57622_1.fits
SN2015F_20150411_Ks_merge_57622_1.fits
SN2015F_20150427_J_merge_57622_1.fits
SN2015F_20160214_J_merge_57624_1.fits
SN2015F_20160414_J_merge_57624_1.fits
SN2016B_20160214_H_merge_57624_1.fits
SN2016B_20160214_J_merge_57624_1.fits
SN2016B_20160214_Ks_merge_57624_1.fits
SN2016adj_20160223_H_merge_57623_1.fits
SN2016adj_20160307_J_merge_57623_1.fits
SN2016adj_20160412_H_merge_57623_1.fits
SN2016adj_20160412_J_merge_57623_1.fits
SN2016adj_20160412_Ks_merge_57623_1.fits
SN2016aiy_20160307_H_merge_57623_1.fits
STD_20150427_H_merge_57622_2.fits


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