Embedded Files
Summary:
The reductions of the SOFI spectroscopy resulted in 32 GB and 3 GR spectra.
2021-11-27:
SN2021acya GB spectrum has been obtained without an accompanying spectroscopic standard star observations. Feige110 from 2021-10-26 was used in the reductions.
2021-11-27:
SN2021acya GB spectrum has been obtained with HIP19501 as the telluric standard star, which is a F5V type star rather than a G or A-type star and the PESSTO pipeline will not make use of it. Therefore, telluric standard star HIP12167 from 2021-10-26 was used in the reductions.
2022-01-12:
SN2022an GB spectrum has been obtained with an accompanying spectroscopic standard star GD71. From the sequence of 4 frames the final two are not useful and were not included in the reductions.
2022-01-12:
SN2022an GB spectrum reduction was extracted of the only clear trace of a point source in the data; however, the spectrum was not necessarily aligned on the correct target.
2022-02-08:
SN2022an GB spectral sequence of 12 exposures included the following image pair (5th and 6th exposure) that is not useful and was excluded from the reductions.
SOFI.2022-02-09T06:10:45.771.fits
SOFI.2022-02-09T06:17:57.101.fits
2022-02-30:
SN2022qh GB spectral sequence of 12 exposures included the following image pair (3th and 4th exposure) that is not useful and was excluded from the reductions.
SOFI.2022-03-31T04:55:40.418.fits
SOFI.2022-03-31T05:02:51.748.fits
2022-02-30:
SN2022ara GB spectral sequence was aborted after 2 exposures by the observers and the resulting data could not be reduced. The affected files are:
SOFI.2022-03-31T04:07:37.017.fits
SOFI.2022-03-31T04:14:45.066.fits
As noted by the observers in the nightlog: "ABORTED. Noisy images, communication problems, could not confidently identify the target, then recurrence of noise."
2022-03-30:
SN2022qh GR spectral sequence of 12 exposures included the following final 6 images that had a notable drop in signal-to-noise ratio and were excluded from the reductions.
SOFI.2022-03-31T07:18:34.401.fits
SOFI.2022-03-31T07:30:24.376.fits
SOFI.2022-03-31T07:42:04.513.fits
SOFI.2022-03-31T07:53:51.206.fits
SOFI.2022-03-31T08:05:31.345.fits
SOFI.2022-03-31T08:17:21.316.fits
2022-04-21:
Hip053982 GB files are associated as SN2022qh files by the PESSTO pipeline and were excluded from the reductions.
SOFI.2022-04-22T07:13:37.061.fits'
SOFI.2022-04-22T07:13:49.715.fits
2022-04-21:
SN2022qh GB spectral sequence has a single non-sequence file, which was excluded from the reductions.
SOFI.2022-04-22T05:22:26.551.fits
2022-04-21:
SN2022qh GB spectral sequence of 9 exposures included the following 4 images that had a notable drop in signal-to-noise ratio and were excluded from the reductions.
SOFI.2022-04-22T06:41:25.910.fits
SOFI.2022-04-22T06:48:33.962.fits
SOFI.2022-04-22T06:55:35.455.fits
SOFI.2022-04-22T07:02:43.505.fits
2022-04-21:
SN2022ara GB sequence was started more than once within poor conditions, only the sequence of the following 12 images was used in the reductions.
SOFI.2022-04-22T03:38:22.522.fits
SOFI.2022-04-22T03:45:33.852.fits
SOFI.2022-04-22T03:52:35.349.fits
SOFI.2022-04-22T03:59:46.680.fits
SOFI.2022-04-22T04:06:48.176.fits
SOFI.2022-04-22T04:14:02.786.fits
SOFI.2022-04-22T04:21:04.281.fits
SOFI.2022-04-22T04:28:15.611.fits
SOFI.2022-04-22T04:35:17.106.fits
SOFI.2022-04-22T04:42:28.437.fits
SOFI.2022-04-22T04:49:29.936.fits
SOFI.2022-04-22T04:56:41.263.fits
2022-05-22:
SN2022zi GB spectral sequence was affected by the instrumental noise in the upper right corner quadrant of SOFI.
2022-10-02:
SN2022zi GB spectral sequence of 20 exposures seem to have lost the target from the slit after 8 exposures and the following files were excluded from the reductions.
SOFI.2022-10-03T08:00:11.690.fits
SOFI.2022-10-03T08:07:26.302.fits
SOFI.2022-10-03T08:14:27.796.fits
SOFI.2022-10-03T08:21:39.126.fits
SOFI.2022-10-03T08:28:40.620.fits
SOFI.2022-10-03T08:35:51.990.fits
SOFI.2022-10-03T08:42:53.485.fits
SOFI.2022-10-03T08:50:21.212.fits
SOFI.2022-10-03T08:57:22.706.fits
SOFI.2022-10-03T09:04:34.038.fits
SOFI.2022-10-03T09:11:35.532.fits
SOFI.2022-10-03T09:18:46.866.fits
2022-11-01:
SN2022vqz GB spectrum has been obtained without an accompanying spectroscopic standard star observations. Feige110 from 2022-10-17 was used in the reductions.
2022-11-01:
SN2022vqz GB spectral sequence of 12 exposures has issues aligning the trace from the following 2 images, which were not used in the reductions.
SOFI.2022-11-02T00:49:44.172.fits
SOFI.2022-11-02T00:56:55.501.fits
2022-11-16:
SN2022vqz GB observations include only the one following exposure. Nightlog reports that "SOFI cooling alarm was triggered again and the observations were halted." This data was not reduced.
SOFI.2022-11-17T01:12:07.646.fits
2022-11-17:
SN2022vqz, SN2022ywc, and SN2022xkq GB spectra have been obtained without an accompanying spectroscopic standard star observations. Feige110 from 2022-10-17 was used in the reductions.
2022-11-17:
SN2022ywc GB spectral sequence of 12 exposures has non-existing trace and was affected by the instrumental noise in the upper right corner quadrant of SOFI, the following 10 images were excluded from the reductions.
SOFI.2022-11-18T04:05:23.359.fits
SOFI.2022-11-18T04:12:24.854.fits
SOFI.2022-11-18T04:19:26.350.fits
SOFI.2022-11-18T04:26:27.844.fits
SOFI.2022-11-18T04:33:29.339.fits
SOFI.2022-11-18T04:40:30.834.fits
SOFI.2022-11-18T04:47:32.329.fits
SOFI.2022-11-18T04:54:43.658.fits
SOFI.2022-11-18T05:01:45.155.fits
SOFI.2022-11-18T05:08:46.651.fits
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