Hi Job,Nice report!Good to see you are getting repeatable results. The fact that you are getting slightly different velocities each time is a bit strange indeed. In your report you mentioned that there were some difficulties with the Vlsr calculation. Have you tried using a Vlsr calculator like this one from ATNF (https://www.narrabri.atnf.csiro.au/observing/obstools/velo.html)?Alternatively you could repeat the observations a few times with the dish pointed away from NML Cyg. If you can demonstrate that the signal is only detected when the dish is pointed at NML Cyg and not when it is pointed at other points in the sky, then you can be quite certain that it is indeed from NML Cyg.Good luck!Eduard--On Sunday, 9 January 2022 at 23:10:57 UTC+1 jobge...@gmail.com wrote:NML CYGNI OH MASER WITH A SMALL RADIO DISH
Job Geheniau – Januari 2022
Dear fellow amateurs,
For over 2 months I have been working on my project 'NML Cygni OH maser', stimulated by observations by Eduard Mol and Michiel Klaassen.
This project involves the reception of the OH spectral line of NML Cygni with a relatively small radio dish. JRT - Job's Radio Telescope, 1.8 meters.
The results are in the attached PDF.
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