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Hi,
I guess I am the water maser guy here so I can share some of my experience…I use a norsat 9000LD unit for water maser observations, have not used any of those chinesium units so I can’t tell how good or bad they are in terms of noise figure and LO stability. The LO stability of those DRO LNBs can indeed be an issue indeed but there are ways to deal with it.You can use a DRO LNB “as is” for water maser detection, in that case your sensitivity will be degraded and you have a large uncertainty in the frequency but it’s still possible to detect the strongest sources.One trick to deal with LO frequency drifting over long integration times is to use a stable reference signal (be sure to offset it by a couple MHz so it does not overlap with the maser!). Then you can do the frequency correction afterwards in the data processing. I have used the weak 28th harmonic of a Leo Bodnar GPSDO for the reference.Michiel Klaasen had some success using an NTC heater to control the temperature of the LO to minimise frequency drifting (which apparently is mainly caused by temperature changes). He also uses a reference signal for frequency calibration (see
It is probably even better to get rid of the DRO entirely and somehow lock the LO to an external reference, at Astropeiler they did something like that if I remember correctly. It is well beyond my expertise though so I have not done any such modifications.
If you want to know more there is an article describing my 22.2GHz setup in the August 2022 SARA journal. There is also a long thread here on the SARA forum documenting the building and first observation results of my water maser setup, see https://groups.google.com/g/sara-list/c/TrZR8yCIWUE/m/3DNdYneJBwAJ.
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FYI, I posted some initial test results for this LNB here:
It does cover the maser frequency, although the NF performance there is not yet known.
James W7TXT
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