Above 30 GHz the Methanol masers at around 37 GHz are probably the easiest. See https://iopscience.iop.org/article/10.1088/0004-637X/742/2/109/pdf for a list.
If you are ok with somewhat lower frequencies, then the 22 GHz water masers are quite bright.
Wolfgang
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Eduard,
Indeed we have observed water maser emission at 22 GHz from various sources. Please find attached an example of one of the stronger sources, W51. The horizontal scale is the VLSR-corrected velocity and the frequency in MHz. The vertical scale is the flux in uncalibrated units.
This observation was made with our 10-m dish and two minutes integration time. The signal to rms noise is 107, so quite good. If one extrapolates this to a 3-m dish, about 250 minutes integration time would be needed to get the same SNR. However, one can certainly live with less SNR. So I thing it is doable to observe water masers with a smaller dish. Since water masers can vary, W51 may not be the strongest source at the moment, so one should try others as well. I should also mention that at 22 GHz or 10-m dish is under-illuminated so the effective area is actually smaller so it may even look better for the 3-m dish.
The tricky thing is the receiver. In our case it was a dual Ku/Ka band LNB. It was modified so that an external reference frequency could be used to get precise frequencies. Whether one can do without that and just live with the fact that there is a frequency offset, I don’t know. I will need to check with Horst (our high frequency expert) which Ku/Ka LNB he was using.
Easier on the receiver side there is Methanol at 12 GHz where one can use a standard LNB. As you pointed out these masers are weaker than the water masers. I have attached an example of the Methanol maser in W3. This is with 10 minutes integration time and a SNR of 41. Extrapolating this to a dish of 3 meter leads to an integration time of ~1230 minutes. But then one could also reduce the spectral resolution and reduce the requirement for the SNR. Reducing the spectral resolution by a factor of 4 (which is still quite ok) reduces the observation time by half, and going from 41 to about 10 for SNR cuts the required integration time by a factor of 16. Then you only need some 20 minutes for a detectable signal.
So in conclusion I would say that both water masers and methanol masers are within the realm of possibilities for a 3-m dish. Obviously it is not easy-going on the receiver side.
Best,
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I can help with the dish end of this potential project. I have three commercial 26 GHz, about four foot diameter, linear polarization feed, terminated with an SMA female connector, dishes. The SMA launcher may be removed to expose a WR34 flange where an LNA would be mounted. Contact me off-list for further details if interested. I am in the San Francisco Bay area.
Doug, W6DSR
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Yes, I figured as much, but I have had some inquiries about the antenna where at least one is only a continent away…
Good luck with your efforts,
-Doug, W6DSR
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