WR-137 Waveguide and Masers
WR-137 waveguide covers roughly 5.8–8.2 GHz, which puts you squarely in C-band.
That is an excellent range for amateur radio astronomy, because it includes one of the brightest and most accessible astrophysical maser lines.
Below are the best targets you can observe with WR-137 hardware.
⭐ Top Target: 6.668 GHz Methanol Masers (CH₃OH)
Frequency: 6.668519 GHz
In WR-137 band: YES – perfect match
Why they’re ideal:
- Extremely bright Class II masers
- Located in active star-forming regions
- Narrow lines that show Doppler velocity beautifully
- Detectable with 1–2 m dishes and a low-noise C-band LNA
- Many sources observable from mid-latitudes
Strong, Amateur-Detectable Methanol Maser Targets
Here are some of the best ones:
| Source | RA / Dec | Notes |
|---|---|---|
| W3(OH) | 02h 27m / +61° 52′ | One of the brightest 6.7 GHz masers in the sky |
| W51 | 19h 23m / +14° 31′ | Very strong; excellent target for smaller dishes |
| W49N | 19h 10m / 09° 06′ | Extremely powerful; good for velocity structure |
| Orion KL | 05h 35m / −05° 22′ | Classic star-forming region; bright masers |
| Cep A | 22h 56m / +62° 01′ | Compact, strong source |
| NGC 7538 | 23h 13m / +61° 28′ | Stable, bright maser emission |
These are the best C-band targets for amateur maser detection worldwide.
With a WR-137 waveguide feed and a good LNA (<1 dB NF if possible), you can definitely detect several of these.
⭐ Additional Targets in WR-137 band
Beyond the methanol masers, there are a few other areas of interest within the 5.8–8.2 GHz range:
1. Radio Continuum
Useful for calibrating your system or doing mapping:
- Galactic H II regions (W3, W49, W51, Orion)
- Supernova remnants such as Cassiopeia A, Cygnus A
- The Galactic plane (broadband synchrotron and thermal emission)
All very strong in C-band.
2. Recombination lines
There are several hydrogen recombination lines near 6–8 GHz (Hnα, e.g., H109α ~5.99 GHz).
These are weaker than masers but can be detected with longer integrations.
⭐ What You Cannot Do With WR-137
Just to clarify expectations:
| Line | Freq | In band? |
|---|---|---|
| Hydrogen 21 cm | 1420 MHz | ❌ Not in WR-137 |
| OH masers | 1.6 GHz | ❌ Not in WR-137 |
| Water maser | 22 GHz | ❌ Not in WR-137 |
| SiO masers | 43/86 GHz | ❌ Not in WR-137 |