Brage and Vale telescopes often picks up significant radio frequency interference (RFI). Work in progress to fix these issues.
If you have any questions or run into problems, please first read the User's manual and experiment instructions below. If you still need help, contact us at salsa.onsala@gmail.com.
We'd also love to hear from anyone using SALSA — what you observed, what worked, what surprised you. Same address. Knowing how the telescopes are being used helps us prioritise the time we put into keeping them running.
The user's manual describes how to operate the SALSA telescope — scheduling observations, pointing, recording spectra, and downloading data.
Step-by-step lab guides covering the scientific background, observing procedure, and data analysis for each experiment.
Observe neutral hydrogen across the Milky Way, measure Doppler-shifted 21 cm emission, derive the rotation curve, and reconstruct the positions of the spiral arms.
Receive and compare radio signals from GPS, Galileo, GLONASS, and BeiDou satellites, and see how their different modulation schemes produce distinct spectral shapes.
Use the Sun as a bright radio source to map the beam pattern of the SALSA antenna, measure its angular resolution, and compare the result to theoretical predictions for a circular aperture.
Target visibility — for a galactic, equatorial, or Sun target on a given date, see when it is above the horizon at the SALSA site (Onsala, Sweden) so you can pick a booking window where it is actually observable. Open the visibility planner.
The observation archive page has built-in baseline-subtraction and Gaussian-fitting tools that cover most analysis workflows. The tools below are kept around for users who prefer to work in their own environment with the FITS files SALSA exports.
For hardware details — signal chain, rotor protocol, LNA measurements, and component references — see the Technical specifications page.