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A SPIDER radio telescope is a complete instrument, specifically developed as a professional but compact radio telescope, not a set of parts. Antenna, low noise amplifiers, 1420 MHz receiver, spectrometer, tracking system and control software arrive as one system, tested in our factory before it ships. We design and manufacture everything in Italy, and we install it on your site.

All three SPIDER models share the same receiver chain, the same RadioUniversePRO control software and the same weatherproof tracking system. What changes is collecting area. A larger antenna detects weaker sources and separates detail that a smaller one blends together. Main features:
SPIDER radio telescopes for radio astronomy are available in diameters from 2.3 meters to 5 meters, offering various types of antenna tracking systems with high precision and load capacity. SPIDER radio telescopes for radio astronomy come with a special 1420 MHz receiver and a full remote control and acquisition software.
A radio telescope is bought for the observations it makes possible. These are the four programmes every SPIDER owner runs.
Neutral hydrogen emits at 1420.406 MHz. Point the antenna at the galactic plane and the peak appears on screen in seconds. It is the clearest introduction to spectroscopy a student can have, because the physics is visible in the shape of the line.
Detect Cassiopeia A, Cygnus A and the Sun through cross scans and transits. With the NSGen-II noise generator you can calculate flux of the source in Jansky, so the measurement is absolute and comparable with published values.
Record hydrogen spectra at different galactic longitudes and read the Doppler shift of each peak. From those velocities a class reconstructs how our galaxy rotates, and finds the evidence that led astronomers to dark matter. This is a full laboratory course from one instrument.
Raster scan a region and RadioUniversePRO builds a radio map of an area your students cannot see with any optical telescope. It is the moment the invisible sky becomes an image they made themselves.

An optical telescope needs a clear, dark night. That is the single biggest problem for a school or a university department, because lessons happen during the day and the weather does not follow the timetable.
At 1420 MHz the sky behaves differently. The Sun does not blind the receiver, clouds are transparent, and rain is not a limitation. A class can point the antenna at 11 in the morning and record a hydrogen line spectrum before the bell. The same instrument runs unattended at night for a research programme.
This is why radio astronomy has become the practical way to give students real observations instead of archive data. They point the telescope, they collect the signal, they reduce the measurement themselves.
Tell us where the antenna will stand, how far the control room is and what your programme needs. We review interference conditions, cable runs and foundation requirements, then quote the configuration that fits. We supply the technical documentation your procurement office needs to open the file.
Every SPIDER is assembled and tested in our factory in Italy, before it ships. Crates are prepared for your destination and we handle documentation for worldwide delivery. Typical lead time is from 1 to 4 months from order.
Our technicians assemble the antenna, prepare the control room, align the instrument on known sky radio sources and train your staff on RadioUniversePRO before leaving. If you prefer to install it yourself (only for SPIDER 230C and 300A), the manual and our remote support cover the full procedure.

RADIO OVER FIBER: Replaces coaxial cable between amplifier and receiver, removing gain loss over distance and reducing interference.
MOUNT OVER FIBER: Controls the tracking system up to 2 km away over dedicated optical fiber.
NSGen-II NOISE GENERATOR: For absolute calibration, so you can calculatensource flux in Jansky.
WIND SENSOR: Parks the antenna at zenith automatically when wind exceeds the safety threshold.
RK19 RACK, 24 UNITS: Houses receiver, control units and computer with power distribution and temperature controlled fans.
CMP-19 CONTROL COMPUTER: Rack format computer running RadioUniversePRO, same form factor as the rest of the chain.
Written by Filippo Bradaschia, co-founder of PrimaLuceLab. 192 pages that explain how radio telescopes work, what the sky looks like in radio waves, and why some of the most interesting objects in the universe are invisible to an optical telescope. It covers electromagnetic waves, how a radio telescope receives them, the radio sources of the universe, the search for extraterrestrial intelligence and the radio phenomena of our own atmosphere. Explained with illustrations and pictures, and without complicated formulas. It is the best place to start if you are preparing a course, writing a thesis proposal, or simply deciding whether radio astronomy belongs in your institute.
