AMATEUR RADIO ASTRONOMY • 21-CM NEUTRAL HYDROGEN
Deep Space
1420 MHz
Radio Telescope
A 4.5-meter radio telescope built for long-term 1420 MHz radio astronomy, repeated observations of the Milky Way, and open sharing of the resulting data and visualizations.
CURRENT OBSERVATORY STATUS
Live sky, solar and local conditions
Current conditions for the observatory. Observation plots and scientific results are kept only in the Observations tab.
Weather: National Weather Service • Solar flux: NOAA SWPC • Sun/Moon positions and phase: calculated in-browser for the observatory location.
LONG-TERM AMATEUR RADIO ASTRONOMY
Observe. Repeat. Compare. Share.
The home page is now kept as an introduction and current-status page. Use the dedicated tabs above for the telescope hardware, observation results, workflow, paper and data archive.
LIVE OBSERVATORY
Current telescope livestream
This panel follows the current live broadcast from the Deep Space 1420 YouTube channel rather than a permanently fixed video.
THE OBSERVATORY
A purpose-built 4.5-meter receiving system
This tab is only about the telescope, receiver chain, positioning system and control station. Observation results are not repeated here.
CONTROL & INSTRUMENTATION
Observation and processing station
The control station handles telescope positioning, receiver monitoring, recording and the software tools used to operate the observatory.
REAL OBSERVATION PRODUCTS
Measured data — no simulated display graphics
This is the dedicated location for continuum, spectral and 3D observation results.
OBSERVATION WORKFLOW
From the sky to a finished radio-astronomy product
The workflow shows how a telescope pointing becomes recorded data, processed measurements and final plots or three-dimensional visualizations.
OBSERVATORY LOG
Notes & Articles
Observing notes, project updates and related links.
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TECHNICAL PAPER
A 4.5-Meter Amateur Radio Telescope for Long-Term Galactic Observations Including Neutral Hydrogen
The paper documents the telescope, instrumentation, observing approach, processing workflow and initial observational results.
PUBLIC DATA ARCHIVE
Plots, scans and supporting observation files
The large working archive remains on Google Drive so the website can stay fast while the underlying material remains accessible.