Personal Radio Observatory
Explore authentic telescope measurements.
Listen to the measured universe. Ingrid Deep Signal is a browser-based workstation for examining authentic radio-telescope observations while keeping measured evidence separate from interpretation.
Verify and Scan the Recording
Deep Signal downloads the complete archived HIP35136 telescope observation, verifies its SHA-256 fingerprint, reads the SIGPROC metadata, and analyzes the frequency band you select.
Spectrum + Waterfall
Visualize the frequency band selected in the verified HIP35136 telescope observation. The spectrum shows mean measured power by frequency channel. The waterfall shows how measured power changes across the 273 observation rows.
Spectrum
Waterfall
Green Bank 20-Meter Radio Telescope
Follow real observations from Green Bank Observatory through UNC’s Skynet Robotic Telescope Network. The automated 20-meter instrument supplies radio measurements, calibrated spectra and FITS products that can be compared with the verified HIP35136 recording above.
See Space Through a Real Optical Telescope
Radio observations appear as spectra and signal measurements. For an actual camera view of stars, nebulae, planets and galaxies, open one of these robotic optical-telescope services.
Slooh streams real telescope feeds and lets members capture deep-space images. Availability depends on darkness, weather and the observing schedule.
Open Slooh Live TelescopesUNC Skynet schedules genuine optical-telescope exposures and returns the resulting astronomical image after the observation is completed.
Open Skynet Optical NetworkSETI Study Workflow
Use several independent observations and record the same evidence fields for every scan before comparing possible signals.
Identify the observation
Record source name, UTC time, telescope, receiver, coordinates, center frequency, bandwidth and channel count.
Compare ON and OFF targets
A candidate associated with the sky target should appear in ON-target data and weaken or disappear in OFF-target controls.
Measure drift and repetition
Track frequency, signal-to-noise ratio, bandwidth and drift rate across time, then look for repeat observations.
Screen terrestrial interference
Compare polarization, known radio-frequency interference, nearby bands and other pointings before elevating a candidate.
Deep Signal Meters
These instruments are calculated directly from the verified HIP35136 radio-telescope samples in the frequency band selected above. No random values, prerecorded motion, or synthetic placeholder measurements are used.
GreenBank-20 · Skynet Live Telescope
This is the official University of North Carolina Skynet GreenBank-20 telescope page. The live panel below loads Skynet directly so telescope status and Live Pointing come from the source rather than being simulated or recreated by Ingrid.
TruthMode: the embedded view is the official Skynet page itself. Ingrid does not manufacture telescope status, pointing, observation, RA, Dec, weather, dome, or control data. If Skynet blocks third-party embedding in a browser, use “Open GreenBank-20 Full Screen” to view the same live source directly.
Hubble Space Telescope · Current Observation
Follow Hubble’s current observing activity through the official Space Telescope Live experience. Because the source blocks third-party iframe embedding, Ingrid opens the official observatory page directly rather than displaying a blocked or simulated panel.
See What Hubble Is Observing
Open the official live-observation interface to view Hubble’s current target, observation information, instrument context, and sky position as provided by Space Telescope Live.
OPEN HUBBLE LIVE OBSERVATIONTruthMode: Space Telescope Live provides current observation information; it is not a continuous onboard video camera feed from Hubble.