e-MERLIN Archives

The WISE and VLASS-SE images of J2335-0004. The right panel is the VLASS-SE image. The FWHM and centroid derived from the VLASS-SE image are blue ellipses and dots in all five panels. The four left panels are W1, W2, W3, and W4 band images of the source. The green contours represent 10𝜎, 50𝜎 and 100𝜎 of the noise levels in WISE W1 and W2 images, 3𝜎 and 6𝜎 in W3 and W4 images, and −1𝜎, 10𝜎 and 80𝜎 in the VLASS-SE image. The candidate star’s location is shown as the red stars in all the panels. -- astro-ph.GA

Astronomy & Telescopes, Imaging & Spectroscopy, Interstellar, Science Fiction, SETI & Technosignatures, Status Report

High-resolution Imaging Of The Radio Source Associated With Project Hephaistos Dyson Sphere Candidate G

by Keith CowingJanuary 11, 2025January 11, 2025

We present high-resolution e-MERLIN and EVN (e-VLBI) observations of a radio source associated with Dyson Sphere candidate G, identified as part of Project Hephaistos.

e-MERLIN

High-resolution Imaging Of The Radio Source Associated With Project Hephaistos Dyson Sphere Candidate G

Gullies In The Equatorial Region of Mars

Orbital Biosignature Assay: Watching Forests Grow From Space

Signs And Signatures Of Intelligence

CO Snow Lines Are Stabilised By The Vertical Transport Of Volatiles

Multi-year Ground-Based Survey Photometry of Active Comet 103P/Hartley 2 and Centaur (2060) Chiron: A Tale of Two Comets in the Pre-LSST Era