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Accuracy of the retrieved oblateness parameter in the light curve which included red noise, for all eight σw noise levels. Squares in the input f–ϑ grid are coloured based on

Estimated sampleability efficiency for Nightingale (left) and Osprey (right) . Blue indicates high efficiency while red indicates low efficiency. The tan circle denotes the area that contained 98.3% of Monte

The Large Dirty Mars Chamber, housed at the Open University. Credit: Petr Brož Scientists have been able to recreate the extreme conditions found on icy moons in deep space –

Deep imaging (top) and polarimetric (bottom) maps of 3I from a subset of VLT observations. The colour scale in the imaging maps does not reflect the absolute brightness of the

This artist’s impression shows the planet-forming disc around the star V883 Orionis. In the outermost part of the disc, volatile gases are frozen out as ice, which contains complex organic

VLA Photo: Credit: NSF/NSF NRAO/AUI/B.Foott This white paper highlights the work that is needed to anticipate the challenges and societal impacts of a possible technosignature detection. We recommend practical steps