We present an imaging-domain search for technosignatures at decametric wavelengths with the OVRO-LWA, targeting ultra-narrowband continuous-wave signals between 50 and 86 MHz.
astronomy
The Mass of TOI-1883 b: A Low Density Super-Neptune In The Ridge Regime Transiting An Early-M dwarf
Recent large-scale transit surveys conducted by space telescopes such as Kepler and TESS have revealed a vast number of exoplanets, uncovering the diversity of their population.
Updated Rules for Evaluating and Revealing the Detection of Extraterrestrial Intelligence
The IAA SETI Committee announced today updated rules for evaluating and revealing the detection of extraterrestrial intelligence.
Rocky Worlds DDT Community Involvement Initiative (CII)
The Rocky Worlds DDT Core Implementation Team is pleased to announce the launch of a new, community-led effort to enable collaboration and coordination around Rocky Worlds DDT science: the Rocky […]
New Model Refines Search For Habitable Planets
Researchers have developed the Smaller Than Earth Habitability Model (STEHM) to assess which planets can maintain life-supporting atmospheres, focusing on size and atmospheric dynamics.
A Critical UV Legacy: A Hubble Roadmap for HWO Science Readiness
The Habitable Worlds Observatory (HWO) will provide the first opportunity to directly image and spectrally characterize terrestrial exoplanets in the habitable zones of nearby stars.
First Ever Live Observation Of The Rotation Of A Planetary Nursery
The rotation of a protoplanetary disc (a disc where planets are being formed) has been observed directly for the very first time by mapping the emissions from the dust grains […]
Some Thoughts on the Future of Technosignature Searches: Constraining the Fermi Paradox
This paper examines how future technosignature searches may constrain competing resolutions of the Fermi Paradox, with particular attention to the possibility that technologically capable entities (TCEs) are either intrinsically rare […]
The First Glimpse of Water Ice Absorption Map in the Milky Way
Interstellar ice plays a key role in the thermal evolution of the interstellar medium and in astrochemical pathways, yet its large-scale distribution remains poorly constrained.
Non-detection Of HC(S)SH: Estimating Upper Limits And Constraining Chemistry
The search for dithioformic acid (t-HC(S)SH) in star-forming regions is crucial for understanding interstellar sulfur chemistry and addressing the ‘missing sulfur’ problem. Motivated by a recent claim of t-HC(S)SH detection […]
