Results 71 to 80 of about 362 (148)

Opportunities for Technosignature Science in the Astro2020 Report [PDF]

open access: green, 2022
Jacob Haqq‐Misra   +9 more
openalex   +1 more source

Dual-backend Multibeam Position-switching Targeted SETI Observations toward Nearby Active Planet-hosting Systems with FAST

open access: yesThe Astronomical Journal
The Five-hundred-meter Aperture Spherical Telescope (FAST), the world’s largest single-dish radio telescope, lists the search for extraterrestrial intelligence (SETI) as one of its key scientific objectives.
Jian-Kang Li   +3 more
doaj   +1 more source

A Model-independent Radio Telescope Dark Matter Search in the L and S Bands

open access: yesThe Astrophysical Journal Letters
Ultralight bosonic dark matter in its most general form can be detected through its decay or annihilation to a quasimonochromatic radio line. Assuming only that this line is consistent with the most general properties of the expected phase space of our ...
Aya Keller   +2 more
doaj   +1 more source

Multibeam SETI Observations Toward Nearby M Dwarfs with FAST

open access: yesThe Astronomical Journal
The search for extraterrestrial intelligence (SETI) targeted searches aim to observe specific areas and objects to find possible technosignatures. Many SETI researches have focused on nearby stars and their planets in recent years.
Xiao-Hang Luan   +5 more
doaj   +1 more source

What Type of Technosignatures Can We Detect?

open access: yes, 2020
The existence of causal constraints introduces a temporal selection effect in the type of technosignatures that we can detect.
openaire   +1 more source

The FAST-SETI Milky Way Globular Cluster Survey. I. A Pilot Multibeam On-the-fly Search of Five Globular Clusters at the L Band

open access: yesThe Astronomical Journal
We report a narrowband technosignature search toward five Milky Way globular clusters—NGC 6171, NGC 6218, NGC 6254, NGC 6838, and IC 1276—using Five-hundred-meter Aperture Spherical radio Telescope (FAST)’s 19 beam L -band receiver (1.05–1.45 GHz).
Bo-Lun Huang   +3 more
doaj   +1 more source

The Case for Technosignatures: Why They May Be Abundant, Long-lived, Highly Detectable, and Unambiguous

open access: gold, 2022
Jason T. Wright   +5 more
openalex   +1 more source

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