Sunscreen: Photometric Signatures of Galaxies Partially Cloaked in Dyson Spheres
Brian C. Lacki

TL;DR
This paper explores how cloaking stars in galaxies with Dyson spheres affects their observed spectra and colors, providing potential photometric signatures to identify advanced extraterrestrial civilizations.
Contribution
It introduces a spectral synthesis model to predict galaxy signatures when stars below certain luminosities are cloaked, highlighting observable differences in galaxy colors and spectra.
Findings
Galaxies with low L_min show minor spectral changes, especially in blue, star-forming galaxies.
Higher L_min thresholds produce galaxies with unnatural colors and luminosities.
Cloaking causes star-forming galaxies to appear bluer in UV and blue wavelengths, resembling quasars.
Abstract
The Search for Extraterrestrial Intelligence has so far come up negative for Kardashev Type III societies that capture all starlight from a galaxy. One possible reason is that shrouding a star in a megastructure is prohibitively expensive. Most of a galaxy's starlight comes from bright stars, which would require structures even larger than the classical Dyson sphere to enclose. Using a custom spectral synthesis code, I calculate what happens to the spectrum and colors of a galaxy when only stars below a luminosity L_min are cloaked. I find the photometric signatures of galaxies with L_min <= 1 L_sun are minor, especially for blue, galaxies with continuing star formation. Larger luminosity thresholds (>~ 30 L_sun) result in galaxies with unnatural colors and luminosities. Galaxies observed in NIR and galaxies without recent star formation observed at UV-NIR wavelengths become redder than…
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