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DOE OSTI · 1843166

Kilonova Detectability with Wide-Field Instruments

Chase, Eve Adde
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Abstract

A diverse set of instruments increase the chances of detecting and identifying a kilonova. Early observations increase the probability of detection. More sensitive wide-field ultraviolet instruments are needed as GW detectors reach design sensitivity. There is a dearth of wide-field infrared instruments.

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79 ASTRONOMY AND ASTROPHYSICSAstronomy and Astrophysics

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Chase, Eve Adde. 2022-02-07. Kilonova Detectability with Wide-Field Instruments. https://doi.org/10.2172/1843166

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