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DOE OSTI · 1841908

Kilonova Detectability with Wide-Field Instruments [Slides]

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. These results are useful for guiding kilonova searches following a GW detection and sGRD observation, proposals for time on current and upcoming instruments, and planning future wide-field instruments.

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79 ASTRONOMY AND ASTROPHYSICS

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BibTeXRIS

Chase, Eve Adde. 2022-01-31. Kilonova Detectability with Wide-Field Instruments [Slides]. https://doi.org/10.2172/1841908

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