Electromagnetic Follow-up to Gravitational Wave Events with the UltraViolet EXplorer (UVEX)

Abstract The Ultraviolet Explorer (UVEX) is expected to fly in 2030 and will have the opportunity—and the rapid near/far-ultraviolet (UV) capabilities—to glean unprecedented insight into the bright UV emission present in kilonovae like that of AT 170817gfo, the electromagnetic counterpart to binary neutron star merger GW170817. To do so, it will need to perform prompt target-of-opportunity observations following detection of binary neutron star mergers by the LIGO–Virgo–KAGRA gravitational observatories. We present initial simulations to develop UVEX target-of-opportunity strategies for such events and provide the community with detailed initial estimates of the prospects for and characteristics of UVEX target-of-opportunity observations following gravitational-wave events, considering fiducial scenarios for the fifth and sixth LIGO–Virgo–KAGRA observing runs. Additionally, in light of the relatively few binary neutron star mergers observed since GW170817, we consider variant target-of-opportunity strategies for UVEX to maximize scientific gain in the case of a lowered binary neutron star merger rate.

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Publication Details

Journal
Publications of the Astronomical Society of the Pacific
Published
2025-05-01
DOI
https://doi.org/10.1088/1538-3873/adcd9c
Citations
2
Primary Topic
Pulsars and Gravitational Waves Research
Type
article
Field-Weighted Citation Impact
2.31

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article

Electromagnetic Follow-up to Gravitational Wave Events with the UltraViolet EXplorer (UVEX)

A. W. Criswell, W. Kiendrébéogo, L. P. Singer, Andrew Toivonen et al.
2 citations
Publications of the Astronomical Society of the Pacific
Pulsars and Gravitational Waves Research
2.31
article

Electromagnetic Follow-up to Gravitational Wave Events with the UltraViolet EXplorer (UVEX)

A. W. Criswell, W. Kiendrébéogo, L. P. Singer, Andrew Toivonen, Hannah P. Earnshaw, Brian W. Grefenstette, M. W. Coughlin, Igor Andreoni, Fiona A. Harrison, Suvi Gezari, M. M. Kasliwal, Sydney C Leggio
article en
2 citations

Abstract

Abstract The Ultraviolet Explorer (UVEX) is expected to fly in 2030 and will have the opportunity—and the rapid near/far-ultraviolet (UV) capabilities—to glean unprecedented insight into the bright UV emission present in kilonovae like that of AT 170817gfo, the electromagnetic counterpart to binary neutron star merger GW170817. To do so, it will need to perform prompt target-of-opportunity observations following detection of binary neutron star mergers by the LIGO–Virgo–KAGRA gravitational observatories. We present initial simulations to develop UVEX target-of-opportunity strategies for such events and provide the community with detailed initial estimates of the prospects for and characteristics of UVEX target-of-opportunity observations following gravitational-wave events, considering fiducial scenarios for the fifth and sixth LIGO–Virgo–KAGRA observing runs. Additionally, in light of the relatively few binary neutron star mergers observed since GW170817, we consider variant target-of-opportunity strategies for UVEX to maximize scientific gain in the case of a lowered binary neutron star merger rate.

Publications of the Astronomical Society of the PacificVol. 137(5)
University of North Carolina at Chapel Hill (US), California Institute of Technology (US), Université Joseph Ki-Zerbo (BF), Space Telescope Science Institute (US), University of Minnesota (US), Goddard Space Flight Center (US), Johns Hopkins University (US), Vanderbilt University (US), Université Côte d'Azur (FR), Physical Sciences (United States) (US), Université Bourgogne Franche-Comté (FR), Observatoire de la Côte d’Azur (FR), Fisk University (US)
National Science Foundation, University of Minnesota, University of Illinois at Urbana-Champaign, Office of Advanced Cyberinfrastructure
Openalex Percentile: Top 12%
Pulsars and Gravitational Waves Research
2.31
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