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Data · dataset · 2026

Discovering and characterising compact mergers in wide-field surveys

Listed in ZivaHub and Deakin Research Online and DMU Figshare and UCL Research Data Repository — shown once because both records carry DOI 10.17034/32631444.v1

This thesis concentrates on efforts to identify and characterize compact mergers involving neutron stars using wide-field survey instruments.

Description

With the Panoramic Survey Telescope and Rapid Response System (Pan-STARRS) and the Asteroid Terrestrial-impact Last Alert System (ATLAS), searches for compact mergers, including kilonovae, have been performed. The Pan-STARRS search identified two rapidly evolving transients with similar decline rates to the first kilonova, AT2017gfo, in PS15cey and PS17cke.

While model fits of black hole-neutron star mergers can match the peak luminosity of PS15cey, a kilonova interpretation is less likely than a rapidly evolving supernova. PS17cke may be a plausible kilonova candidate, however, based on supporting modelling. The ATLAS search has returned no plausible kilonova candidates, but has identified a unique optical transient in AT2018kzr whose peak luminosity and rapid decline are difficult to describe using a traditional Nickel-56 driven explosion models.

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This necessitates the inclusion of an additional powering source, such as the spin-down of a magnetic neutron star remnant, to provide a plausible model fit to the bolometric lightcurve. Spectral modelling suggests the object is characterised by intermediate mass elements (including oxygen, silicone and magnesium) which disfavours a neutron star-neutron star merger scenario, but is consistent with predictions of white dwarfneutron star mergers.

The lack of a kilonova detection by ATLAS has prompted the development of an efficiency simulation to understand the challenges of observing rapidly evolving and intrinsically faint transients with all-sky survey telescopes. Such a simulation has been used to constrain the volumetric rate of AT2017gfo-like transients in the local universe, with the results being consistent with other optically-derived rates estimates and rate of binary neutron star mergers measured gravitational wave observatories.

Given the available information, it is predicted ATLAS will need to continue observing for at least a decade in order to observe a kilonova.

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Where it is published

Catalogue records · 1

Topics

Inferred from text
Geoinformatics 69% · Simulation 75%
Provenance · 4 source records, 10 field assertions
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ZivaHuboai:figshare.com:article/326314445 d agoJSON v1
Deakin Research Onlineoai:figshare.com:article/326314445 d agoJSON v1
DMU Figshareoai:figshare.com:article/326314445 d agoJSON v1
UCL Research Data Repositoryoai:figshare.com:article/326314445 d agoJSON v1
FieldAssertionExtractorEvidence
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