A challenge to identify an optical counterpart of the gravitational wave event GW151226 with Hyper Suprime-Cam

on behalf of the J-GEM collaboration

Research output: Contribution to journalArticle

5 Citations (Scopus)

Abstract

We present the results of detailed analysis of an optical imaging survey conducted using the Subaru/Hyper Suprime-Cam (HSC) that aimed to identify an optical counterpart to the gravitational wave event GW151226. In half a night, the i- and z-band imaging survey by HSC covered 63.5 deg 2 of the error region, which contains about 7% of the LIGO localization probability, and the same fieldwas observed in three different epochs. The detectable magnitude of the candidates in a differenced image is evaluated as i ∼ 23.2 mag for the requirement of at least two 5 σ detections, and 1744 candidates are discovered. Assuming a kilonova as an optical counterpart, we compare the optical properties of the candidates with model predictions. A red and rapidly declining light curve condition enables the discrimination of a kilonova from other transients, and a small number of candidates satisfy this condition. The presence of stellar-like counterparts in the reference frame suggests that the surviving candidates are likely to be flare stars. The fact that most of those candidates are in the galactic plane, |b| < 5°, supports this interpretation. We also check whether the candidates are associated with the nearby GLADE galaxies, which reduces the number of contaminants even with a looser color cut. When a better probability map (with localization accuracy of ∼50 deg 2 ) is available, kilonova searches of up to approximately 200 Mpc will become feasible by conducting immediate follow-up observations with an interval of 3.6 d.

Original languageEnglish
Article number1
JournalPublications of the Astronomical Society of Japan
Volume70
Issue number1
DOIs
Publication statusPublished - 2018 Jan 1

Keywords

  • Gravitational waves
  • stars: black holes
  • stars: neutron

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

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