RATIR Followup of LIGO/Virgo Gravitational Wave Events
arXiv:1706.03898 · doi:10.3847/1538-4357/aab665
Abstract
Recently we have witnessed the first multi-messenger detection of colliding neutron stars through Gravitational Waves (GWs) and Electromagnetic (EM) waves (GW170817), thanks to the joint efforts of LIGO/Virgo and Space/Ground-based telescopes. In this paper, we report on the RATIR followup observation strategies and show the results for the trigger G194575. This trigger is not of astrophysical interest; however, is of great interests to the robust design of a followup engine to explore large sky error regions. We discuss the development of an image-subtraction pipeline for the 6-color, optical/NIR imaging camera RATIR. Considering a two band ( and ) campaign in the Fall of 2015, we find that the requirement of simultaneous detection in both bands leads to a factor 10 reduction in false alarm rate, which can be further reduced using additional bands. We also show that the performance of our proposed algorithm is robust to fluctuating observing conditions, maintaining a low false alarm rate with a modest decrease in system efficiency that can be overcome utilizing repeat visits. Expanding our pipeline to search for either optical or NIR detections (3 or more bands), considering separately the optical and NIR bands, should result in a false alarm rate and an efficiency . RATIR's simultaneous optical/NIR observations are expected to yield about one candidate transient in the vast 100 LIGO error region for prioritized followup with larger aperture telescopes.
10 pages, 8 figures, 1 table, Accepted to AJ
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- GROWTH on S190425z: Searching thousands of square degrees to identify an optical or infrared counterpart to a binary neutron star merger with the Zwicky Transient Facility and Palomar Gattini IR
- GROWTH on S190510g: DECam Observation Planning and Follow-Up of a Distant Binary Neutron Star Merger Candidate
- DDOTI Observations of Gravitational-Wave Sources Discovered in O3
- A strategy for LSST to unveil a population of kilonovae without gravitational-wave triggers