GROWTH on S190426c II: GROWTH-India Telescope search for an optical counterpart with a custom image reduction and candidate vetting pipeline
arXiv:2209.02077 · doi:10.1093/mnras/stac2516
Abstract
S190426c / GW190426_152155 was the first probable neutron star - black hole merger candidate detected by the LIGO-Virgo Collaboration. We undertook a tiled search for optical counterparts of this event using the 0.7m GROWTH-India Telescope. Over a period of two weeks, we obtained multiple observations over a 22.1 deg^2 area, with a 17.5% probability of containing the source location. Initial efforts included obtaining photometry of sources reported by various groups, and a visual search for sources in all galaxies contained in the region. Subsequently, we have developed an image subtraction and candidate vetting pipeline with ~ 94% efficiency for transient detection. Processing the data with this pipeline, we find several transients, but none that are compatible with kilonova models. We present the details of our observations, working of our pipeline, results from the search, and our interpretations of the non-detections that will work as a pathfinder during the O4 run of LVK.
12 pages, 6 figures, Accepted for publication in Monthly Notices of the Royal Astronomical Society
References in corpus (23)
- GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral
- Multi-messenger Observations of a Binary Neutron Star Merger
- Gravitational Waves and Gamma-rays from a Binary Neutron Star Merger: GW170817 and GRB 170817A
- Advanced LIGO
- An Ordinary Short Gamma-Ray Burst with Extraordinary Implications: Fermi-GBM Detection of GRB 170817A
- Swope Supernova Survey 2017a (SSS17a), the Optical Counterpart to a Gravitational Wave Source
- Spectroscopic identification of r-process nucleosynthesis in a double neutron star merger
- Light Curves of the Neutron Star Merger GW170817/SSS17a: Implications for R-Process Nucleosynthesis
- Illuminating Gravitational Waves: A Concordant Picture of Photons from a Neutron Star Merger
- Constraining the Maximum Mass of Neutron Stars From Multi-Messenger Observations of GW170817
- Swift and NuSTAR observations of GW170817: detection of a blue kilonova
- GW170817: Joint Constraint on the Neutron Star Equation of State from Multimessenger Observations
- A Radio Counterpart to a Neutron Star Merger
- The discovery of the electromagnetic counterpart of GW170817: kilonova AT 2017gfo/DLT17ck
- Kilonova Light Curves from the Disk Wind Outflows of Compact Object Mergers
- Integrated Nucleosynthesis in Neutrino Driven Winds
- Data-driven expectations for electromagnetic counterpart searches based on LIGO/Virgo public alerts
- Simulations of early kilonova emission from neutron star mergers
- Light-curve models of black hole - neutron star mergers: steps towards a multi-messenger parameter estimation
- Comparing inclination dependent analyses of kilonova transients
- Target of Opportunity Observations of Gravitational Wave Events with Vera C. Rubin Observatory
- Measuring the Hubble Constant with a sample of kilonovae
- 2900 square degree search for the optical counterpart of short gamma-ray burst GRB 180523B with the Zwicky Transient Facility
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