Searching for electromagnetic counterpart of LIGO gravitational waves in the Fermi GBM data with ADWO
arXiv:1603.06611 · doi:10.1051/0004-6361/201628569
Abstract
The Fermi collaboration identified a possible electromagnetic counterpart of the gravitational wave event of September 14, 2015. Our goal is to provide an unsupervised data analysis algorithm to identify similar events in Fermi's Gamma-ray Burst Monitor CTTE data stream. We are looking for signals that are typically weak. Therefore, they can only be found by a careful analysis of count rates of all detectors and energy channels simultaneously. Our Automatized Detector Weight Optimization (ADWO) method consists of a search for the signal, and a test of its significance. We developed ADWO, a virtual detector analysis tool for multi-channel multi-detector signals, and performed successful searches for short transients in the data-streams. We have identified GRB150522B, as well as possible electromagnetic candidates of the transients GW150914 and LVT151012. ADWO is an independently developed, unsupervised data analysis tool that only relies on the raw data of the Fermi satellite. It can therefore provide a strong, independent test to any electromagnetic signal accompanying future gravitational wave observations.
4 pages and 4 figures, A&A Letters accepted
References in corpus (12)
- Observation of Gravitational Waves from a Binary Black Hole Merger
- Astrophysical Implications of the Binary Black-Hole Merger GW150914
- A new route towards merging massive black holes
- GW150914: First results from the search for binary black hole coalescence with Advanced LIGO
- Fermi GBM Observations of LIGO Gravitational Wave event GW150914
- Rotational mixing in massive binaries: detached short-period systems
- Short Gamma-Ray Bursts from the Merger of Two Black Holes
- INTEGRAL upper limits on gamma-ray emission associated with the gravitational wave event GW150914
- High-energy electromagnetic offline follow-up of LIGO-Virgo gravitational-wave binary coalescence candidate events
- Fermi-LAT Observations of the LIGO event GW150914
- Swift follow-up of the Gravitational Wave source GW150914
- GLAST: physics goals and instrument status
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- Searching the Gamma-ray Sky for Counterparts to Gravitational Wave Sources: Fermi GBM and LAT Observations of LVT151012 and GW151226
- Testing Isotropic Universe Using the Gamma-Ray Burst Data of Fermi / GBM
- Probing extra dimension through gravitational wave observations of compact binaries and their electromagnetic counterparts
- Binary Black Hole Mergers within the LIGO Horizon: Statistical Properties and prospects for detecting Electromagnetic Counterparts
- Role of supergiants in the formation of globular clusters
- Probing intrinsic properties of short gamma-ray bursts with gravitational waves
- Supergiants and their shells in young globular clusters
- Some statistical remarks on GRBs jointly detected by Fermi and Swift satellites