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Searching for electromagnetic counterpart of LIGO gravitational waves in the Fermi GBM data with ADWO

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arxiv 1603.06611 v2 pith:RNTIACBG submitted 2016-03-21 astro-ph.HE astro-ph.IMgr-qcphysics.data-an

Searching for electromagnetic counterpart of LIGO gravitational waves in the Fermi GBM data with ADWO

classification astro-ph.HE astro-ph.IMgr-qcphysics.data-an
keywords dataadwoanalysiselectromagneticfermigravitationalcounterpartdetector
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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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.

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