Chua, SheonInta, RaLam, Ping KoyMcClelland, DavidMiller, JohnMow-Lowry, C.Mullavey, AdamScott, Susan M.Shaddock, DanielSlagmolen, BramStefszky, MichaelWade, AndrewMarka, S.LIGO, Scientific Collaboration (700 Scientists)VIRGO, Scientific Collaboration (numerous Scientists)2015-12-082015-12-080264-9381http://hdl.handle.net/1885/28833Comprehensive multimessenger astronomy with gravitational waves is a pioneering field bringing us interesting results and presenting us with exciting challenges for the future. During the era of the operation of advanced interferometric gravitational wave detectors, we will have the opportunity to investigate sources of gravitational waves that are also expected to be observable through other messengers, such as gamma rays, x-rays, optical, radio, and/or neutrino emission. Multimessenger searches for gravitational waves with the LIGO-GEO600-Virgo interferometer network have already produced insights on cosmic events and it is expected that the simultaneous observation of electromagnetic or neutrino emission could be a crucial aspect for the first direct detection of gravitational waves in the future. Trigger time, direction and expected frequency range enhances our ability to search for gravitational wave signatures with amplitudes closer to the noise floor of the detector. Furthermore, multimessenger observations will enable the extraction of otherwise unaccessible scientific insight. We summarize the status of transient multimessenger detection efforts as well as mention some of the open questions that might be resolved by advanced or third generation gravitational wave detector networks.201110.1088/0264-9381/28/11/1140132019-11-25