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\title{Finding untriggered gamma-ray transients in the Fermi GBM data
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\author{\speaker{Michelle Hui}\\
        NASA/MSFC
 \\
        E-mail: \email{cmhui.astro@gmail.com
}}

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\abstract{
  The all-sky monitoring capability of Fermi GBM makes it ideal for finding transients.  Fermi GBM triggers on events such as gamma-ray bursts, soft gamma-ray repeaters, X-ray bursters, solar flares, and terrestrial gamma-ray flashes.  A  previous systematic search in offline data for X-ray bursts has uncovered untriggered gamma-ray bursts, and currently there is a dedicated offline search pipeline looking for weak transients overlooked by the onboard trigger conditions.  The untargeted search looks for significant background-subtracted signals in two or more detectors at various timescales in the continuous data, detecting ~80 additional short GRB candidates per year.  Since July 2017, these candidates have been published in GCN under Fermi-GBM Subthreshold transients notices, accompanied by localization maps and lightcurves.  At present only short GRB candidates are published, expansion to long GRBs and other transient types are forthcoming.
}

\FullConference{7th Fermi Symposium 2017\\
		15-20 October 2017\\
		Garmisch-Partenkirchen, Germany}


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