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In March 2010 the Large Area Telescope (LAT) on-board the Fermi Gamma-raySpace Telescope discovered for the first time >100 MeV gamma-ray emission froma nova within our galaxy, V407 Cyg. The high-energy spectrum and light curvewas explained as a consequence of shock acceleration in the nova shell as itinteracts with the local ambient medium. It was suspected that the necessaryconditions for high-energy emission from novae would be rare. In June 2012 theLAT detected a new flaring source, Fermi J1750-3243, that is spatiallycoincident and contemporaneous with a new nova, Nova Sco 2012. We report on theexciting discovery of this new 'gamma-ray' nova and present a detailed analysisof its high-energy properties.

The discovery of gamma-ray emission from Nova Sco 2012: An analysis using reprocessed Pass7 data