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I present and summarize a software package ("LPipe") for completelyautomated, end-to-end reduction of both bright and faint sources with theLow-Resolution Imaging Spectrometer (LRIS) at Keck Observatory. It supports allgratings, grisms, and dichroics, and also reduces imaging observations,although it does not include multislit or polarimetric reduction capabilitiesat present. It is suitable for on-the-fly quicklook reductions at thetelescope, for large-scale reductions of archival data-sets, and (in manycases) for science-quality post-run reductions of PI data. To demonstrate itscapabilities the pipeline is run in fully-automated mode on all LRIS longslitdata in the Keck Observatory Archive acquired during the 12-month periodbetween August 2016 and July 2017. The reduced spectra (of 675 single-objecttargets, totaling ~200 hours of on-source integration time in each camera), andthe pipeline itself, are made publicly available to the community.

Fully-Automated Reduction of Longslit Spectroscopy with the Low Resolution Imaging Spectrometer at Keck Observatory