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The Herschel Reference Survey (HRS) is a guaranteed time Herschel key projectaimed at studying the physical properties of the interstellar medium ingalaxies of the nearby universe. This volume limited, K-band selected sample iscomposed of galaxies spanning the whole range of morphological types (fromellipticals to late-type spirals) and environments (from the field to thecentre of the Virgo Cluster). We present flux density measurements of the wholesample of 323 galaxies of the HRS in the three bands of the Spectral andPhotometric Imaging Receiver (SPIRE), at 250, 350 and 500 microns. Aperturephotometry is performed on extended galaxies and point spread function (PSF)fitting on timeline data for unresolved objects; we carefully estimate errorsand upper limits. The flux densities are found to be in good agreement withthose of the HeViCS and KINGFISH key projects in all SPIRE bands, and of thePlanck consortium at 350 and 550 microns, for the galaxies in common. Thissubmillimetre catalogue of nearby galaxies is a benchmark for the study of thedust properties in the local universe, giving the zero redshift reference forany cosmological survey.

Submillimetre Photometry of 323 Nearby Galaxies from the Herschel Reference Survey