  The Atacama Large Millimetre/submillimetre Array (ALMA) is the world's most
advanced radio interferometric facility, producing science data with an average
rate of about 1 TB per day. After a process of calibration, imaging and quality
assurance, the scientific data are stored in the ALMA Science Archive (ASA),
along with the corresponding raw data, making the ASA an invaluable resource
for original astronomical research. Due to their complexity, each ALMA data set
has the potential for scientific results that go well beyond the ideas behind
the original proposal that led to each observation. For this reason, the
European ALMA Regional Centre initiated the High-Level Data Products initiative
to develop science-oriented data products derived from data sets publicly
available in the ASA, that go beyond the formal ALMA deliverables. The first
instance of this initiative is the creation of a catalogue of submillimetre
(submm) detections of Sloan Digital Sky Survey (SDSS) quasars from the SDSS
Data Release 14 that lie in the aggregate ALMA footprint observed since ALMA
Cycle 0. The ALMA fluxes are extracted in an automatic fashion, using the ALMA
Data Mining Toolkit. All extractions above a signal-to-noise cut of 3.5 are
considered, they have been visually inspected and the reliable detections are
presented in a catalogue of 376 entries, corresponding to 275 unique quasars.
Interesting targets found in the process, i.e. lensed or jetted quasars as well
as quasars with nearby submm counterparts are highlighted, to facilitate
further studies or potential follow up observations.
