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We introduce the New-ANGELS program, an XMM-Newton survey of$\sim7.2\rm~deg^2$ area around M 31, which aims to study the X-ray populationsin M 31 disk and the X-ray emitting hot gas in the inner halo of M 31 up to 30kpc. In this first paper, we report the catalogue of 4506 detected X-raysources, and attempt to cross-identify or roughly classify them. We identify352 single stars in the foreground, 35 globular clusters and 27 supernovaremnants associated with M 31, as well as 62 AGNs, 59 galaxies, and 1 galaxyclusters in the background. We uniquely classify 236 foreground stars and 17supersoft sources based on their X-ray colors. X-ray binaries (83 LMXBs, 1HMXBs) are classified based on their X-ray colors and X-ray variabilities. Theremaining X-ray sources either have too low S/N to calculate their X-ray colorsor do not have a unique classification, so are regarded as unclassified. TheX-ray source catalogue is published online. Study of the X-ray sourcepopulations and the contribution of X-ray sources in the unresolved X-rayemissions based on this catalogue will be published in companion papers.

An XMM-Newton View of the ANdromeda Galaxy as Explored in a Legacy Survey (New-ANGELS) I: the X-ray Source Catalogue