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  • Chairing the LSST:UK Science Working Group. This group is intended to represent the range of scientific interests of the LSST:UK community and to aid its interaction with the international LSST Science Collaborations. The detailed role of this group, as we approach and enter LSST operations, will be for the incoming Project Scientist to develop.

  • Maintaining of the LSST:UK Science Requirements Document. The SRD translates the high-level goals of the LSST:UK Long-Term Plan into specific scientific requirements for the LUSC work packages. These mainly correspond to in-kind contributions, so their scope is primarily set by their respective Recipient Groups, but the PS, with the assistance of the Project Leader and Science Working Group, is responsible for ensuring their scientific validity.

  • Attending Consortium Board, Executive Group and STFC Oversight Committee meetings. The PS is responsible for representing the UK community’s science interests in these meetings, and for ensuring that these bodies are provided with sufficient scientific advice to make decisions on science-based matters.

  • Leading the Community Scientist aspect of the UK in-kind programme. The Community Scientist scheme will provide effort to the Rubin Community Science Team (CST) through secondment of UK researchers. It is intended to be beneficial both to the Rubin CST, by providing it with additional effort located in a European time-zone, and to the UK community, by providing a conduit through which expertise from the Rubin CST can be disseminated through UK institutions. This in-kind contribution has not yet started, and the profiling of its effort will be determined by the incoming PS, in conjunction with Melissa Graham, who leads the Rubin CST.

  • Providing a scientific interface between LSST:UK and the Rubin Observatory. The PS is responsible for ensuring that the Rubin Observatory is kept apprised of the scientific priorities of the UK community. For example, the PS is expected to accept invitations to join Rubin committees (e.g., the Science Advisory Committee, the Survey Cadence Optimisation Committee, the Users Committee) and/or secure UK representation on them from suitable members of the LSST:UK community. More generally, the PS will identify when opportunities arise for members of the UK community to contribute scientific expertise to Rubin activities.

  • Promoting Rubin and LSST to the UK astronomical community. The PS will enhance the prominence of the Rubin LSST within the UK astronomical community and, hence, expand the scientific return that the community derives from the survey. This will include providing support for the organisation of LSST-specific science meetings, and promoting the Rubin LSST and LSST:UK at other scientific meetings (e.g., related to synergistic programmes) and through talks at UK institutions.

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