This page gathers basic resources that may be useful to ISSC members preparing proposals requesting support for small-team LSST-related projects involving significant data science research.
The main sources of US federal support for LSST-related research are NSF and DOE.
Relevant programs run by NSF include:
- Astronomy and Astrophysics Research Grants (AAG) — Annual, deadline typically in mid-November
- Statistics Grants — Annual, deadline typically in mid-December
- Programs under NSF's Harnessing the Data Revolution (HDR) theme, one of NSF's 10 Big Ideas (note that LSST-related research also falls under the Windows on the Universe theme, but that theme has no dedicated programs)
- Programs under the Directorate for Computer and Information Science and Engineering (CISE)
This list is not exhaustive; in particular, NSF occasionally announces short-lived grant opportunities not listed here.
DOE supports the construction of the LSST camera. DOE's science support for LSST mainly focuses on dark energy and dark matter research. See the DOE Office of Science Funding, specifically their annual funding opportunity announcements. Note that DOE opportunities often have more strict eligibility requirements than NSF opportunities (e.g., PIs may have to hold tenured or tenure-track positions).
The LSST Project runs the telescope and the Data Management effort; it is federally funded. The LSST Corporation (LSSTC) is a not-for-profit corporation that helped initiate the project, and that raises philanthropic funding to help the project succeed. LSSTC occasionally solicits proposals for small research projects; see their Enabling Science page for more information.
LSST information for proposers
- LSST Project Schedule — Note that SC members will have access to some data during the Science Verification period. Also note that the schedule includes a significant contingency period. As of late 2019, the expectation is that much of the contingency will be needed to make up for unanticipated construction delays.
- LSST System & Survey Key Numbers — The latest estimates of basic survey information, including telescope properties, observation properties, and data release properties including catalog sizes and expected data volume.
- LSST Science Book — Although it dates from 2009, this book, prepared by the project team and the science collaborations, remains the most comprehensive overview of the science goals and capabilities of LSST. Note that the ISSC did not exist when the book was prepared. Note, too, that some quantitative information in the book may be out of date.
- LSST Publications — This section of LSST.org archives numerous reports, papers, and presentations prepared by project members. It includes technical reports on the design and capabilities of elements of the telescope and data management system. See especially the section with Key Project Documents.
Three publications likely to be especially useful are these:
- LSST: From Science Drivers To Reference Design And Anticipated Data Products — This paper is the official description of LSST's goals and planned capabilities. It first appeared on arXiv in 2008, but it has been regularly updated since then. The 2019 version has been published in ApJ: ADS entry (with BibTeX). Further information about LSST's science requirements and data products are in reports in the "Key Project Documents" archive cited above.
- Keith Bechtol's presentation for the Feb 2018 workshop, "NOAO Community Needs for Science in the 2020s," organized in preparation for the Astro2020 decadal survey: "Science with LSST". This slide deck include more information about the "key numbers" referenced above, including current estimates of the numbers of stars and galaxies LSST will observe. It also briefly describes the LSST Science Platform (for co-located data analysis) and survey cadence considerations.
- Summary of Data Management Principles — If your proposal requires a data management plan that needs to describe LSST's own data management principles, you may want to cite this report.
Thanks in part to support from DOE, the Dark Energy Science Collaboration (DESC) has been especially active in this pre-survey preparation period. If your work is relevant for cosmology (including some topics in extragalactic astronomy and transient and variable star astronomy), these documents hosted at the LSST DESC public website may be useful (DESC also maintains a very extensive collaboration-only website with lots more):
These and other related documents are collected on DESC's Information for Collaborators page.
LSSTC hosts a Confluence site where community members share and maintain various information sources. It includes two glossaries proposers may find useful (especially data scientists unfamiliar with some astronomical terminology):
- LSST Astro Glossary — Covers astronomical terms, or other LSST terms related to the astronomy domain.
- LSST Data Management System (DMS) Glossary — Covers terms used by the DMS
As examples of what you'll find in the Astro Glossary, note the specific ways that "object" and "source" are used in LSST publications:
- Object: Refers to an astronomical object, such as a star, galaxy, asteroid, or other physical entity. Objects can be static, or change brightness or position with time. Generally an object will be associated with more than one instance of a source detection
- Source: A single detection of an astrophysical object in an image, the characteristics for which are stored in the Source Catalog of the science database. The Data Management System attempts to associate multiple source detections to single objects, which may vary in brightness or position over time.