NSF award 2606531 · Princeton University

Collaborative Research: The mass profiles of dwarf galaxies with the Rubin Observatory

Final report due

29 December 2029

in 1,168 days · The award ends on 31 August 2029.

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award ending 2029-08-31 · Research.gov
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award ending 2029-08-31 · Research.gov
PAPPG 24-1: “at least ten calendar days prior to the end date”
Final report due29 Dec 2029in 1168 days
award ending 2029-08-31 · Research.gov
PAPPG 24-1: “no later than 120-days following the end date of the award”
Project outcomes report due29 Dec 2029in 1168 days
award ending 2029-08-31 · Research.gov
PAPPG 24-1: “no later than 120 days following the end date”
Award is closed out29 Dec 2029in 1168 days
award ending 2029-08-31 · Research.gov
PAPPG 24-1: “financially closed out 120 days after their expiration date”

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NSF lists this award's end date as 31 August 2029.
NSF rules say the final report is due no later than 120 days after that.
So the final report is due by 29 December 2029.

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Award card

Award number: 2606531
Period of support: 1 Sep 2026 – 31 Aug 2029
Amount: $510,337
Awardee: Princeton University, Princeton, NJ
Program: EXTRAGALACTIC ASTRON & COSMOLO, Simonyi-NSF Scholars
Directorate: MPS

Abstract

Most of the matter in the universe is invisible "dark matter," whose nature remains one of the deepest open questions in physics. Dwarf galaxies — the smallest and most numerous galaxies — are among the most sensitive laboratories for understanding what dark matter is and how galaxies form, because competing theories differ most in their predictions for these tiny systems. Yet dwarf galaxies are faint and difficult…

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