NSF award 2605354 · University of California-San Diego

Unveiling the Black Hole Populations of Milky Way Globular Clusters

Final report due

28 January 2030

in 1,198 days · The award ends on 30 September 2029.

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Final report due28 Jan 2030in 1198 days
award ending 2029-09-30 · Research.gov
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Project outcomes report due28 Jan 2030in 1198 days
award ending 2029-09-30 · Research.gov
PAPPG 24-1: “no later than 120 days following the end date”
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So the final report is due by 28 January 2030.

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Award card

Award number: 2605354
Period of support: 1 Oct 2026 – 30 Sep 2029
Amount: $490,197
Awardee: University of California-San Diego, LA Jolla, CA
Program: GALACTIC ASTRONOMY PROGRAM
Directorate: MPS

Abstract

Stellar clusters have emerged as a possible site for black hole binary mergers that would produce gravitational wave sources like those now detected readily by today’s gravitational wave observatories. To test this possible connection, a more robust census of black hole populations and properties in globular clusters is needed. One method for unambiguously identifying a black hole in a globular cluster is via…

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