NSF award 2514216 · Temple University

WoU-MMA: Multi-TeV, Multi-Messenger, and Multi-Wavelength Particle Astrophysics with HAWC

Final report due

30 March 2027

in 163 days · The award ends on 30 November 2026.

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No-cost extension notice20 Nov 2026in 33 days
award ending 2026-11-30 · Research.gov
PAPPG 24-1: “at least ten calendar days prior to the end date”
Final report due30 Mar 2027in 163 days
award ending 2026-11-30 · Research.gov
PAPPG 24-1: “no later than 120-days following the end date of the award”
Project outcomes report due30 Mar 2027in 163 days
award ending 2026-11-30 · Research.gov
PAPPG 24-1: “no later than 120 days following the end date”
Award is closed out30 Mar 2027in 163 days
award ending 2026-11-30 · 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 30 November 2026.
NSF rules say the final report is due no later than 120 days after that.
So the final report is due by 30 March 2027.

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Award card

Award number: 2514216
Period of support: 1 Sep 2025 – 30 Nov 2026
Amount: $200,000
Awardee: Temple University, Philadelphia, PA
Program: Particle Astrophysics/Cosmic P, WoU-Windows on the Universe: T
Directorate: MPS

Abstract

Gamma rays are the most energetic form of light in the universe. By studying them, this project seeks to understand some of the most energetic and mysterious cosmic phenomena, including exploding stars and black holes. One of the central questions in high-energy astrophysics is how subatomic particles traveling through space at nearly the speed of light, known as “cosmic rays,” reach extraordinarily high energies.…

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