NSF award 2511242 · Arizona State University

Characterizing Gas Flow Pathways In High-resolution In the Local Universe

Final report due

29 December 2028

in 803 days · The award ends on 31 August 2028.

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award ending 2028-08-31 · Research.gov
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Extension request17 Jul 2028in 638 days
award ending 2028-08-31 · Research.gov
PAPPG 24-1: “at least 45 days prior to the end date”
No-cost extension notice21 Aug 2028in 673 days
award ending 2028-08-31 · Research.gov
PAPPG 24-1: “at least ten calendar days prior to the end date”
Final report due29 Dec 2028in 803 days
award ending 2028-08-31 · Research.gov
PAPPG 24-1: “no later than 120-days following the end date of the award”
Project outcomes report due29 Dec 2028in 803 days
award ending 2028-08-31 · Research.gov
PAPPG 24-1: “no later than 120 days following the end date”
Award is closed out29 Dec 2028in 803 days
award ending 2028-08-31 · 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 2028.
NSF rules say the final report is due no later than 120 days after that.
So the final report is due by 29 December 2028.

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Award card

Award number: 2511242
Period of support: 1 Sep 2025 – 31 Aug 2028
Amount: $469,850
Awardee: Arizona State University, Scottsdale, AZ
Program: EXTRAGALACTIC ASTRON & COSMOLO
Directorate: MPS

Abstract

Galaxies continuously form stars over billions of years. To keep forming stars during these exceedingly long timescales, galaxies need a fresh supply of gas flowing right into their centers. Gas is the primordial building material of stars. This program will study how gas flows from outside galaxies into their inner regions, sustaining the process of star formation for billions of years. To achieve the main…

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