← LeaderboardsInvestigatorsiAttributed = a PI's even-split share of each grant — a $1M grant with 2 PIs counts $500K each.
Associated Universities Inc
$2,031,513
Total funding
11
Grants
Funding over time
peak $1M · FY2016–23$2M$1.5M$1M$500K$0
'16
'17
'18
'19
'20
'21
'22
'23
Funding mix
By agency
DOD$1,180,115 · 2
NASA$851,398 · 9
By mechanism
—$2,031,513 · 11
Investigators at Associated Universities Inc
InvestigatorsiAttributed = a PI's even-split share of each grant — a $1M grant with 2 PIs counts $500K each.
Exposure= the full size of every grant they're on ($1M each).
Rising Stars
First grant in the last 5 yrs
Not enough data
Emerging Leaders
6–10 yrs in
Not enough data
All-Time
Most funded here, all years
Not enough data
Largest grants
SUPPORTING AND ENHANCING THE VLA LOW BAND IONOSPHERIC AND TRANSIENT EXPERIMENT$1,047,940
· FY2023 · Department of the Navy
NASA'S SPITZER SPACE TELESCOPE AND THE WIDE-FIELD INFRARED SURVEY EXPLORER (WISE) HAVE IDENTIFIED THOUSANDS OF DISKS SPANNING THE SPECTRUM OF STELLAR$343,927
· FY2016 · National Aeronautics and Space Administration
EO14042 CHARACTERIZING PROTOSTELLAR DISK STRUCTURE AT THE DAWN OF PLANET FORMATION$235,791
· FY2022 · National Aeronautics and Space Administration
SUPPORTING AND ENHANCING THE EXPANDED VLA LOW BAND IONOSPHERIC AND TRANSIENT EXPERIMENT$132,175
· FY2018 · Department of the Navy
THE NICER MISSION, IN PREPARATION FOR LAUNCH IN EARLY 2017, WISHES TO ENGAGE ITS APPROVED COINVESTIGATORS FOR PLANNING OF CALIBRATION AND ASTROPHYSIC$82,263
· FY2016 · National Aeronautics and Space Administration
EO14042 NUSTAR CYCLE 7 TIME WAS AWARDED TO OBSERVE THREE UITRALUMINOUS INFRARED GALAXIES (ULIRGS) TO FINISH A STATISTICALLY COMPLETE SAMPLE OF LOW-REDSHIFT ULIRGS WITH HARD X-RAY OBSERVATIONS. THIS PROJECT SUPPORTS THE REDUCTION AND ANALYSIS OF THE$77,070
· FY2022 · National Aeronautics and Space Administration
FERMI HAS HAD A SPECTACULAR IMPACT ON PULSAR RESEARCH, AND MILLISECOND PULSARS (MSPS) IN PARTICULAR. IN THE PAST 7 YEARS, ASTRONOMERS HAVE DISCOVERED$59,756
· FY2016 · National Aeronautics and Space Administration
WE ARE DEVELOPING A BETTER WAY TO TIME GAMMA-RAY PULSARS USING INDIVIDUAL PHOTONS. LEVERAGING NEW TIMING SOFTWARE (PINT) AND MCMC OUR "BETA" CODE CAN TIME LAT PULSARS THAT WERE PREVIOUSLY IMPOSSIBLE. USING EACH PHOTON ALLOWS US TO DETECT SHORT-TERM EFFECTS (LIKE ORBITAL SHAPIRO DELAY) WHICH TRADITIONAL METHODS AVERAGE OUT. WE PROPOSE TO DEVELOP AND EXTEND THESE TECHNIQUES AND MAKE THE CODE AVAILABLE TO THE COMMUNITY. THIS WORK WILL IMPROVE GAMMA-RAY DETECTIONS FOR PULSARS WITH SHORT RADIO TIMING BASELINES OR SIGNIFICANT TIMING NOISE WILL MEASURE NEW PROPER MOTIONS AND MAY ALLOW US TO INCORPORATE THE BEST MSPS INTO GRAVITATIONAL WAVE SEARCHES. WE WILL UPDATE OUR EXISTING LAT TIMING PIPELINE (DOUBLING THE NUMBER OF TIMED PULSARS) AND PROVIDE UPDATED TIMING MODELS TO THE COMMUNITY.$27,053
· FY2020 · National Aeronautics and Space Administration
ULTRALUMINOUS INFRARED GALAXIES (ULIRGS LIR > 10^12 LSUN) ARE THE MOST INTRINSICALLY LUMINOUS GALAXIES IN THE LOW-REDSHIFT UNIVERSE YET THE POWER SOURCE OF ULIRGS (AGN VS STARBURST) IS STILL DEBATED. WE PROPOSE NUSTAR OBSERVATIONS OF 7 LOCAL ULIRGS$19,539
· FY2021 · National Aeronautics and Space Administration
THE FERMI MISSION HAS USED IT SPECTRAL AND SPATIAL RESOLUTION TO GREAT AFFECT TO STUDY THE SITES OF COSMIC RAY ACCELERATION IN GALACTIC SUPERNOVA REM$6,000
· FY2016 · National Aeronautics and Space Administration
PI (G. PRIVON) WILL SUPERVISE THE WORK OF A POSTDOCTORAL SCHOLAR. HE WILL ALSO COORDINATE ACCESS TO EXISTING ANCILLARY DATA ON THE TARGET GALAXIES. POSTDOCTORAL SCHOLAR (TBD) AT THE NATIONAL RADIO ASTRONOMY OBSERVATORY WILL CON- TINUE THE REDUCTION AND ANALYSIS OF THE COMPLETED CYCLE 4 OBSERVATIONS OF NGC 7252. THE POSTDOCTORAL SCHOLAR WILL LEAD THE WRITEUP AND PUBLICATION OF THE RESULTS OF THE STUDY.$0
· FY2021 · National Aeronautics and Space Administration