← LeaderboardsInvestigatorsiAttributed = a PI's even-split share of each grant — a $1M grant with 2 PIs counts $500K each.
The Corporation Of Haverford College
$697,466
Total funding
9
Grants
Funding over time
peak $349.8K · FY2020–22$500K$375K$250K$125K$0
'20
'21
'22
Funding mix
By agency
NASA$697,466 · 9
By mechanism
—$697,466 · 9
Investigators at The Corporation Of Haverford College
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
THE GLOBAL IONOSPHERE ELECTRIC FIELD VARIES CONSIDERABLY LONGITUDINALLY AND FROM DAY-TO-DAY BUT THE CAUSES OF THESE CHANGES ARE NOT WELL UNDERSTOOD. THE MAIN PROCESSES THAT PRODUCE ELECTRIC FIELDS INCLUDE:$247,983
· FY2020 · National Aeronautics and Space Administration
WE ARE REQUESTING $134 083 OVER THE 11-MONTH PERIOD BEGINNING NOVEMBER 1 2021 TO CONTRIBUTE SIGNIFICANTLY TO THE NICER SCIENCE GOALS WITH TIMING PRECISION PROFILE STABILITY LIGHTCURVE MODELING MAGNETARS MAGNETOSPHERES AND PULSATION SEARCHES.$134,083
· FY2022 · National Aeronautics and Space Administration
MONITORING X-RAY PULSARS FOR GRAVITATIONAL WAVE SEARCHES NICER GUEST OBSERVER CYCLE 4$87,964
· FY2022 · National Aeronautics and Space Administration
WE PROPOSE TO PERFORM MONITORING CAMPAIGNS FOR FIVE PULSARS FOUR OF WHICH CAN ONLY BE DONE VIA X-RAY OBSERVATIONS. OUR REQUESTED TOTAL EXPOSURE TIMES ARE 260 KS FOR PSR J0537-6910 48 KS FOR PSR J1412+7922 294 KS FOR PSR J1813-1749 60 KS FOR PSR J1849-0001 AND 200 KS FOR PSR J2229+6114. THESE DATA WILL ALLOW US TO COMPUTE ACCURATE PHASE-CONNECTED TIMING MODELS FOR EACH PULSAR WHICH WILL ENABLE LIGO/VIRGO TO PERFORM SEARCHES OF GRAVITATIONAL WAVES FROM THESE MOSTLY YOUNG AND POTENTIALLY STRONGER GRAVITATIONALWAVE EMITTING PULSARS. OUR PROPOSED OBSERVATIONS WILL OCCUR CONTEMPORANEOUSLY WITH LIGO/VIRGO'S NEXT MOST SENSITIVE OBSERVING RUN WHICH BEGINS IN SPRING 2019. IN ADDITION OUR HIGH CADENCE OBSERVATIONS OF PSR J0537-6910 WILL PROVIDE AN OPPORTUNITY TO FURTHER PIN-DOWN AND TEST THIS PULSAR'S UNIQUE GLITCH PREDICTABILITY AND TO MEASURE POTENTIAL X-RAY SIGNATURES ASSOCIATED WITH GLITCHES.$53,945
· FY2020 · National Aeronautics and Space Administration
STELLAR OSCILLATION MODES KNOWN AS R-MODES CAN CONVERT ROTATIONAL ENERGY OF FAST SPINNING NEUTRON STARS INTO GRAVITATIONAL WAVES AND INTERNAL HEATING. BY MEASURING X-RAY FLUX FROM THE HOT SURFACE OF RAPIDLY ROTATING PULSARS WE CAN CONSTRAIN THE PHYSICS THAT GOVERN R-MODES SUCH AS THE STATE OF NUCLEAR MATTER. WITH A SPIN RATE OF 707 HZ PSR J0952-0607 IS THE FASTEST-SPINNING PULSAR KNOWN OUTSIDE A GLOBULAR CLUSTER. THE LOW INTERVENING NH (4 X 1020 CM-2) AND SMALL SOURCE DISTANCE (0.97-1.74 KPC) INDICATE THAT AN XMM-NEWTON OBSERVATION CAN SIGNIFICANTLY IMPROVE UPON THE X-RAY FLUX CONSTRAINT OBTAINED BY SWIFT. PSR J0952-0607 IS THUS AN EXCELLENT TARGET FOR INVESTIGATING WHAT LIMITS THE SPIN EVOLUTION OF MILLISECOND PULSARS. FINALLY MODELING OF A NONTHERMAL COMPONENT OF THE X-RAY SPECTRUM CAN YIELD VALUABLE INSIGHTS INTO THE INTRABINARY SHOCK BETWEEN PSR J0952-0607 AND ITS COMPANION STAR.$47,921
· FY2020 · National Aeronautics and Space Administration
E014042 - TIMING OBSERVATIONS OF MEV PULSARS PSR J1838 AND PSR J1846$37,480
· FY2022 · National Aeronautics and Space Administration
WE PROPOSE MONITORING OBSERVATIONS OF THE YOUNG HIGHLY ENERGETIC PULSARS PSR J1838-0655 AND PSR J1846-0258. THESE SOURCES ARE ONLY EASILY DETECTABLE AS PULSARS AT X-RAY ENERGIES WHICH MAKES NICER THE IDEAL INSTRUMENT TO CONDUCT THE NECESSARY OBSERVATIONS.$37,477
· FY2021 · National Aeronautics and Space Administration
WE PROPOSE MONITORING CAMPAIGNS FOR FIVE PULSARS FOUR OF WHICH CAN ONLY BE DONE VIA X-RAY OBSERVATIONS USING NICER WITH TOTAL EXPOSURE TIMES OF 520 KS FOR PSR J0537-6910 300 KS FOR PSR J1101-6101 48 KS FOR PSR J1412+7922 60 KS FOR PSR J1849-0001 AND 200 KS FOR PSR J2229+6114.$25,309
· FY2021 · National Aeronautics and Space Administration
WE PROPOSE MONITORING CAMPAIGNS FOR FIVE PULSARS FOUR OF WHICH CAN ONLY BE DONE VIA X-RAY OBSERVATIONS USING NICER WITH TOTAL EXPOSURE TIMES OF 520 KS FOR PSR J0537-6910 300 KS FOR PSR J1101-6101 48 KS FOR PSR J1412+7922 60 KS FOR PSR J1849-0001 AND 200 KS FOR PSR J2229+6114. THESE DATA WILL ALLOW US TO COMPUTE ACCURATE PHASE-CONNECTED TIMING MODELS FOR EACH PULSAR WHICH WILL$25,304
· FY2021 · National Aeronautics and Space Administration