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Nanohmics Inc

$8,020,051

Total funding

13

Grants

Funding over time

peak $2.5M · FY2008–21

$2.5M$1.9M$1.3M$625K$0

'08

'09

'10

'11

'12

'13

'14

'15

'16

'17

'18

'19

'20

'21

Funding mix

By agency

DOE$6,515,904 · 9

NASA$1,504,147 · 4

By mechanism

—$8,020,051 · 13

Investigators at Nanohmics Inc

Investigator-initiated All funding

Investigatorsi

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

ROBUST, SELECTIVE NOX SPECIES SENSOR FOR TAILPIPE EMISSIONS$2,499,990

· FY2021 · Department of Energy

LOW-COST AND EFFICIENT COOLING OF ON-DETECTOR ELECTRONICS USING CONFORMAL THERMOELECTRIC MODULES$1,206,498

· FY2019 · Department of Energy

A NOVEL INTEGRATED DEFLECTOR SENSOR FOR SPM SYSTEMS$1,149,988

· FY2015 · Department of Energy

THE PROGRAM GOAL IS THE DEVELOPMENT AND SUBSEQUENT DEMONSTRATION OF A MWIR HYPERSPECTRAL FRAMING CAMERA WITH A CHIP-SCALE SPECTRAL ELEMENT.$904,212

· FY2020 · National Aeronautics and Space Administration

HIGH TEMPERATURE, HIGH ENERGY DENSITY FILM CAPACITORS$849,484

· FY2008 · Department of Energy

ALL STARS EXHIBIT INTENSITY FLUCTUATIONS OVER SEVERAL TIME SCALES FROM NANOSECONDS TO DAYS; THESE INTENSITY FLUCTUATIONS ECHO OFF PLANETARY BODIES IN THE STAR SYSTEM AND PROVIDE AN OPPORTUNITY TO DETECT AND POSSIBLY IMAGE EXOPLANETS USING MODERN COMPUTATIONAL IMAGING TECHNIQUES. A MISSION UTILIZING STELLAR ECHO DETECTORS COULD PROVIDE CONTINENT-LEVEL IMAGING OF EXOPLANETS MORE READILY THAN INTERFEROMETRIC TECHNIQUES AS HIGH TEMPORAL RESOLUTION DETECTION IS LESS TECHNICALLY CHALLENGING AND MORE COST EFFECTIVE THAN MULTIKILOMETER- BASELINE FRINGE-TRACKING PARTICULARLY IN A PHOTON-STARVED REGIME. THE CONCEPT IS ALSO VIABLE FOR SURVEY MISSIONS FOR DETECTING EXOPLANETS AT MORE DIVERSE ORBITAL INCLINATIONS THAN IS POSSIBLE WITH TRANSIT OR RADIAL VELOCITY TECHNIQUES. UNDER A PHASE I NIAC PROGRAM WE EVALUATED THE FEASIBILITY OF THE STELLAR ECHO TECHNIQUE AND WHILE SEVERAL PRACTICAL CONSTRAINTS HAVE BEEN IDENTIFIED WE HAVE NOT IDENTIFIED ANY FUNDAMENTAL LIMITATIONS. WE DETERMINED THAT THE FOUNDATIONAL TECHNOLOGY ALREADY EXISTS AND HAS HIGH TRL IN SPACE MISSIONS. FURTHERMORE THE MEASUREMENTS REQUIRED TO DEMONSTRATE THE FEASIBILITY OF STELLAR ECHO DETECTION ARE COMPLEMENTARY TO ASTEROSEISMOLOGY MEASUREMENTS SO A DEMONSTRATION MISSION WOULD PROVIDE HIGH-VALUE SCIENTIFIC INFORMATION TO OTHER ACTIVE ASTROPHYSICS PROGRAMS. UNDER THE PHASE II PROGRAM WE WILL CONTINUE TO ADVANCE THE THEORETICAL UNDERSTANDING OF STELLAR ECHO IMAGING IMPROVE ON THE COMPUTATIONAL METHODS DEVELOPED IN PHASE I EVALUATE SPECIFIC HARDWARE IMPLEMENTATIONS AND ULTIMATELY PRODUCE A ROADMAP FOR THE DEMONSTRATION OF STELLAR ECHO DETECTION AND IMAGING OF EXOPLANETS.$468,163

· FY2020 · National Aeronautics and Space Administration

TITLE: VACUUM MICROELECTRONIC THERMOELECTRIC COOLER; PI: DONALD PATTERSON$199,986

· FY2009 · Department of Energy

RAPID AND LOW TEMPERATURE DENSIFICATION OF GADOLINIA DOPED CERIA BARRIER LAYERS BY PHOTONIC CURING$155,000

· FY2017 · Department of Energy

ENHANCED PROPPANT DISTRIBUTION ANALYSIS METHODS$154,999

· FY2017 · Department of Energy

INNOVATIVE NOX SENSOR FOR TAILPIPE EMISSIONS$149,994

· FY2013 · Department of Energy

LASER CLADDING APPLIED TO THE CONSTUCTION OF PFC'S WITH INTEGRAL TRITIUM DIFFUSION BARRIERS$149,965

· FY2013 · Department of Energy

ALL STARS EXHIBIT INTENSITY FLUCTUATIONS OVER SEVERAL TIME SCALES FROM NANOSECONDS TO DAYS; THESE INTENSITY FLUCTUATIONS ECHO OFF PLANETARY BODIES IN THE STAR SYSTEM AND PROVIDE AN OPPORTUNITY TO DETECT AND IMAGE EXOPLANETS USING MODERN COMPUTATIONAL IMAGING TECHNIQUES. A MISSION UTILIZING DISTRIBUTED-APERTURE STELLAR ECHO DETECTORS COULD PROVIDE CONTINENT-LEVEL IMAGING OF EXOPLANETS MORE READILY THAN INTERFEROMETRIC TECHNIQUES AS HIGH TEMPORAL RESOLUTION DETECTION IS LESS TECHNICALLY CHALLENGING AND MORE COST EFFECTIVE THAN MULTI-KILOMETER-BASELINE FRINGE-TRACKING PARTICULARLY IN A PHOTON-STARVED REGIME. THE CONCEPT IS VIABLE FOR DETECTING EXOPLANETS AT MORE DIVERSE ORBITAL INCLINATIONS THAN IS POSSIBLE WITH TRANSIT OR RADIAL VELOCITY TECHNIQUES.$99,935

· FY2016 · National Aeronautics and Space Administration

ALL STARS EXHIBIT INTENSITY FLUCTUATIONS OVER SEVERAL TIME SCALES FROM NANOSECONDS TO DAYS; THESE INTENSITY FLUCTUATIONS ECHO OFF PLANETARY BODIES IN THE STAR SYSTEM AND PROVIDE AN OPPORTUNITY TO DETECT AND POSSIBLY IMAGE EXOPLANETS USING MODERN COMPUTATIONAL IMAGING TECHNIQUES. A MISSION UTILIZING STELLAR ECHO DETECTORS COULD PROVIDE CONTINENT-LEVEL IMAGING OF EXOPLANETS MORE READILY THAN INTERFEROMETRIC TECHNIQUES AS HIGH TEMPORAL RESOLUTION DETECTION IS LESS TECHNICALLY CHALLENGING AND MORE COST EFFECTIVE THAN MULTI- KILOMETER-BASELINE FRINGE-TRACKING PARTICULARLY IN A PHOTON-STARVED REGIME. THE CONCEPT IS ALSO VIABLE FOR SURVEY MISSIONS FOR DETECTING EXOPLANETS AT MORE DIVERSE ORBITAL INCLINATIONS THAN IS POSSIBLE WITH TRANSIT OR RADIAL VELOCITY TECHNIQUES. UNDER A PHASE I NIAC PROGRAM WE EVALUATED THE FEASIBILITY OF THE STELLAR ECHO TECHNIQUE AND WHILE SEVERAL PRACTICAL CONSTRAINTS HAVE BEEN IDENTIFIED WE HAVE NOT IDENTIFIED ANY FUNDAMENTAL LIMITATIONS. WE DETERMINED THAT THE FOUNDATIONAL TECHNOLOGY ALREADY EXISTS AND HAS HIGH TRL IN SPACE MISSIONS. FURTHERMORE THE MEASUREMENTS REQUIRED TO DEMONSTRATE THE FEASIBILITY OF STELLAR ECHO DETECTION ARE COMPLEMENTARY TO ASTEROSEISMOLOGY MEASUREMENTS SO A DEMONSTRATION MISSION WOULD PROVIDE HIGH-VALUE SCIENTIFIC INFORMATION TO OTHER ACTIVE ASTROPHYSICS PROGRAMS. UNDER THE PHASE II PROGRAM WE WILL CONTINUE TO ADVANCE THE THEORETICAL UNDERSTANDING OF STELLAR ECHO IMAGING IMPROVE ON THE COMPUTATIONAL METHODS DEVELOPED IN PHASE I EVALUATE SPECIFIC HARDWARE IMPLEMENTATIONS AND ULTIMATELY PRODUCE A ROADMAP FOR THE DEMONSTRATION OF STELLAR ECHO DETECTION AND IMAGING OF EXOPLANETS.$31,837

· FY2017 · National Aeronautics and Space Administration