Wavefront, Llc
CAGE Code: 66GV3
NCAGE Code: 66GV3
Status: Discontinued
Type: Commercial Supplier
Dun & Bradstreet (DUNS): 965404242
Summary
Wavefront, Llc is a Discontinued Commercial Supplier with the Cage Code 66GV3 and is tracked by Dun & Bradstreet under DUNS Number 965404242..
Address
7 Johnston Cir
Basking Ridge NJ 07920-3741
United States
Points of Contact
No Points of Contact...
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Frequently Asked Questions (FAQ) for CAGE 66GV3
- What is CAGE Code 66GV3?
- 66GV3 is the unique identifier used by NATO Organizations to reference the physical entity known as Wavefront, Llc located at 7 Johnston Cir, Basking Ridge NJ 07920-3741, United States.
- Who is CAGE Code 66GV3?
- 66GV3 refers to Wavefront, Llc located at 7 Johnston Cir, Basking Ridge NJ 07920-3741, United States.
- Where is CAGE Code 66GV3 Located?
- CAGE Code 66GV3 is located in Basking Ridge, NJ, USA.
Contracting History for CAGE 66GV3 Most Recent 25 Records
- NNX16CS77C
- Igf::Ot::Igf We Propose To Develop A Photon-Counting Integrated Circuit (Pcic) Detector And Focal Plane Array (Fpa) With Highest Sensitivity, Lowest Noise And Hence Highest Signal-To-Noise Ratio (S/N) Among All Fpas Covering The Shortwave Infrared Band, For Incorporation Into A Prototype Imaging Spectroscopy Camm Instrument For Real-Time Operation On A Planetary Surface To Guide Rover Targeting, Sample Selection (For Missions Involving Sample Return), And Science Optimization Of Data Returned To Earth, Thus Improving Science Return From Instruments Used To Study The Elemental, Chemical, And Mineralogical Composition Of Planetary Materials. During Phase I, We Have Successfully Proven The Concept Of A Limited-Size Array Of Pcic Detector Pixels As Well As The Imaging Spectrometer Camm Instrument. In Phase Ii, We Will Develop And Prototype A Pcic Focal Plane Array (Fpa) As Well As The Imaging Spectrometer Camm Instrument.
- 1 Jun 2018
- Igf::Ot::Igf We Propose To Develop A Photon-Counting Integrated Circuit (Pcic) Detector And Focal Plane Array (Fpa) With Highest Sensitivity, Lowest Noise And Hence Highest Signal-To-Noise Ratio (S/N) Among All Fpas Covering The Shortwave Infrared Band, For Incorporation Into A Prototype Imaging Spectroscopy Camm Instrument For Real-Time Operation On A Planetary Surface To Guide Rover Targeting, Sample Selection (For Missions Involving Sample Return), And Science Optimization Of Data Returned To Earth, Thus Improving Science Return From Instruments Used To Study The Elemental, Chemical, And Mineralogical Composition Of Planetary Materials. During Phase I, We Have Successfully Proven The Concept Of A Limited-Size Array Of Pcic Detector Pixels As Well As The Imaging Spectrometer Camm Instrument. In Phase Ii, We Will Develop And Prototype A Pcic Focal Plane Array (Fpa) As Well As The Imaging Spectrometer Camm Instrument.
- Nasa Shared Services Center
- National Aeronautics And Space Administration (Nasa)
- $749,994.00
- National Aeronautics And Space Administration (Nasa)
- NNX16CS77C
- Igf::Ot::Igf We Propose To Develop A Photon-Counting Integrated Circuit (Pcic) Detector And Focal Plane Array (Fpa) With Highest Sensitivity, Lowest Noise And Hence Highest Signal-To-Noise Ratio (S/N) Among All Fpas Covering The Shortwave Infrared Band, For Incorporation Into A Prototype Imaging Spectroscopy Camm Instrument For Real-Time Operation On A Planetary Surface To Guide Rover Targeting, Sample Selection (For Missions Involving Sample Return), And Science Optimization Of Data Returned To Earth, Thus Improving Science Return From Instruments Used To Study The Elemental, Chemical, And Mineralogical Composition Of Planetary Materials. During Phase I, We Have Successfully Proven The Concept Of A Limited-Size Array Of Pcic Detector Pixels As Well As The Imaging Spectrometer Camm Instrument. In Phase Ii, We Will Develop And Prototype A Pcic Focal Plane Array (Fpa) As Well As The Imaging Spectrometer Camm Instrument.
- 1 Jun 2018
- Igf::Ot::Igf We Propose To Develop A Photon-Counting Integrated Circuit (Pcic) Detector And Focal Plane Array (Fpa) With Highest Sensitivity, Lowest Noise And Hence Highest Signal-To-Noise Ratio (S/N) Among All Fpas Covering The Shortwave Infrared Band, For Incorporation Into A Prototype Imaging Spectroscopy Camm Instrument For Real-Time Operation On A Planetary Surface To Guide Rover Targeting, Sample Selection (For Missions Involving Sample Return), And Science Optimization Of Data Returned To Earth, Thus Improving Science Return From Instruments Used To Study The Elemental, Chemical, And Mineralogical Composition Of Planetary Materials. During Phase I, We Have Successfully Proven The Concept Of A Limited-Size Array Of Pcic Detector Pixels As Well As The Imaging Spectrometer Camm Instrument. In Phase Ii, We Will Develop And Prototype A Pcic Focal Plane Array (Fpa) As Well As The Imaging Spectrometer Camm Instrument.
- Nasa Shared Services Center
- National Aeronautics And Space Administration (Nasa)
- $749,994.00
- National Aeronautics And Space Administration (Nasa)
- NNX16CS77C
- Igf::Ot::Igf We Propose To Develop A Photon-Counting Integrated Circuit (Pcic) Detector And Focal Plane Array (Fpa) With Highest Sensitivity, Lowest Noise And Hence Highest Signal-To-Noise Ratio (S/N) Among All Fpas Covering The Shortwave Infrared Band, For Incorporation Into A Prototype Imaging Spectroscopy Camm Instrument For Real-Time Operation On A Planetary Surface To Guide Rover Targeting, Sample Selection (For Missions Involving Sample Return), And Science Optimization Of Data Returned To Earth, Thus Improving Science Return From Instruments Used To Study The Elemental, Chemical, And Mineralogical Composition Of Planetary Materials. During Phase I, We Have Successfully Proven The Concept Of A Limited-Size Array Of Pcic Detector Pixels As Well As The Imaging Spectrometer Camm Instrument. In Phase Ii, We Will Develop And Prototype A Pcic Focal Plane Array (Fpa) As Well As The Imaging Spectrometer Camm Instrument.
- 21 Sep 2018
- Igf::Ot::Igf We Propose To Develop A Photon-Counting Integrated Circuit (Pcic) Detector And Focal Plane Array (Fpa) With Highest Sensitivity, Lowest Noise And Hence Highest Signal-To-Noise Ratio (S/N) Among All Fpas Covering The Shortwave Infrared Band, For Incorporation Into A Prototype Imaging Spectroscopy Camm Instrument For Real-Time Operation On A Planetary Surface To Guide Rover Targeting, Sample Selection (For Missions Involving Sample Return), And Science Optimization Of Data Returned To Earth, Thus Improving Science Return From Instruments Used To Study The Elemental, Chemical, And Mineralogical Composition Of Planetary Materials. During Phase I, We Have Successfully Proven The Concept Of A Limited-Size Array Of Pcic Detector Pixels As Well As The Imaging Spectrometer Camm Instrument. In Phase Ii, We Will Develop And Prototype A Pcic Focal Plane Array (Fpa) As Well As The Imaging Spectrometer Camm Instrument.
- Nasa Shared Services Center
- National Aeronautics And Space Administration (Nasa)
- $749,994.00
- National Aeronautics And Space Administration (Nasa)
- NNX16CS77C
- Igf::Ot::Igf We Propose To Develop A Photon-Counting Integrated Circuit (Pcic) Detector And Focal Plane Array (Fpa) With Highest Sensitivity, Lowest Noise And Hence Highest Signal-To-Noise Ratio (S/N) Among All Fpas Covering The Shortwave Infrared Band, For Incorporation Into A Prototype Imaging Spectroscopy Camm Instrument For Real-Time Operation On A Planetary Surface To Guide Rover Targeting, Sample Selection (For Missions Involving Sample Return), And Science Optimization Of Data Returned To Earth, Thus Improving Science Return From Instruments Used To Study The Elemental, Chemical, And Mineralogical Composition Of Planetary Materials. During Phase I, We Have Successfully Proven The Concept Of A Limited-Size Array Of Pcic Detector Pixels As Well As The Imaging Spectrometer Camm Instrument. In Phase Ii, We Will Develop And Prototype A Pcic Focal Plane Array (Fpa) As Well As The Imaging Spectrometer Camm Instrument.
- 21 Sep 2018
- Igf::Ot::Igf We Propose To Develop A Photon-Counting Integrated Circuit (Pcic) Detector And Focal Plane Array (Fpa) With Highest Sensitivity, Lowest Noise And Hence Highest Signal-To-Noise Ratio (S/N) Among All Fpas Covering The Shortwave Infrared Band, For Incorporation Into A Prototype Imaging Spectroscopy Camm Instrument For Real-Time Operation On A Planetary Surface To Guide Rover Targeting, Sample Selection (For Missions Involving Sample Return), And Science Optimization Of Data Returned To Earth, Thus Improving Science Return From Instruments Used To Study The Elemental, Chemical, And Mineralogical Composition Of Planetary Materials. During Phase I, We Have Successfully Proven The Concept Of A Limited-Size Array Of Pcic Detector Pixels As Well As The Imaging Spectrometer Camm Instrument. In Phase Ii, We Will Develop And Prototype A Pcic Focal Plane Array (Fpa) As Well As The Imaging Spectrometer Camm Instrument.
- Nasa Shared Services Center
- National Aeronautics And Space Administration (Nasa)
- $749,994.00
- National Aeronautics And Space Administration (Nasa)