Select Gallery View : Slideshow | Thumbnails | PDF
For more information about these technologies visit our Technology Database.
Significance: World-class thin grazing-angle
Project Title: Next Generation
PI: Zhang, William (GSFC)
Significance: Highest-resolution
Project Title: High Resolution and High Efficiency
PI: Mark Schattenburg (MIT Kavli Institute for Astrophysics and Space Research)
Significance: Enhances manufacturability of highest-resolution
Project Title: Readying
PI: Randall Smith (SAO)
Significance: Fast readouts are crucial for large focal plane arrays in future missions
Project Title: Development of Low-Power FPGA-based Readout Electronics for Superconducting Detector Arrays
PI: Philip Mauskopf (ASU)
Significance: Low-noise detectors are crucial for future missions
Project Title: A Single-Photon-Sensing and Photon-Number-Resolving Detector for NASA Missions
PI: Don Figer (RIT)
Significance: CMB polarimetry is crucial for identifying echoes of the Big Bang
Project Title: Superconducting Detectors for Cosmic Microwave Background (CMB) Polarimetry in PICO
PI: Roger O’Brient (JPL/Caltech)
Significance: High-resolution TES microcalorimeters may enable the next
Project Title: Advanced
PI: Caroline Kilbourne (GSFC)
Significance: MMCs offer energy resolution that may enable the next
Project Title: MMC Arrays for
PI: Simon Bandler (GSFC)
Significance: High-quality
Project Title: Advanced
PI: Jacqueline Davis (MSFC)
Significance: High-quality
Project Title: Advanced
PI: Stephen Bongiorno (MSFC)
Significance: High-quality EUV and
Project Title: Advanced
PI: David Broadway (MSFC)
Significance: Adjustable
Project Title: Adjustable
PI: Paul Reid (SAO)
Significance: Advanced
Project Title: Toward Fast, Low-Noise, Radiation Tolerant
PI: Mark Bautz (MIT Kavli Institute for Astrophysics and Space Research)
Significance: Replacing windows of commercial DMD may enable far-UV multi-object spectrometry in future missions
Project Title: Development of DMD for Far-UV Applications
PI: Zoran Ninkov (RIT)
Significance: High-density readout may enable large focal planes needed for future missions
Project Title: Advancing High-Density Readout Technology for Superconducting Sensor Arrays for Spaceflight
PI: Josef Frisch (SLAC)
Significance: High-multiplexing-factor readouts may enable missions such as the next
Project Title: Technology Development for Microwave Superconducting QUantum Interference Device (SQUID) Multiplexing for the Lynx
PI: Douglas Bennett (NIST)
Significance: This advanced sub-Kelvin cooling technology may enable multiple future strategic missions
Project Title: High-Efficiency Continuous Cooling for Cryogenic Instruments and sub-Kelvin Detectors
PI: James Tuttle (GSFC)
Significance: Ultra-stability and -precision (~10 pm) may enable the next IR/optical/UV Great Observatory
Project Title: Ultra-Stable Structures
PI: Babak Saif (GSFC)
Significance: Advanced
Project Title: Development of a Robust, Efficient Process to Produce Scalable, Superconducting Kilopixel
PI: Johannes Staguhn (JHU & GSFC)
Significance: Advanced coatings may enable future far-UV missions
Project Title: High-Performance, Stable, and Scalable UV Aluminum Mirror Coatings Using ALD
PI: John Hennessy (JPL)
Significance: High far-UV reflectance is prevented by oxidation of aluminum mirrors; removing it may enable future far-UV missions
Project Title: E-Beam-Generated Plasma Etching for Developing High-Reflectance Mirrors for Far-Ultraviolet Astronomical Instrument Applications
PI: Manuel Quijada (GSFC)
Significance: Extremely sensitive
Project Title: Ultra-Sensitive Bolometers for
PI: C. Matt Bradford (JPL)
Significance: Further development of this high-resolution
Project Title: Development of High-Resolution
PI: Imran Mehdi (JPL)
Significance: Ultra-low-noise detectors may enable spectroscopy of extrasolar planets
Project Title: Photon-Counting NIR LmAPD Arrays for Ultra-Low Background Space Observations
PI: Michael Bottom (U. of Hawaii)
Significance: This technology may enable required ultra-stability (~10 pm) for the next IR/Optical/UV Great Observatory
Project Title: Predictive Thermal Control (PTC) Technology to Enable Thermally Stable Telescopes
PI: H. Philip Stahl (MSFC)
Significance: May enable future UV/optical spectroscopic missions; enables current UV suborbital missions
Project Title: Electron-Beam-Lithography Ruled Gratings for Future UV/Optical Missions: High Efficiency and Low Scatter in the Vacuum UV
PI: Brian Fleming (U. of Colorado)
Significance: May enable future Cosmic Microwave Background (CMB) missions, e.g. LiteBIRD
Project Title: Technology Development for LiteBIRD and Other CMB Missions
PI: Adrian T. Lee (UC Berkeley)
Significance: May enable sparse-field multi-object spectroscopy for future strategic and other missions
Project Title: Scalable Microshutter Systems for UV, Visible, and IR Spectroscopy
PI: Matt Greenhouse (GSFC)
Significance: Baselined by HabEx, LUVOIR, and CETUS for UV/Visible light detection
Project Title: High-Performance Sealed-Tube Cross-Strip (XS) Photon-Counting Sensors for UV-Vis Astrophysics Instruments
PI: Oswald Siegmund (UC Berkeley)
Significance: Four-side-buttable low-power readout chips may enable future far-UV missions with large focal planes
Project Title: Large-Format, High-Dynamic-Range UV Detector Using MCPs and Timepix4 Readouts
PI: John Vallerga (UC Berkeley)
Significance: Supports NASA
Project Title: Advanced
PI: F. Scott Porter (GSFC)
For more information about these technologies visit our Technology Database.
Significance: World-class thin grazing-angle
Project Title:
Next GenerationProject Title:
PI: Zhang, William (GSFC)
Significance: Highest-resolution
Project Title: High Resolution and High Efficiency
PI: Mark Schattenburg (MIT Kavli Institute for Astrophysics and Space Research)
Significance: Enhances manufacturability of highest-resolution
Project Title: Readying
PI: Randall Smith (SAO)
Significance: Fast readouts are crucial for large focal plane arrays in future missions
Project Title: Development of Low-Power FPGA-based Readout Electronics for Superconducting Detector Arrays
PI: Philip Mauskopf (ASU)
Significance: Low-noise detectors are crucial for future missions
Project Title: A Single-Photon-Sensing and Photon-Number-Resolving Detector for NASA Missions
PI: Don Figer (RIT)
Significance: CMB polarimetry is crucial for identifying echoes of the Big Bang
Project Title: Superconducting Detectors for Cosmic Microwave Background (CMB) Polarimetry in PICO
PI: Roger O’Brient (JPL/Caltech)
Significance: High-resolution TES microcalorimeters may enable the next
Project Title: Advanced
PI: Caroline Kilbourne (GSFC)
Significance: MMCs offer energy resolution that may enable the next
Project Title: MMC Arrays for
PI: Simon Bandler (GSFC)
Significance: High-quality
Project Title: Advanced
PI: Jacqueline Davis (MSFC)
Significance: High-quality
Project Title: Advanced
PI: Stephen Bongiorno (MSFC)
Significance: High-quality EUV and
Project Title: Advanced
PI: David Broadway (MSFC)
Significance: Adjustable
Project Title: Adjustable
PI: Paul Reid (SAO)
Significance: Advanced
Project Title: Toward Fast, Low-Noise, Radiation Tolerant
PI: Mark Bautz (MIT Kavli Institute for Astrophysics and Space Research)
Significance: Replacing windows of commercial DMD may enable far-UV multi-object spectrometry in future missions
Project Title: Development of DMD for Far-UV Applications
PI: Zoran Ninkov (RIT)
Significance: High-density readout may enable large focal planes needed for future missions
Project Title: Advancing High-Density Readout Technology for Superconducting Sensor Arrays for Spaceflight
PI: Josef Frisch (SLAC)
Significance: High-multiplexing-factor readouts may enable missions such as the next
Project Title: Technology Development for Microwave Superconducting QUantum Interference Device (SQUID) Multiplexing for the Lynx
PI: Douglas Bennett (NIST)
Significance: This advanced sub-Kelvin cooling technology may enable multiple future strategic missions
Project Title: High-Efficiency Continuous Cooling for Cryogenic Instruments and sub-Kelvin Detectors
PI: James Tuttle (GSFC)
Significance: Ultra-stability and -precision (~10 pm) may enable the next IR/optical/UV Great Observatory
Project Title: Ultra-Stable Structures
PI: Babak Saif (GSFC)
Significance: Advanced
Project Title: Development of a Robust, Efficient Process to Produce Scalable, Superconducting Kilopixel
PI: Johannes Staguhn (JHU & GSFC)
Significance: Advanced coatings may enable future far-UV missions
Project Title: High-Performance, Stable, and Scalable UV Aluminum Mirror Coatings Using ALD
PI: John Hennessy (JPL)
Significance: High far-UV reflectance is prevented by oxidation of aluminum mirrors; removing it may enable future far-UV missions
Project Title: E-Beam-Generated Plasma Etching for Developing High-Reflectance Mirrors for Far-Ultraviolet Astronomical Instrument Applications
PI: Manuel Quijada (GSFC)
Significance: Extremely sensitive
Project Title: Ultra-Sensitive Bolometers for
PI: C. Matt Bradford (JPL)
Significance: Further development of this high-resolution
Project Title: Development of High-Resolution
PI: Imran Mehdi (JPL)
Significance: Ultra-low-noise detectors may enable spectroscopy of extrasolar planets
Project Title: Photon-Counting NIR LmAPD Arrays for Ultra-Low Background Space Observations
PI: Michael Bottom (U. of Hawaii)
Significance: This technology may enable required ultra-stability (~10 pm) for the next IR/Optical/UV Great Observatory
Project Title: Predictive Thermal Control (PTC) Technology to Enable Thermally Stable Telescopes
PI: H. Philip Stahl (MSFC)
Significance: May enable future UV/optical spectroscopic missions; enables current UV suborbital missions
Project Title: Electron-Beam-Lithography Ruled Gratings for Future UV/Optical Missions: High Efficiency and Low Scatter in the Vacuum UV
PI: Brian Fleming (U. of Colorado)
Significance: May enable future Cosmic Microwave Background (CMB) missions, e.g. LiteBIRD
Project Title: Technology Development for LiteBIRD and Other CMB Missions
PI: Adrian T. Lee (UC Berkeley)
Significance: May enable sparse-field multi-object spectroscopy for future strategic and other missions
Project Title: Scalable Microshutter Systems for UV, Visible, and IR Spectroscopy
PI: Matt Greenhouse (GSFC)
Significance: Baselined by HabEx, LUVOIR, and CETUS for UV/Visible light detection
Project Title: High-Performance Sealed-Tube Cross-Strip (XS) Photon-Counting Sensors for UV-Vis Astrophysics Instruments
PI: Oswald Siegmund (UC Berkeley)
Significance: Four-side-buttable low-power readout chips may enable future far-UV missions with large focal planes
Project Title: Large-Format, High-Dynamic-Range UV Detector Using MCPs and Timepix4 Readouts
PI: John Vallerga (UC Berkeley)
Significance: Supports NASA
Project Title: Advanced
PI: F. Scott Porter (GSFC)