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APD’s technology development investments have advanced TRLs of dozens of technologies and led to 170 infusions and 66 potential infusions into space, suborbital, and ground-based missions and projects. Infusion here means that a technology was implemented in a mission/project (Implemented), baselined by a mission (Planned), or incorporated into a strategic mission concept’s reference design (Concepts/Studies). Technologies developed for strategic astrophysics missions often find applications beyond strategic missions, including Probes, Explorers, sub-orbital rockets, balloon missions, and ground-based projects. Further, applications aren’t limited to astrophysics, with technologies being infused into cross-cutting applications in Earth Science, Planetary Science, and Heliophysics.

Infusions resulting from APD funding to technology-maturation PIs (from Jan 2009 to Jul 2025; includes SAT/ISFM funding and APRA funding of SAT/ISFM PIs)

Technology Infusions Summary 9-11-2025
1. Implemented in a past or current flight mission or ground-based project (e.g., Hitomi, XRISM, ICON, Solar Orbiter).
2. Upcoming flight mission or ground project (e.g., RST, LISA, ATHENA, Sprite CubeSat) baselined the tech.
3. Concept or reference design of APD-funded large-mission study (LUVOIR, HabEx, Lynx, Origins); Probe (e.g., PICO, AXIS, GEP, CETUS, AXIS, PRIMA); or Phase-1 Explorer or Mission of Opportunity study/proposal (e.g., STAR-X) baselined the tech.
4. Infusion-ready at TRL 5 but not yet included in any of the above categories, likely due to lack of opportunity.

Infusions Breadth

236 infusions (implemented, upcoming, and potential):

Of 100 technologies

Into 117 mission/projects/funded studies

Across all four SMD Division disciplines and beyond

  • Astrophysics (200)
  • Earth Science (7)
  • Planetary (9)
  • Heliophysics (15)
  • Other (5) (IF board for ONI, APS sensors for ePIC, mandrel for NIF, neutron microscope optics for NIST, and lab X-ray diagnostics of high-resolution inner-shell transition measurements)

69 infusions supporting 41 missions/projects/funded studies involving other

US/international agencies and bodies (with or without NASA involvement)

Infusions – Implemented (a)

Space Missions

Bautz: Directly deposited optical blocking filters flying on OSIRIS-REx/OSIRIS-APEX

Bongiorno: High-precision mirror shell alignment and mounting used for IXPE

Gaskin/Ramsey/Thomas/Bongiorno/Baumgartner/Champey: High-Energy Replicated Optics contributed to IXPE and SRG (ART-XC) optics

Kilbourne: Si-thermistor/HgTe microcalorimeter array flew on Hitomi and flying on XRISM

Klipstein: Phasemeter flying on GRACE Follow-On

Quijada: UV coatings flying on GOLD and ICON

Shirron: Adiabatic Demagnetization Refrigerator (ADR) flew on Hitomi and flying on XRISM

Siegmund/Vallerga: APD-funded MCPs flying on ICON, GOLD, JUNO, JUICE, Solar Orbiter, and Europa Clipper

Thomas/Baumgartner: X-Ray test processes and techniques (off-loader, mounting, analysis, etc.) used for IXPE and SRG (ART-XC)

Zhang: Slumped-glass X-ray mirrors flying on NuStar

Sounding Rocket Missions

Bongiorno: High-precision mirror shell alignment and mounting used by FOXSI-4

Fleming: Electron-beam-lithography-ruled gratings flew on OAxFORTIS

Fleming: Image Slicer flew on INFUSE

Gaskin/Ramsey/Thomas/Bongiorno/Baumgartner/Champey: Electroformed X-ray mirror shells flew on FOXSI-4 and MaGIXS-2

Greenhouse: Next-gen microshutter arrays flew on OAxFORTIS

Gurgew: Single and multilayer coating techniques used by FOXSI-4

Hoenk: delta-doped SRI 2kx4k CMOS image sensors flew on SSAXI-Rocket and Hi-C Flare rocket

Kilbourne: Si-thermistor/HgTe microcalorimeter array flew on XQC

McEntaffer: X-ray reflection grating flew on WRXR and tREXS

Nikzad: ALD mirror coating flew on SISTINE

Nikzad: Superlattice-doped detector flew on SHIELDS

Quijada: Far-UV coatings flew on OAxFORTIS

Schattenburg/Heilmann: Blazed soft X-ray reflection grating flew on MaGIXS

Scowen: Next-gen microshutter arrays flew on OAxFORTIS

Siegmund/Vallerga: MCPs flew on FIRE, SLICE, EUNIS, FORTIS, VeSpR, CHESS, SISTINE, INFUSE, OAxFORTIS and DEUCE

Singam: Electroforming Process Modeling used by FOXSI-4

Thomas/Baumgartner: X-Ray test processes and techniques (off-loader, mounting, analysis, etc.) used by FOXSI-4

Ullom: TES microcalorimeters and Time-division SQUID multiplexers flew on Micro-X

Vallerga: Tpx3 CdTe detector flew on FOXSI-4

Vorobiev: DMDs flew on INFUSE

Infusions – Implemented (b)

Balloon Missions

Bennett: microwave SQUID multiplexer firmware and parameters flew on DR. TES

Bock: Antenna-coupled detectors flew on Spider

Gaskin/Ramsey/Thomas/Bongiorno/Baumgartner/Champey: Electroformed X-ray mirror shells flew on HEROES

Hu: 4.7 THz local oscillator flew on STO-2 and GUSTO

Mehdi: Heterodyne detectors flew on STO-2

Mehdi: Heterodyne-detector-related C&DH and ASIC flew on HASP

Nikzad: Advanced CCD detectors flew on FIREBall 2

Serabyn: Broadband Light Rejection with Optical Vortex Coronagraph flew on PICTURE-C

Staguhn: Far-IR large-format detectors flew on PIPER

Ullom: Time-division SQUID multiplexers flew on Spider and PIPER

Zmuidzinas: TiN KIDs were integrated into BLAST-TNG balloon mission

Airborne Experiments

Mosely: TES Bolometers for the HAWC+ flew on SOFIA

Ullom: Time-division SQUID multiplexers for the HAWC+ flew on SOFIA

Wollack: Absorptive mixtures and glint reduction coatings for HAWC+ flew on SOFIA

Balloon Missions

Bennett: microwave SQUID multiplexer firmware and parameters flew on DR. TES

Bock: Antenna-coupled detectors flew on Spider

Gaskin/Ramsey/Thomas/Bongiorno/Baumgartner/Champey: Electroformed X-ray mirror shells flew on HEROES

Hu: 4.7 THz local oscillator flew on STO-2 and GUSTO

Mehdi: Heterodyne detectors flew on STO-2

Mehdi: Heterodyne-detector-related C&DH and ASIC flew on HASP

Nikzad: Advanced CCD detectors flew on FIREBall 2

Serabyn: Broadband Light Rejection with Optical Vortex Coronagraph flew on PICTURE-C

Staguhn: Far-IR large-format detectors flew on PIPER

Ullom: Time-division SQUID multiplexers flew on Spider and PIPER

Zmuidzinas: TiN KIDs were integrated into BLAST-TNG balloon mission

Airborne Experiments

Mosely: TES Bolometers for the HAWC+ flew on SOFIA

Ullom: Time-division SQUID multiplexers for the HAWC+ flew on SOFIA

Wollack: Absorptive mixtures and glint reduction coatings for HAWC+ flew on SOFIA

Infusions – Implemented (c)

Ground-Based Projects

Bennett: microwave SQUID multiplexer crosstalk avoidance implemented at Simons Observatory

Bock: Antenna-coupled detectors were deployed on BICEP2, BICEP3/Keck, and BICEP Array

Bottom: Near-IR LmAPD implemented in UH 2.2m telescope ULBCam and Subaru

Bradford: Ultra-Sensitive Bolometers were deployed at Kitt’s Peak (TIME)

Guyon: Linear Wavefront Control deployed to Subaru observatory

Hoenk: delta-doped SRI 4kx4k CMOS image sensors implemented in CHaS on the MDM Observatory

Kolodziejczak: Mandrel used to form NIF X-ray microscope optic

Mauskopf: IF Board used in Toltec camera at LMT

Mawet: Spectrograph and Wavefront Control Architectures were deployed on Keck Planet Imager and Characterizer

Nikzad: Delta-doped CCDs at Palomar-WaSP and ZTF as permanent facilities

Ninkov: DMDs were deployed on the 4.1-m SOAR telescope

Ramsey/Thomas: Electroformed X-ray mirror shell techniques used for NIST Neutron Microscope optics

Schattenburg/Heilmann: X-ray CAT grating used at SAO lab for diagnostics of X-ray inner-shell transition measurements

Serabyn: Vortex coronagraph deployed to Palomar, Keck, and Subaru observatories

Staguhn: TES bolometers used in the IRAM bolometer camera at the IRAM 30m telescope

Ullom: Microwave SQUID multiplexers deployed on GBT MUSTANG2 and Simons Observatory

Ullom: OMT-coupled TES bolometers deployed on ABS, ACTPol, AdvancedACT, ALI-CPT, GBT MUSTANG2, SPTPol, and Simons Observatory

Ullom: TES bolometers deployed on JCMT SCUBA2

Ullom: Time-division SQUID multiplexers were deployed on ABS, ACT, ACTPol, AdvancedACT, BICEP2, BICEP3/Keck, and JCMT SCUBA2

Ullom: TiN KIDs were deployed on Toltec Camera at LMT

Wollack: Feedhorn-coupled symmetric-OMT architectures implemented on ABS, ACTpol, Advanced ACTpol, CLASS, and Simons Observatory

Wollack: Feedhorn-coupled symmetric-OMT focal planes and Absorptive mixtures and glint reduction coatings deployed on CLASS

Infusions – Upcoming (a)

Space Missions

Belikov: Multi-star Wavefront Sensing and Control to fly on RST (2027)

Conklin: Charge Management System (CMS) being developed as NASA contribution for LISA (2035)

Fleming: Protected eLiF mirror coatings and MCP anti-coincidence shielding to fly on SPRITE CubeSat (2025)

Fleming: Electron-beam-lithography-ruled gratings to be flown on MANTIS CubeSat (2028)

Hennessy: ALD UV coatings to fly on SPARCS (2025), SPRITE (2026), and Aspera (2026) CubeSats, and on UVEX (2030)

Hennessy: Multilayer aluminum dielectric filters for UV detectors to fly on SPARCS CubeSat (2025)

Hoenk: delta-doped SRI 4kx4k CMOS image sensors to fly on UVEX

Kasdin: Wavefront Control with two deformable mirrors baselined for RST

Kilbourne: TES Microcalorimeter arrays and Time-Domain Multiplexing (TDM) baselined for ATHENA (2037) X-IFU

Krist, Shaklan: End-to-end Coronagraph models baselined for RST

Lee: CMB detectors baselined for LiteBIRD (2032)

Livas: Telescope being developed as NASA contribution for LISA

Nikzad: Advanced CCD detectors baselined by SPARCS CubeSat

Quijada: Physical Vapor Deposition in support of Hennessy’s ALD UV Coatings to fly on SPRITE and Aspera CubeSats

Rauscher: H4RG IR detectors baselined for RST

Rauscher: Radiation-Tolerant, Photon-Counting, Visible and Near-IR Detectors to fly on DarkNESS CubeSat (2026) and DAVINCI (2029)

Siegmund/Vallerga: MCPs planned to fly on SPRITE, Aspera, GLIDE (2025), EUVST (2026), and MANTIS

Trauger: Hybrid Lyot Coronagraph baselined for RST

Vallerga: Timepix2 ASICs to fly on PADRE CubeSat (2025)

Wollack: Feedhorn-coupled symmetric-OMT architectures adopted by LiteBIRD

Yu: Laser technology being developed as NASA contribution for LISA

Infusions – Upcoming (b)

Sounding Rocket Missions

Fleming: Electron-beam-lithography-ruled gratings to be flown on MOBIUS (2027)

Gaskin/Ramsey/Thomas/Bongiorno/Baumgartner/Champey: Electroformed X-ray mirror shells to fly on REDSoX (2027)

Hennessy: Multilayer aluminum dielectric filters for UV detectors and ALD UV coatings to fly on FLUID (2026)

McEntaffer: X-ray reflection gratings to be flown on OGRE (2025)

Nikzad: EMCCDs to fly on SHIMCO sounding rocket (2027)

Schattenburg/Heilmann: X-ray CAT grating baselined for REDSoX

Siegmund/Vallerga: MCP detectors to fly on MOBIUS, and FLUID

Zhang: Single-crystal silicon X-ray mirrors to be flown on OGRE

Balloon Missions

Bradford: setup developed for Ultra-Sensitive Bolometers to fly on TIM (2026)

Gaskin/Ramsey/Thomas/Bongiorno/Baumgartner/Champey: Electroformed X-ray mirror shells to fly on SuperHERO (2028)

Goldsmith: Far-IR heterodyne technology to fly on ASTHROS (2025)

Mauskopf: RFSoC readout baselined for PUEO (2025), and TIM

Stahl: Arnold Mirror Modeler Tool and Structure Optimization Tool used for POEMM primary mirror

Airborne Experiments

Mauskopf: IF Board to be flown in ONR airborne KID instrument (~2026)

Ground-Based Projects

Caputo: AstroPix CMOS Monolithic Active Pixel Sensors (APSs) to be implemented at the Electron-Proton/Ion Collider (ePIC) at BNL (2030s)

Mauskopf: RFSoC-based readout firmware to be used in Prime Cam camera at CCAT receivers (2025)

Staguhn: GISMO to be deployed to GLT (2025)

Ullom: OMT-coupled TES bolometers are the baseline technology for CMB-S4 (2030)

Vasisht: EPRV etalon will be deployed on Keck Planet Finder (2025)

Wollack: Feedhorn-coupled symmetric-OMT architectures adopted by CMB-S4

Infusions – Concept/Study DRMs

Space Missions

Bautz: Directly deposited optical blocking filters baselined for Lynx

Bautz: Advanced CCD detector baselined by AXIS Probe and Star-X Explorer (Phase 1 Study)

Belikov: Multi-star Wavefront Sensing and Control for HabEx and LUVOIR

Belikov: PIAACMC Coronagraph for HabEx and LUVOIR

Bierden: MEMS deformable mirrors are baselined for HabEx and LUVOIR

Bock/O’Brient: CMB detectors and antenna-coupled detectors baselined for PICO

Bradford: Ultrasensitive Far-IR Kinetic Inductance Detector Arrays baselined for the PRIMA IR Probe concept

Fleming: MCP Anti-coincidence shielding baselined for LUVOIR

Gaskin/Ramsey/Thomas/Bongiorno/Baumgartner/Champey: Electroformed X-ray mirror shells baselined by ESCAPE

Greenhouse: Next-gen microshutter arrays baselined for HabEx, LUVOIR, and CETUS Probe

Guyon: Linear wavefront control for HabEx and LUVOIR

Guyon: Predictive wavefront control and sensor fusion for HabEx and LUVOIR

Hall (Bottom): Avalanche Photodiode HgCdTe NIR detectors baselined for HabEx and LUVOIR

Hoenk: delta-doped SRI 4kx4k CMOS image sensors baselined by CASTOR (CSA funded study for 2030 launch)

Kaaret: High-precision mirror shell alignment and mounting baselined by APRA-funded Lobster-Eye Telescope Development Study

Kasdin, Casement, Glassman, Cash: Starshade technologies baselined for Starshade-RST Rendezvous Probe

Lee: CMB detectors baselined for PICO

Mauskopf: Low-power FPGA-based readout electronics for superconducting arrays baselined for PICO, Origins, GEP, and Cosmic Dawn

McEntaffer: Low-blaze-angle grating baselined by ESCAPE (funded Phase A study)

Nikzad: Delta-doped EMCCDs baselined for HabEx

Nikzad: Delta-doped CMOS detector arrays baselined for LUVOIR

Schattenburg: CAT X-ray gratings baselined for Lynx

Schattenburg: Thermal oxide coating-stress compensation for Lynx, AXIS Probe, and TAP Probe mirrors

Serabyn: Vortex Coronagraph baselined for HabEx and LUVOIR

Siegmund/Vallerga: Cross-strip MCP detector systems baselined for HabEx, LUVOIR, and CETUS

Siegmund/Vallerga: MCP detectors are baselined for HabEx, LUVOIR, CETUS, ESCAPE and MAGIC (funded studies)

Singam: Electroforming Process Modeling used for MiXO for CubeX

Soummer: Apodized Pupil Lyot Coronagraph baselined for LUVOIR

Staguhn: Superconducting kilo-pixel far-IR detector architecture baselined for Origins

Stahl: PTC is expected to serve as a pathfinder for zonal thermal control in HabEx

Thomas/Baumgartner: X-Ray test processes and techniques (off-loader, mounting, analysis, etc.) used for MiXO for CubeX

Tuttle/Jahromi/Kimball: Continuous ADR is baselined for Lynx, Origins, PICO, GEP, and PRIMA

Ullom: Microwave SQUID multiplexers baselined for Lynx and Origins

Ullom: Time-division SQUID multiplexers baselined for PICO

Zhang: Single-crystal-silicon X-ray mirrors baselined for Lynx, AXIS, TAP Probe, and STAR-X (funded MidEx study)

Ziemer: Micro-Newton thrusters are baselined for HabEx fine pointing and jitter suppression

Infusion-Ready (TRL 5)

Space Missions

Burrows: Fast X-ray Event Recognition

Figer: A Single-Photon-Sensing and Photon-Number-Resolving Detector for NASA Missions (Quanta Image Sensor)