Bryant invented the hexabundle — a lightly-fused bundle of optical fibres that behaves as an imaging integral-field unit while retaining high throughput — and leads the Hector galaxy survey instrument built around them. Her work is squarely instrumentation: fibre bundle design and fabrication, throughput and cross-talk characterisation, and the deployment of hundreds of these units on a telescope to obtain spatially resolved spectroscopy of thousands of galaxies. Positioned against the established body of NV-ensemble quantum sensing work — DEER, nanoscale NMR and T1 relaxometry protocols operating at pT/sqrt(Hz) field sensitivity — the connection is device-level rather than conceptual, but the discipline — squeezing every photon out of a fibre-coupled optical train — is the same one that governs collection-efficiency-limited pT/sqrt(Hz) NV ensemble readout. Borderline inclusion under the astronomy criterion; kept because the sensor front end is the object of study.
NON-PREFERRED (astronomy pivot, kept for review). Burdge discovers and characterizes compact binary systems (white dwarfs, neutron stars, black holes) using time-domain, multi-messenger methods, and develops ultrafast sub-electron-noise optical camera instrumentation (Lightspeed) for ground-based telescopes; this is a good fit for the 'sufficiently complicated sensor enabling temporal resolution' astro-pivot category rather than core quantum sensing.
Buscher leads optical/infrared astronomical interferometry research at the Cavendish, co-leading COAST and serving as System Architect for the Magdalena Ridge Observatory Interferometer (MROI) in New Mexico. Current work focuses on MROI science-combiner instrumentation, fringe tracking, and light source/alignment systems for the beam train. He also holds an EPSRC grant (with Haniff and Young) on machining metre-sized gratings with nanometre precision for ELT high-resolution spectrographs. He is President of the Scientific Council of the European Interferometry Initiative.
Experimental cosmologist building and operating CMB telescopes. Directions: (1) South Pole Telescope — PI of SPT series; SPT-3G currently mapping CMB temperature and polarization at arcminute resolution; (2) thermal and kinematic Sunyaev-Zel'dovich effect mapping for galaxy cluster cosmology; (3) CMB gravitational lensing for large-scale structure; (4) CMB-S4 design and planning. Argonne joint appointment. APS and AAAS Fellow.
Carr designs, builds and calibrates fluxgate magnetometers for planetary and heliophysics space missions (including ESA's JUICE and BepiColombo), covering everything from sensor electronics to in-flight calibration of magnetic-field instrumentation.
Develops superconducting detector and readout systems for CMB observations. Directions: (1) SQUID-multiplexed readout architecture for large TES bolometer arrays (SPT-3G, CMB-S4); (2) transition-edge sensor bolometer fabrication and characterization; (3) MKID detector development; (4) CMB-S4 instrument design. Argonne joint appointment. Deep expertise in quantum-limited cryogenic detector readout.
Clements studies dusty, infrared-luminous galaxies and gravitationally lensed submillimetre sources using Herschel, ALMA and other facilities to probe galaxy formation and evolution, and works on transient/anomaly detection in large astronomical surveys.
DePoy heads the Munnerlyn Astronomical Instrumentation Lab, building high-throughput spectrographs and precision photometric-calibration systems (DECam/DECal for the Dark Energy Survey, VIRUS for HETDEX, GMACS for the Giant Magellan Telescope). A strong astronomy pivot where detector/spectrograph sensitivity is the enabling technology.
Doeleman founded and directs the Event Horizon Telescope, assembling a global mm-wavelength VLBI network to image the immediate environments of supermassive black holes at horizon-scale resolution — an astronomy pivot whose entire scientific case rests on pushing angular resolution to its fundamental (diffraction/baseline) limit via a globally distributed, highly complex sensor array.
Observational exoplanet astronomer studying planetary system architectures and demographics using transit and radial-velocity surveys.