Ashley builds instruments that must work unattended in the worst environment on Earth: the PLATO and related autonomous observatories on the Antarctic plateau (Dome A/C), where he characterised the site's exceptional infrared background, seeing and atmospheric stability, and built the power, thermal and control systems needed for a telescope to survive a polar winter with no human present. He also works on low-noise infrared detectors and on CubeSat instrumentation. 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 discipline here — making a low-noise detector work reliably outside a controlled laboratory, with a hard power and thermal budget — is the same one that separates a benchtop pT/sqrt(Hz) magnetometer from a deployable one, and it is a skill set the quantum sensing field is short of. Borderline inclusion under the astronomy criterion; kept because the sensor and its environment are the entire object of study.
Crozier holds a joint Physics/Electrical Engineering chair and runs a nanophotonics laboratory spanning plasmonic and dielectric metasurfaces, on-chip optical trapping and manipulation of nanoparticles and cells, mid-infrared spectroscopy and detection with metasurface-enhanced and colloidal-nanocrystal devices, and light emission from 2D semiconductors. The unifying theme is engineering the local optical density of states to increase the signal available from a very small number of emitters or molecules. 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 plasmonic and dielectric antenna work is the same physics used to raise photon collection efficiency and hence the shot-noise floor of NV-ensemble magnetometers operating at pT/sqrt(Hz). Note: a substantial fraction of the group's output is device fabrication rather than sensitivity-limited measurement, which is a caveat against the stated preference.
Prof. Mohseni's group (Bio-inspired Sensors and Optoelectronics) pushes III-V semiconductor photodetector technology toward thermodynamic and quantum limits of photon sensitivity. Key directions: (1) Nanoscale IR photodetectors: shrinking pixel dimensions below the diffraction limit using quantum confinement effects (InGaAs/InAlAs quantum well and dot structures) to improve sensitivity, bandwidth, and resolution simultaneously; (2) Superlattice photomultipliers — high-gain, low-noise avalanche photodetectors at room temperature approaching quantum-limited sensitivity for mid-wave and long-wave infrared detection; (3) Quantum sensing applications including squeezed-light-enhanced thermoreflectance imaging of electronic hotspots, and photon-counting receivers for quantum communications. Co-author on 275+ papers, 33+ US patents; NAI Fellow 2023; W.M. Keck Foundation Award, DARPA YFA, NSF CAREER. Fellow of SPIE and Optica. Also Professor of Physics and Astronomy.
Unnithan runs a sensor-engineering group spanning plasmonic colour filters and metasurface-based CMOS image and spectral sensors, thermal/hyperspectral cameras, machine learning on sensor data, and — the relevant thread here — the engineering and packaging of quantum diamond magnetometers, in a joint programme with the Melbourne physics groups and Phasor Innovation aimed at navigation, subsurface sensing and eventual healthcare use. He has extensive industry links (Hort-Eye, KDH) and an entrepreneurial orientation. 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 — his role in that collaboration is on the readout, optics and integration side rather than the spin physics, i.e. turning a laboratory pT/sqrt(Hz) NV ensemble into a fielded instrument. Caveat against the stated preference: this group is substantially device-fabrication and product-oriented rather than sensitivity-limited fundamental measurement.
Trenti combines high-redshift galaxy and gamma-ray-burst science with hands-on space instrumentation: he leads SkyHopper, a 6U CubeSat carrying a cooled near-infrared telescope intended for rapid follow-up of transients and exoplanet transits, which is an unusually complete exercise in building a photon-starved instrument under severe SWaP constraints. The group also works on infrared detector characterisation and on-board autonomy. 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 relevance to a quantum-sensing candidate is the engineering discipline of getting a low-noise detector to work in a hostile, uncontrolled environment — the same problem that separates a laboratory pT/sqrt(Hz) NV magnetometer from a fieldable one. Borderline inclusion on the astronomy criterion; kept because instrumentation is a genuine focus rather than a by-product.