My research lies at the intersection of astronomical instrumentation and observational astrophysics. I develop new instruments and observational techniques that enable new and/or improved measurements of astrophysical systems. These instruments are then applied to address fundamental questions in astrophysics, particularly the physics of the interstellar medium, magnetic fields, and, more recently, the direct detection and characterisation of exoplanets.

My research philosophy is broadly captured below:

Develop new techniques and instruments ↔ validate them on the sky ↔ use them to answer exciting scientific questions.

Research Themes

Astronomical Instrumentation

Modern astronomy advances because of advances in instrumentation and observational techniques. My work spans the complete life cycle of astronomical instruments—from scientific motivation and instrument design and building to commissioning and scientific exploitation.

Current projects include:


Precision Polarimetry

Polarimetry is one of the most powerful yet technically demanding techniques in observational astronomy. My research focuses on developing instruments and calibration methods that improve both the precision and accuracy of polarimetric observations.

Research areas include


Science with Polarimetry

New instruments are ultimately valuable because of the science they enable. I use optical and near-infrared polarimetry to study

These studies combine observations from facilities including SALT, IRSF, the SAAO 1.9 m Telescope, and future Extremely Large Telescope instrumentation. Recently, I have also become heavily involved with the upcoming NASA Mission to measure the polarisation of stellar sightlines in the UV.


Current Projects

ProjectDescription
WALOPFour-camera wide-field imaging polarimeter for the PASIPHAE survey
FiberPolHigh-precision fiber-fed spectropolarimeter developed at SAAO
ELT PCSInstrument concept development for the 39-m Extremely Large Telescope
PUFFINSNASA Mission for UV Spectropolarimetry of dust