| Evidence in favour of density wave theory through age gradients observed in star formation history maps and spatially resolved stellar clusters | Monthly Notices of the Royal Astronomical Society | 2022 |
| Probing the Low-Mass End of the Black Hole Mass Function via a Study of Faint Local Spiral Galaxies | | 2022 |
| Spirality: A Novel Way to Measure Spiral Arm Pitch Angle | GALAXIES | 2022 |
| Early solar eclipse images and tests of relativity | PHYSICS TODAY | 2020 |
| Determining the co-rotation radii of spiral galaxies using spiral arm pitch angle measurements at multiple wavelengths | MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | 2020 |
| Investigating the Origins of Spiral Structure in Disk Galaxies through a Multiwavelength Study | ASTROPHYISCAL JOURNAL | 2019 |
| Prospects of detecting the nonlinear gravitational wave memory | Physical Review D | 2019 |
| A hundred years of the first experimental test of general relativity | Nature Physics | 2019 |
| Darboux transformation in black hole perturbation theory | Physical Review D | 2017 |
| The binary pulsar and the quadrupole formula controversy | European Physical Journal H | 2017 |
| 2DFFT: Measuring Galactic Spiral Arm Pitch Angle | Astrophysics Source Code Library | 2016 |
| Strong Evidence for the Density-wave Theory of Spiral Structure in Disk Galaxies | The Astrophysical Journal Letters | 2016 |
| STRONG EVIDENCE FOR THE DENSITY-WAVE THEORY OF SPIRAL STRUCTURE IN DISK GALAXIES | ASTROPHYISCAL JOURNAL LETTERS | 2016 |
| A Fundamental Plane of Spiral Structure in Disk Galaxies | Astrophysical Journal Letters | 2015 |
| Reviewing Einstein | Science | 2015 |
| The Black Hole Mass Function Derived from Local Spiral Galaxies | Astrophysical Journal | 2014 |
| Constraining Dark Matter Halo Profiles and Galaxy Formation Models using Spiral Arm Morphology. II. Dark and Stellar Mass Concentrations for 13 Nearby Face-On Galaxies | Astrophysical Journal | 2014 |
| Superradiance-tidal friction correspondence | Physical Review D | 2014 |
| Further Evidence for a Supermassive Black Hole Mass - Pitch Angle Relation | Astrophysical Journal | 2013 |
| Do floating orbits in extreme mass ratio binary black holes exist? | Physical Review D | 2013 |
| Identification of Outflows and Candidate Dual Active Galactic Nuclei in SDSS Quasars at z=0.8-1.6 | Astrophysical Journal | 2013 |
| On the link between central black holes, bar dynamics and dark matter haloes in spiral galaxies | Monthly Notices of the Royal Astronomical Society | 2012 |
| Measurement of Galactic Logarithmic Spiral Arm Pitch Angle using Two-Dimensional Fast Fourier Transform Decomposition | Astrophysical Journal Supplement Series | 2012 |
| Testing relativity from the 1919 eclipse-a question of bias | Physics Today | 2009 |
| Computational efficiency of frequency- and time-domain calculations of extreme mass-ratio binaries: Equatorial orbits | Physical Review D | 2008 |
| Discovery of a relationship between spiral arm morphology and supermassive black hole mass in disk galaxies (vol 678, pg L93, 2008) | Astrophysical Journal Letters | 2008 |
| Discovery of a relationship between spiral arm morphology and supermassive black hole mass in disk galaxies | Astrophysical Journal Letters | 2008 |
| Gravitational radiation timescales for extreme mass ratio inspirals RID E-8576-2010 | Astrophysical Journal | 2006 |
| Semirelativistic approximation to gravitational radiation from encounters with nonspinning black holes (vol 72, art no 084009, 2005) RID E-8576-2010 | Physical Review D | 2006 |
| Semirelativistic approximation to gravitational radiation from encounters with nonspinning black holes RID E-8576-2010 | Physical Review D | 2005 |
| Empire of the stars | TLS-The Times Literary Supplement | 2005 |
| Einstein versus the physical review | Physics Today | 2005 |
