Area of research
Astronomy and Astrophysics · Nuclear and High Energy Physics
Research interest
Research interests include Physics, Reionization, Astrophysics, HERA, Quasar, and Redshift.
Percent-level timing of reionisation: Self-consistent, implicit-likelihood inference from XQR-30+ Lyα forest data
Mapping reionization bubbles in JWST era
The reionizing bubble size distribution around galaxies
Hydrogen Epoch of Reionization Array (HERA) Phase II Deployment and Commissioning
IGM damping wing constraints on the tail end of reionization from the enlarged XQR-30 sample
Improved Constraints on the 21 cm EoR Power Spectrum and the X-Ray Heating of the IGM with HERA Phase I Observations
XQR-30: The ultimate XSHOOTER quasar sample at the reionization epoch
Probing Ultralate Reionization: Direct Measurements of the Mean Free Path over 5 < z < 6
Hydrogen reionization ends by <i>z</i> = 5.3: Lyman-α optical depth measured by the XQR-30 sample
First Results from HERA Phase I: Upper Limits on the Epoch of Reionization 21 cm Power Spectrum
HERA Phase I Limits on the Cosmic 21 cm Signal: Constraints on Astrophysics and Cosmology during the Epoch of Reionization
IGM damping wing constraints on reionization from covariance reconstruction of two <i>z</i> ≳ 7 QSOs
Suppression of black-hole growth by strong outflows at redshifts 5.8–6.6
Measuring the Density Fields around Bright Quasars at z ∼ 6 with XQR-30 Spectra
The impact of scatter in the galaxy UV luminosity to halo mass relation on Ly α visibility during the epoch of reionization
Mitigating Internal Instrument Coupling for 21 cm Cosmology. II. A Method Demonstration with the Hydrogen Epoch of Reionization Array
Redundant-baseline calibration of the hydrogen epoch of reionization array
Optimizing sparse RFI prediction using deep learning
The Universe Is Reionizing at z ∼ 7: Bayesian Inference of the IGM Neutral Fraction Using Lyα Emission from Galaxies
Are we witnessing the epoch of reionisation at <i>z</i> = 7.1 from the spectrum of J1120+0641?
Lyα emission-line reconstruction for high-<i>z</i>QSOs
First limits on the 21 cm power spectrum during the Epoch of X-ray heating
Constraining high-redshift X-ray sources with next generation 21-cm power spectrum measurements
Model-independent evidence in favour of an end to reionization by z ≈ 6
Reionization and beyond: detecting the peaks of the cosmological 21 cm signal