Area of research
Astronomy and Astrophysics · Instrumentation
Research interest
Research interests include Galaxies: Formation, Evolution, Phenomena, Astronomy and Astrophysical Research, Gamma-ray bursts and supernovae, and Stellar, planetary, and galactic studies.
JWST spectroscopic confirmation of the Cosmic Gems arc at <i>z</i> = 9.625
The <i>z</i> = 9.625 Cosmic Gems galaxy was a compact “blue monster” propelled by massive star clusters
A Radio Flare in the Long-lived Afterglow of the Distant Short GRB 210726A: Energy Injection or a Reverse Shock from Shell Collisions?
The host of GRB 171205A in 3D
Cosmography from accurate mass modeling of the lens group SDSS J0100+1818: Five sources at three different redshifts
Origin of the Strong Sodium Absorption of the Lensed Supernova 2016geu at z = 0.4
Heavy-element production in a compact object merger observed by JWST
JWST detection of heavy neutron capture elements in a compact object merger
The THESEUS space mission: science goals, requirements and mission concept
Exploration of the high-redshift universe enabled by THESEUS
Exploration of the high-redshift universe enabled by THESEUS
STRIDES: a 3.9 per cent measurement of the Hubble constant from the strong lens system DES J0408−5354
Compact binary mergers: R-process kilonovae and ultra-relativistic jets
UWA Profiles and Research Repository (University of Western Australia) 2020cited by 0position: middle
Linking gas and galaxies at high redshift: MUSE surveys the environments of six damped Lyα systems at z ≈ 3
FIGS: spectral fitting constraints on the star formation history of massive galaxies since the cosmic noon
Extreme magnification of an individual star at redshift 1.5 by a galaxy-cluster lens
New constraints on the free-streaming of warm dark matter from intermediate and small scale Lyman-<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi>α</mml:mi></mml:math> forest data
The most distant, luminous, dusty star-forming galaxies: redshifts from NOEMA and ALMA spectral scans
FIGS—Faint Infrared Grism Survey: Description and Data Reduction
Extreme magnification of a star at redshift 1.5 by a galaxy-cluster lens
2017cited by 6position: middle
HIGH-RESOLUTION SPECTROSCOPY OF A YOUNG, LOW-METALLICITY OPTICALLY THIN L = 0.02L* STAR-FORMING GALAXY AT z = 3.12*
XQ-100: A legacy survey of one hundred 3.5 ≲<i>z</i>≲ 4.5 quasars observed with VLT/X-shooter
A young star-forming galaxy at<i>z</i>= 3.5 with an extended Lyman α halo seen with MUSE
A merger in the dusty,<i>z</i>= 7.5 galaxy A1689-zD1?
Nature and statistical properties of quasar associated absorption systems in the XQ-100 Legacy Survey
Dark matter fraction of low-mass cluster members probed by galaxy-scale strong lensing
Emission-line-selected galaxies at<i>z</i>= 0.6–2 in GOODS South: Stellar masses, SFRs, and large-scale structure
MUSE integral-field spectroscopy towards the Frontier Fields cluster Abell S1063
Testing metallicity indicators at z ∼ 1.4 with the gravitationally lensed galaxy CASSOWARY 20★
CLASH: EXTENDING GALAXY STRONG LENSING TO SMALL PHYSICAL SCALES WITH DISTANT SOURCES HIGHLY MAGNIFIED BY GALAXY CLUSTER MEMBERS