Area of research
Astronomy and Astrophysics · Instrumentation
Research interest
Research interests include Astronomy and Astrophysical Research, Galaxies: Formation, Evolution, Phenomena, Stellar, planetary, and galactic studies, and Astrophysics and Star Formation Studies.
The Ly <i>α</i> and Continuum Origins Survey. II. The Connection between the Escape of Ionizing Radiation and Ly <i>α</i> Halos in Star-forming Galaxies
The AURORA survey: the evolution of multiphase electron densities at high redshift
Mapping dusty galaxy growth at <i>z</i> &gt; 5 with FRESCO: detection of Hα in submm galaxy HDF850.1 and the surrounding overdense structures
The first billion years according to JWST
Accelerated formation of ultra-massive galaxies in the first billion years
<i>JWST</i> FRESCO: a comprehensive census of H <i>β</i> + [O <scp>iii</scp>] emitters at 6.8 &lt; z &lt; 9.0 in the GOODS fields
Multivariate Predictors of Lyman Continuum Escape. I. A Survival Analysis of the Low-redshift Lyman Continuum Survey*
Ubiquitous broad-line emission and the relation between ionized gas outflows and Lyman continuum escape in Green Pea galaxies
JWST and ALMA Multiple-line Study in and around a Galaxy at z = 8.496: Optical to Far-Infrared Line Ratios and the Onset of an Outflow Promoting Ionizing Photon Escape
Linking Mg II and [O II] spatial distribution to ionizing photon escape in confirmed LyC leakers and non-leakers
The cold interstellar medium of a normal sub-<i>L</i><sup>⋆</sup> galaxy at the end of reionization
The <i>JWST</i> FRESCO survey: legacy NIRCam/grism spectroscopy and imaging in the two GOODS fields
The Gas and Stellar Content of a Metal-poor Galaxy at <i>z</i> = 8.496 as Revealed by JWST and ALMA
Clues on the presence and segregation of very massive stars in the Sunburst Lyman-continuum cluster at <i>z</i> = 2.37
Molecular gas cloud properties at<i>z</i>≃ 1 revealed by the superb angular resolution achieved with ALMA and gravitational lensing
Metal-enriched Neutral Gas Reservoir around a Strongly Lensed Low-mass Galaxy at z = 4 Identified by JWST/NIRISS and VLT/MUSE
The Low-redshift Lyman Continuum Survey. I. New, Diverse Local Lyman Continuum Emitters
The Low-redshift Lyman Continuum Survey. II. New Insights into LyC Diagnostics
The far-ultraviolet continuum slope as a Lyman Continuum escape estimator at high redshift
The VIMOS Ultra Deep Survey: The reversal of the star-formation rate − density relation at 2 <<i>z</i>< 5
The ALMA REBELS Survey: Average [C ii] 158 μm Sizes of Star-forming Galaxies from z ∼ 7 to z ∼ 4
Tracing Lyα and LyC Escape in Galaxies with Mg ii Emission
The ALPINE-ALMA [C II] survey. Dust attenuation curves at <i>z</i> = 4.4–5.5
The synchrony of production and escape: half the bright Lyα emitters at <i>z</i> ≈ 2 have Lyman continuum escape fractions ≈50
The ALPINE-ALMA [CII] survey
The VANDELS ESO public spectroscopic survey
The ALPINE-ALMA [C <scp>ii</scp>] Survey: kinematic diversity and rotation in massive star-forming galaxies at <i>z</i> ~ 4.4–5.9
The ALPINE-ALMA [C II] survey: Luminosity function of serendipitous [C II] line emitters at z ∼5
The ALPINE-ALMA [CII] survey
The ALPINE-ALMA [CII] survey