Area of research
Instrumentation · Astronomy and Astrophysics
Research interest
Research interests include Physics, Astrophysics, Galaxy, Astronomy, Reionization, and Redshift.
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
Little Red Dots: An Abundant Population of Faint Active Galactic Nuclei at z ∼ 5 Revealed by the EIGER and FRESCO JWST Surveys
The <i>JWST</i> EXCELS survey: too much, too young, too fast? Ultra-massive quiescent galaxies at 3 &lt; z &lt; 5
Accelerated formation of ultra-massive galaxies in the first billion years
Deciphering Lyman-α emission deep into the epoch of reionization
<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
Unveiling the hidden Universe with <i>JWST</i>: the contribution of dust-obscured galaxies to the stellar mass function at <i>z</i> ~ 3 – 8
Ionized Gas Kinematics with FRESCO: An Extended, Massive, Rapidly Rotating Galaxy at z = 5.4
The <i>JWST</i> FRESCO survey: legacy NIRCam/grism spectroscopy and imaging in the two GOODS fields
Unveiling the nature of infrared bright, optically dark galaxies with early <i>JWST</i> data
Two Remarkably Luminous Galaxy Candidates at z ≈ 10–12 Revealed by JWST
The prevalence of galaxy overdensities around UV-luminous Lyman 𝛼 emitters in the Epoch of Reionization
The Brightest z ≳ 8 Galaxies over the COSMOS UltraVISTA Field
The HDUV Survey: A Revised Assessment of the Relationship between UV Slope and Dust Attenuation for High-redshift Galaxies
Rotation in [C ii]-emitting gas in two galaxies at a redshift of 6.8
HST Imaging of the Brightest z ∼ 8–9 Galaxies from UltraVISTA: The Extreme Bright End of the UV Luminosity Function
SEDS: THE SPITZER EXTENDED DEEP SURVEY. SURVEY DESIGN, PHOTOMETRY, AND DEEP IRAC SOURCE COUNTS