Area of research
Astronomy and Astrophysics · Instrumentation
Research interest
Research interests include Galaxies: Formation, Evolution, Phenomena, Astronomy and Astrophysical Research, Astrophysics and Star Formation Studies, and Stellar, planetary, and galactic studies.
Accelerated formation of ultra-massive galaxies in the first billion years
JWST/CEERS sheds light on dusty star-forming galaxies: Forming bulges, lopsidedness, and outside-in quenching at cosmic noon
Noema formIng Cluster survEy (NICE): Discovery of a starbursting galaxy group with a radio-luminous core at <i>z</i> = 3.95
CEERS: 7.7 μm PAH Star Formation Rate Calibration with JWST MIRI
Dusty Starbursts Masquerading as Ultra-high Redshift Galaxies in JWST CEERS Observations
The Physical Conditions of Emission-line Galaxies at Cosmic Dawn from JWST/NIRSpec Spectroscopy in the SMACS 0723 Early Release Observations
Two Massive, Compact, and Dust-obscured Candidate z ≃ 8 Galaxies Discovered by JWST
JWST CEERS probes the role of stellar mass and morphology in obscuring galaxies
A<sup>3</sup>COSMOS: The infrared luminosity function and dust-obscured star formation rate density at 0.5 < <i>z</i> < 6
CEERS: Spatially Resolved UV and Mid-infrared Star Formation in Galaxies at 0.2 < z < 2.5: The Picture from the Hubble and James Webb Space Telescopes
ALMA FIR View of Ultra-high-redshift Galaxy Candidates at z ∼ 11–17: Blue Monsters or Low-z Red Interlopers?
A Long Time Ago in a Galaxy Far, Far Away: A Candidate z ∼ 12 Galaxy in Early JWST CEERS Imaging
CCAT-prime Collaboration: Science Goals and Forecasts with Prime-Cam on the Fred Young Submillimeter Telescope
Turbulent Gas in Lensed Planck-selected Starbursts at z ∼ 1–3.5
GOODS-ALMA: 1.1 mm galaxy survey
THE ALMA SPECTROSCOPIC SURVEY IN THE HUBBLE ULTRA DEEP FIELD: CONTINUUM NUMBER COUNTS, RESOLVED 1.2 mm EXTRAGALACTIC BACKGROUND, AND PROPERTIES OF THE FAINTEST DUSTY STAR-FORMING GALAXIES
THE ALMA SPECTROSCOPIC SURVEY IN THE HUBBLE ULTRA DEEP FIELD: MOLECULAR GAS RESERVOIRS IN HIGH-REDSHIFT GALAXIES
COMBINED CO AND DUST SCALING RELATIONS OF DEPLETION TIME AND MOLECULAR GAS FRACTIONS WITH COSMIC TIME, SPECIFIC STAR-FORMATION RATE, AND STELLAR MASS
SUBMILLIMETER GALAXIES AS PROGENITORS OF COMPACT QUIESCENT GALAXIES
Tracing the cosmic growth of supermassive black holes to z ∼ 3 with Herschel★
The far-infrared/radio correlation and radio spectral index of galaxies in the SFR–<i>M</i><sub>∗</sub>plane up to<i>z</i>~2
A multiwavelength consensus on the main sequence of star-forming galaxies at z ∼ 2
The host galaxies of X-ray selected active galactic nuclei to<i>z</i>= 2.5: Structure, star formation, and their relationships from CANDELS and<i>Herschel</i>/PACS
Linking the X-ray and infrared properties of star-forming galaxies at z < 1.5★
Large-scale clustering measurements with photometric redshifts: comparing the dark matter haloes of X-ray AGN, star-forming and passive galaxies at z ≈ 1
The evolution of galaxy star formation activity in massive haloes
The Herschel★ PEP/HerMES luminosity function – I. Probing the evolution of PACS selected Galaxies to z ≃ 4
The incidence of obscuration in active galactic nuclei
The evolution of the dust and gas content in galaxies
The evolution of the dust temperatures of galaxies in the SFR–<i>M</i><sub>∗</sub>plane up to<i>z</i> ~ 2