Area of research
Instrumentation · Astronomy and Astrophysics
Research interest
Research interests include Physics, Astrophysics, Galaxy, Redshift, Star formation, and Stellar mass.
The Cosmic Evolution Early Release Science Survey (CEERS)
What Is the Nature of Little Red Dots and what Is Not, MIRI SMILES Edition
The evolution of star formation histories of quiescent galaxies
CEERS Key Paper. VIII. Emission-line Ratios from NIRSpec and NIRCam Wide-Field Slitless Spectroscopy at z > 2
The Ultraviolet Luminosity Function at 0.6 < z < 1 from UVCANDELS
Dusty Starbursts Masquerading as Ultra-high Redshift Galaxies in JWST CEERS Observations
CEERS Key Paper. IV. A Triality in the Nature of HST-dark Galaxies
First Look at z > 1 Bars in the Rest-frame Near-infrared with JWST Early CEERS Imaging
Two Massive, Compact, and Dust-obscured Candidate z ≃ 8 Galaxies Discovered by JWST
CEERS Key Paper. V. Galaxies at 4 < z < 9 Are Bluer than They Appear–Characterizing Galaxy Stellar Populations from Rest-frame ∼1 μm Imaging
A Milky Way-like barred spiral galaxy at a redshift of 3
An Updated Dust-to-Star Geometry: Dust Attenuation Does Not Depend on Inclination in 1.3 ≤z ≤2.6 Star-forming Galaxies from MOSDEF
A Long Time Ago in a Galaxy Far, Far Away: A Candidate z ∼ 12 Galaxy in Early JWST CEERS Imaging
The MOSDEF survey: the mass–metallicity relationship and the existence of the FMR at <i>z</i> ∼ 1.5
Quenching as a Contest between Galaxy Halos and Their Central Black Holes
The MOSDEF Survey: Neon as a Probe of ISM Physical Conditions at High Redshift<sup>*</sup>
The MOSDEF survey: direct-method metallicities and ISM conditions at z ∼ 1.5–3.5
The CANDELS/SHARDS Multiwavelength Catalog in GOODS-N: Photometry, Photometric Redshifts, Stellar Masses, Emission-line Fluxes, and Star Formation Rates
Optically faint massive Balmer break galaxies at z > 3 in the CANDELS/GOODS fields
LA Referencia (Red Federada de Repositorios Institucionales de Publicaciones Científicas) 2019cited by 48position: middle
The MOSDEF Survey: Significant Evolution in the Rest-frame Optical Emission Line Equivalent Widths of Star-forming Galaxies at z = 1.4–3.8
A simultaneous search for high-z LAEs and LBGs in the SHARDS survey
CANDELS Multi-wavelength Catalogs: Source Identification and Photometry in the CANDELS Extended Groth Strip
CANDELS MULTI-WAVELENGTH CATALOGS: SOURCE IDENTIFICATION AND PHOTOMETRY IN THE CANDELS COSMOS SURVEY FIELD
Structural and Star-forming Relations since z similar to 3: Connecting Compact Star-forming and Quiescent Galaxies
eScholarship (California Digital Library) 2017cited by 100position: first
Lyman continuum escape fraction of faint galaxies at <i>z</i> ~ 3.3 in the CANDELS/GOODS-North, EGS, and COSMOS fields with LBC
CANDELS: Elevated Black Hole Growth in the Progenitors of Compact Quiescent Galaxies at z ∼ 2
Major merging history in CANDELS. I. Evolution of the incidence of massive galaxy–galaxy pairs from z = 3 to z ∼ 0
Spatially Resolved Kinematics in the Central 1 kpc of a Compact Star-forming Galaxy at z ∼ 2.3 from ALMA CO Observations
shards: constraints on the dust attenuation law of star-forming galaxies at z ∼ 2
Galaxy Zoo: quantitative visual morphological classifications for 48 000 galaxies from CANDELS