Area of research
Astronomy and Astrophysics · Instrumentation
Research interest
Research interests include Galaxies: Formation, Evolution, Phenomena, Astronomy and Astrophysical Research, Stellar, planetary, and galactic studies, and Gamma-ray bursts and supernovae.
Structural decomposition of merger-free galaxies hosting luminous AGNs
The MOSDEF survey: properties of warm ionized outflows at <i>z</i> = 1.4–3.8
The Impact of Star-formation-rate Surface Density on the Electron Density and Ionization Parameter of High-redshift Galaxies*
CO Emission, Molecular Gas, and Metallicity in Main-sequence Star-forming Galaxies at z ∼ 2.3*
An Updated Dust-to-Star Geometry: Dust Attenuation Does Not Depend on Inclination in 1.3 ≤z ≤2.6 Star-forming Galaxies from MOSDEF
Kinematics, Structure, and Mass Outflow Rates of Extreme Starburst Galactic Outflows
The most luminous, merger-free AGNs show only marginal correlation with bar presence
The Spatial Clustering of ROSAT All-Sky Survey Active Galactic Nuclei. V. The Evolution of Broad-line AGN Clustering Properties in the Last 6 Gyr
The MOSDEF-LRIS survey: detection of inflowing gas towards three star-forming galaxies at <i>z</i> ∼ 2
Exploring the correlation between H<i>α</i>-to-UV ratio and burstiness for typical star-forming galaxies at <i>z</i> ∼ 2
The Effects of Stellar Population and Gas Covering Fraction on the Emergent Lyα Emission of High-redshift Galaxies*
The MOSFIRE Deep Evolution Field Survey: Implications of the Lack of Evolution in the Dust Attenuation–Mass Relation to z ∼ 2*
Infrared Spectral Energy Distributions and Dust Masses of Sub-solar Metallicity Galaxies at z ∼ 2.3
The dust-to-gas mass ratio of luminous galaxies as a function of their metallicity at cosmic noon
The MOSDEF-LRIS survey: connection between galactic-scale outflows and the properties of <i>z</i> ∼ 2 star-forming galaxies
The MOSDEF survey: the mass–metallicity relationship and the existence of the FMR at <i>z</i> ∼ 1.5
Compact Starburst Galaxies with Fast Outflows: Central Escape Velocities and Stellar Mass Surface Densities from Multiband Hubble Space Telescope Imaging
Erratum: Secularly powered outflows from AGNs: the dominance of non-merger driven supermassive black hole growth
The MOSDEF Survey: The First Direct Measurements of the Nebular Dust Attenuation Curve at High Redshift*
The MOSDEF-LRIS Survey: The Interplay Between Massive Stars and Ionized Gas in High-Redshift Star-Forming Galaxies1
The MOSDEF-LRIS Survey: The connection between massive stars and ionized gas in individual galaxies at <i>z</i> ∼ 2
The MOSDEF Survey: Neon as a Probe of ISM Physical Conditions at High Redshift<sup>*</sup>
The MOSDEF Survey: calibrating the relationship between H α star formation rate and radio continuum luminosity at 1.4 &lt; <i>z</i> &lt; 2.6
The MOSDEF survey: direct-method metallicities and ISM conditions at z ∼ 1.5–3.5
X-rays across the galaxy population – III. The incidence of AGN as a function of star formation rate
The MOSDEF Survey: Significant Evolution in the Rest-frame Optical Emission Line Equivalent Widths of Star-forming Galaxies at z = 1.4–3.8
X-rays across the galaxy population – II. The distribution of AGN accretion rates as a function of stellar mass and redshift
The evolution of the hard X-ray luminosity function of AGN
2016cited by 222position: middle
A massive, quiescent, population II galaxy at a redshift of 2.1
X-rays across the galaxy population – I. Tracing the main sequence of star formation
Collaborative Research: Extreme Starbursts and Outflows: The Formation of Massive Compact Galaxies
Collaborative Research: The MOSFIRE Deep Evolution Field Survey.
CAREER: Galaxy Evolution Over Half of Cosmic History
Collaborative Research:Finding the Gas that lights up Galaxies
Collaborative Research: Tracking Galaxy Growth with 200,000 Spectroscopic Redshifts