Area of research
Astronomy and Astrophysics · Instrumentation
Research interest
Research interests include Physics, Astrophysics, Galaxy, Astronomy, Star formation, and Bulge.
Bar fraction and its dependence on host galaxy properties in the local Universe
Time-scales for the effects of interactions on galaxy properties and SMBH growth
Structural decomposition of merger-free galaxies hosting luminous AGNs
Galaxy Zoo DESI: large-scale bars as a secular mechanism for triggering AGNs
The Eighteenth Data Release of the Sloan Digital Sky Surveys: Targeting and First Spectra from SDSS-V
Post-starburst properties of post-merger galaxies
A Multiwavelength Study of Active Galactic Nuclei in Post-merger Remnants
The most luminous, merger-free AGNs show only marginal correlation with bar presence
Harnessing the Hubble Space Telescope Archives: A Catalog of 21,926 Interacting Galaxies
The Milky Way tomography with APOGEE: intrinsic density distribution and structure of mono-abundance populations
Resolved Molecular Gas Observations of MaNGA Post-starbursts Reveal a Tumultuous Past
Gems of the Galaxy Zoos—A Wide-ranging Hubble Space Telescope Gap-filler Program*
SDSS-IV MaNGA: How the stellar populations of passive central galaxies depend on stellar and halo mass
Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Cosmological implications from two decades of spectroscopic surveys at the Apache Point Observatory
Galaxy Zoo DECaLS: Detailed visual morphology measurements from volunteers and deep learning for 314 000 galaxies
H <scp>i</scp>-MaNGA: tracing the physics of the neutral and ionized ISM with the second data release
Kiloparsec-scale AGN outflows and feedback in merger-free galaxies
Galaxy zoo builder: Morphological dependence of spiral galaxy pitch angle
Erratum: Secularly powered outflows from AGNs: the dominance of non-merger driven supermassive black hole growth
SDSS-IV MaNGA: spatially resolved star formation in barred galaxies
SDSS-IV MaNGA: The link between bars and the early cessation of star formation in spiral galaxies
SDSS-IV MaNGA: spatially resolved dust attenuation in spiral galaxies
Are the Milky Way and Andromeda unusual? A comparison with Milky Way and Andromeda analogues
The Effect of Bars on the Ionized ISM: Optical Emission Lines from Milky Way Analogs
Galaxy Zoo DECaLS: Detailed Visual Morphology Measurements from Volunteers and Deep Learning for 314,000 Galaxies
Galaxy Zoo: probabilistic morphology through Bayesian CNNs and active learning
Galaxy Zoo: unwinding the winding problem – observations of spiral bulge prominence and arm pitch angles suggest local spiral galaxies are winding
SDSS-IV MaNGA: stellar population gradients within barred galaxies
Milky Way analogues in MaNGA: multiparameter homogeneity and comparison to the Milky Way
SDSS IV MaNGA – sSFR profiles and the slow quenching of discs in green valley galaxies