We have carried a detailed analysis on the impact of cosmological redshift in the non-
parametric approach to automated galaxy morphology classification. We artificially …

The amount of power contained in the variations in galaxy star-formation histories (SFHs)
across a range of timescales encodes key information about the physical processes which …

With current and upcoming experiments such as the Wide Field Infrared Survey Telescope,
Euclid, and Large Synoptic Survey Telescope, we can observe up to billions of galaxies …

We present an analysis of star formation and quenching in the SDSS-IV MaNGA-DR15,
utilizing over 5 million spaxels from∼ 3500 local galaxies. We estimate star formation rate …

Morphological classification conveys abundant information on the formation, evolution, and
environment of galaxies. In this work, we refine a two-step galaxy morphological …

Historically, metallicity profiles of galaxies have been modelled using a radially symmetric,
two-parameter linear model, which reveals that most galaxies are more metal-rich in their …

In today's modern wide-field galaxy surveys, there is the necessity for parametric surface
brightness decomposition codes characterised by accuracy, small degree of user …

To study the role of environment in galaxy evolution, we reconstruct the underlying density
field of galaxies based on COSMOS2020 (The Farmer catalog) and provide the density …

Galaxies play a key role in our endeavor to understand how structure formation proceeds in
the Universe. For any precision study of cosmology or galaxy formation, there is a strong …

Quantifying galaxy morphology is a challenging yet scientifically rewarding task. As the
scale of data continues to increase with upcoming surveys, traditional classification methods …