Research

Stemming from my passions towards theoretical physics since my undergraduate days, my research interests have been mostly focussed on cosmology, gravity, early universe, galactic dynamics and dark matter. Broadly I like to work on a field where there is a healthy combination of theory, observational data and statistical modelling.

Doctoral research: power-spectrum analysis of early-type galaxies

For my PhD thesis I worked on a project on quantifying the distribution of dark matter in massive elliptical galaxies using strong gravitational lensing at Leon Koopman’s group. I developed a statistical methodology to measure the mass power-spectrum of early type lens galaxies in the 1-10 kpc scales. In collaboration with the other members of the research group, we also applied the theory to Hubble Space Telescope (HST) imaging of the galaxy-galaxy strong gravitational lens system SDSS J0252+0039 and gave observational constraints on the sub-galactic matter-power spectrum. Below I show the lens and it’s surface brightness modeling:

stiff_HIU_original
Color-composite image of SDSS J0252+0039 based  on U-band (blue), visual (green) and infrared bands (red).
Smooth_n3_final
Smooth-lens modelling of SDSS J0252+0039 in the U-band by means of an adaptive and grid-based Bayesian lens-modelling technique.

We looked at the residuals and had done power spectrum analysis to statistically infer the fluctuations in the lens potential which might arise from the low mass substructures (for details of this work, look Dorota et al, arXiv:1803.05952). We also compared different galaxy formation scenarios using the state-of-the-art N-body hydrodynamic simulation Evolution and Assembly of GaLaxies and their Environments (EAGLE). In order to perform such comparative analysis, we applied the power-spectrum formalism to the simulated galaxies to gain insights about the sub-grid physics behind the galaxy formation and evolution.

REFERENCE
A subset of strong lenses simulated from EAGLE (Reference model), 50 cMpc box, redshift z = 0.271

Application of AI in strong-lensing:

Since 2015, I have also been involved in a project of applying artificial intelligence in the fields of astronomy. We used Convolutional Neural Network (CNN) to find the strong-lens galaxies in Kilo Degree Survey (KiDS). This work was also highlighted by a press release. My contribution in this work (and the follow up papers) was mostly in simulating the training set for the CNN, consisting of a large number of realistic lens-galaxies — some examples are given below:

simulated_source
Simulated lensed images. The image size is 101×101 pixels, corresponding to 20×20 arcsec

Below I show few RGB images out of the 56 candidates down-selected through a visual inspection of the 761 CNN candidates:

Post-doctoral research:

Currently, as part of my post-doctoral research at Target Field Lab, I am primarily working on data mining and data validation — with a special emphasis on text mining and Natural Language Processing (NLP) using Deep Learning networks, such as hierarchical attention networks, BERT Question-Answering system etc.

Tasks in Natural Language Understanding (NLU), Natural Language Processing (NLP) and Automatic Speech Recognition (ASR).
Source: https://nlp.stanford.edu/~wcmac/papers/20140716-UNLU.pdf

Master thesis and undergraduate research:

My Masters and Bachelor research thesis are titled briefly below:

During my Masters I was also involved in two short projects on Gravitational Waves Data Analysis and Numerical Relativity (Unuqual-mass precessing binary black-hole simulations).

Websites and links:

University of Groningen profile page