activity
20182021
most citedThe auto and cross angular power spectrum of the Cas A supernova remnant in radio and X-ray

8 citations · 10 across the 4 of their papers we have counts for

collaborators

7 papers

cond-mat.str-el2021

Honeycomb-lattice Gamma model in a magnetic field: hidden Néel order and spin-flop transition

Zhongzheng Tian, Zhijie Fan, Preetha Saha +1

We show that a magnetic field in the high-symmetry direction lifts the macroscopic classical ground-state degeneracy of the honeycomb model and induces a long-range magnetic or…

astro-ph.GA20218 cited

The auto and cross angular power spectrum of the Cas A supernova remnant in radio and X-ray

Preetha Saha, Somnath Bharadwaj, Susmita Chakravorty +4

The shell type supernova remnant (SNR) Cas A exhibits structures at nearly all angular scales. Previous studies show the angular power spectrum of the radio emission t…

astro-ph.GA20201 cited

Angular power spectrum of supernova remnants: effects of structure, geometry and diffuse foreground

Samir Choudhuri, Preetha Saha, Nirupam Roy +2

The study of the intensity fluctuation power spectrum of individual supernova remnants (SNRs) can reveal the structures present at sub-pc scales, and also constrain the physical pr…

cond-mat.str-el20201 cited

Machine learning dynamics of phase separation in correlated electron magnets

Puhan Zhang, Preetha Saha, Gia-Wei Chern

We demonstrate machine-learning enabled large-scale dynamical simulations of electronic phase separation in double-exchange system. This model, also known as the ferromagnetic Kond…

astro-ph.GA2019

A study of Kepler supernova remnant: angular power spectrum estimation from radio frequency data

Preetha Saha, Somnath Bharadwaj, Nirupam Roy +2

Supernova remnants (SNRs) have a variety of overall morphology as well as rich structures over a wide range of scales. Quantitative study of these structures can potentially reveal…

astro-ph.GA2018

On estimating the atomic hydrogen column density from the H I 21 cm emission spectra

Preetha Saha, Nirupam Roy, Mukul Bhattacharya

The 21 cm hyperfine transition of the atomic hydrogen (HI) in ground state is a powerful probe of the neutral gas content of the universe. This radio frequency transition has been…