output
19932026
most citedObservation of the rare decay from the combined analysis of CMS and LHCb data

508 citations

Showing astro-ph.COShow all

29 papers · 1 filter

astro-ph.CO2025

Tracing correlations between galaxy properties across the Cosmic Web: An IllustrisTNG-based study

Anindita Nandi, Biswajit Pandey, Prakash Sarkar

We explore the impact of cosmic web environments on galaxy properties such as colour, stellar mass, star formation rate, and stellar metallicity, using a stellar mass-matc…

astro-ph.CO2024★ 4 cited

Unveiling galaxy pair alignment in cosmic filaments: A 3D exploration using EAGLE simulation

Suman Sarkar, Biswajit Pandey

We investigate how galaxy pairs are oriented in three dimensions within cosmic filaments using data from the EAGLE simulation. We identify filament spines using DisPerSE and isolat…

astro-ph.CO2024★ 4 cited

The size and shape dependence of the SDSS galaxy bispectrum

Anindita Nandi, Sukhdeep Singh Gill, Debanjan Sarkar +3

We have measured the spherically averaged bispectrum of the SDSS main galaxy sample, considering a volume-limited data cube with mean galaxy number density $…

astro-ph.CO2023

Time evolution of the mutual information between disjoint regions in the Universe

Biswajit Pandey

We study the time evolution of the mutual information between the mass distributions in spatially separated but casually connected regions in an expanding universe. The evolution o…

astro-ph.CO2023★ 7 cited

The correlations between galaxy properties in different environments of the cosmic web

Anindita Nandi, Biswajit Pandey, Prakash Sarkar

We study the correlations between colour, stellar mass, specific star formation rate (sSFR) and metallicity of galaxies in different geometric environments of the cosmic we…

astro-ph.CO2022★ 6 cited

The maximum extent of the filaments and sheets in the cosmic web: an analysis of the SDSS DR17

Prakash Sarkar, Biswajit Pandey, Suman Sarkar

Filaments and sheets are striking visual patterns in cosmic web. The maximum extent of these large-scale structures are difficult to determine due to their structural variety and c…