activity
20182026
most citedImproving constraints on the reionization parameters using 21-cm bispectrum

34 citations · 235 across the 18 of their papers we have counts for

collaborators

18 papers

astro-ph.IM2026

Machine Learning and the SKA for Cosmic Dawn and the Epoch of Reionization

Anshuman Acharya, Michele Bianco, Daniela Breitman +18

When operational, the SKA will generate unprecedented amounts of data and provide exquisite sensitivity for 21 cm tomography of Cosmic Dawn (CD) and the Epoch of Reionization (EoR)…

astro-ph.CO2026

Cosmology with Multi-Wavelength Line Intensity Mapping Synergies in the SKAO Era

Debanjan Sarkar, Suman Majumdar, Chandra Shekhar Murmu +21

Line intensity mapping (LIM) has emerged as a powerful tool for surveying the large-scale structure of the Universe across cosmic time by measuring spatial fluctuations in the cumu…

astro-ph.CO2026

Cosmology with Intensity Mapping via Statistics Beyond the Power Spectrum in the SKAO Era

Suman Majumdar, Debanjan Sarkar, Leon Noble +38

The cosmological distribution of neutral hydrogen (HI) during the post-reionization era is highly non-Gaussian due to the underlying non-linear structure formation, complex galaxy…

astro-ph.CO2025★ 1 cited

Machine Learning-Driven Analysis of kSZ Maps to Predict CMB Optical Depth

Farshid Farhadi Khouzani, Abinash Kumar Shaw, Paul La Plante +2

Upcoming measurements of the kinetic Sunyaev-Zel'dovich (kSZ) effect, which results from Cosmic Microwave Background (CMB) photons scattering off moving electrons, offer a powerful…

astro-ph.CO2025★ 2 cited

From ANN to BNN: Inferring Reionization Parameters using Uncertainty-aware Emulators of 21-cm Summaries

Yashrajsinh Mahida, Sanjay Kumar Yadav, Suman Majumdar +6

Inferring astrophysical parameters from radio interferometric observations of the redshifted 21-cm signal from the Epoch of Reionization (EoR) is a challenging yet crucial task. Th…

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★ 10 cited

The monopole and quadrupole moments of the Epoch of Reionization (EoR) 21-cm bispectrum

Sukhdeep Singh Gill, Suman Pramanick, Somnath Bharadwaj +2

We study the monopole () and quadrupole () moments of the 21-cm bispectrum (BS) from EoR simulations and present results for squeezed and stretched triang…

astro-ph.IM2023★ 22 cited

SKA Science Data Challenge 2: analysis and results

P. Hartley, A. Bonaldi, R. Braun +105

The Square Kilometre Array Observatory (SKAO) will explore the radio sky to new depths in order to conduct transformational science. SKAO data products made available to astronomer…

astro-ph.CO2023★ 6 cited

Studying the Multi-frequency Angular Power Spectrum of the Cosmic Dawn 21-cm Signal

Abinash Kumar Shaw, Raghunath Ghara, Saleem Zaroubi +5

The light-cone (LC) anisotropy arises due to cosmic evolution of the cosmic dawn 21-cm signal along the line-of-sight (LoS) axis of the observation volume. The LC effect makes the…

astro-ph.CO2022★ 16 cited

Probing early universe through redshifted 21-cm signal: Modelling and observational challenges

Abinash Kumar Shaw, Arnab Chakraborty, Mohd Kamran +8

The redshifted 21-cm radiation from the atomic hydrogen (HI) provides an excellent direct probe to study the evolution of HI in IGM and thus reveal the nature of the first luminous…

astro-ph.IM2022

Detecting galaxies in a large H{\sc i}~spectral cube

Abinash Kumar Shaw, Manoj Jagannath, Aishrila Mazumder +4

The upcoming Square Kilometer Array (SKA) is expected to produce humongous amount of data for undertaking H{\sc i}~science. We have developed an MPI-based {\sc Python} pipeline to…

astro-ph.CO2021★ 34 cited

Improving constraints on the reionization parameters using 21-cm bispectrum

Himanshu Tiwari, Abinash Kumar Shaw, Suman Majumdar +2

Radio interferometric experiments aim to constrain the reionization model parameters by measuring the 21-cm signal statistics, primarily the power spectrum. However the Epoch of Re…

astro-ph.CO2021★ 13 cited

A fast estimator for quantifying the shape dependence of the 3D bispectrum

Abinash Kumar Shaw, Somnath Bharadwaj, Debanjan Sarkar +3

The dependence of the bispectrum on the size and shape of the triangle contains a wealth of cosmological information. Here we consider a triangle parameterization which allows us t…

astro-ph.CO2021★ 22 cited

The Epoch of Reionization 21-cm Bispectrum: The impact of light-cone effects and detectability

Rajesh Mondal, Garrelt Mellema, Abinash Kumar Shaw +2

We study the spherically averaged bispectrum of the 21-cm signal from the Epoch of Reionization (EoR). This metric provides a quantitative measurement of the level of non-Gaussiani…

astro-ph.CO2020★ 22 cited

The impact of non-Gaussianity on the Epoch of Reionization parameter forecast using 21-cm power spectrum measurements

Abinash Kumar Shaw, Somnath Bharadwaj, Rajesh Mondal

Measurements of the Epoch of Reionization (EoR) 21-cm signal hold the potential to constrain models of reionization. In this paper we consider a reionization model with three astro…

astro-ph.CO2019★ 28 cited

Predictions for measuring the 21-cm multi-frequency angular power spectrum using SKA-Low

Rajesh Mondal, Abinash Kumar Shaw, Ilian T. Iliev +5

The light-cone (LC) effect causes the mean as well as the statistical properties of the redshifted 21-cm signal to change with frequency (or cosmic t…

astro-ph.CO2019★ 30 cited

The impact of non-Gaussianity on the error covariance for observations of the Epoch of Reionization 21-cm power spectrum

Abinash Kumar Shaw, Somnath Bharadwaj, Rajesh Mondal

Recent simulations show the Epoch of Reionization (EoR) 21-cm signal to be inherently non-Gaussian whereby the error covariance matrix of the 21-cm power spectrum…

astro-ph.CO2018★ 25 cited

A method to determine the evolution history of the mean neutral Hydrogen fraction

Rajesh Mondal, Somnath Bharadwaj, Ilian T. Iliev +4

The light-cone (LC) effect imprints the cosmological evolution of the redshifted 21-cm signal along the frequency axis which is the line of sight (L…