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20082025
most citedUpper limits on the 21-cm Epoch of Reionization power spectrum from one night with LOFAR

290 citations · 1.8k across the 59 of their papers we have counts for

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Showing 2021Show all

10 papers · 1 filter

astro-ph.CO2021★ 21 cited

Extracting the 21-cm Power Spectrum and the reionization parameters from mock datasets using Artificial Neural Networks

Madhurima Choudhury, Abhirup Datta, Suman Majumdar

Detection of the \hi~ 21-cm power spectrum is one of the key science drivers of several ongoing and upcoming low-frequency radio interferometers. However, the major challenge in su…

astro-ph.CO2021★ 5 cited

Large HI optical depth and Redshifted 21-cm signal from cosmic dawn

Kanan K. Datta, Raghunath Ghara, Ariful Hoque +1

The HI 21-cm optical depth () can be considerably large as the kinetic and spin temperature of the inter-galactic medium (IGM) is expected to be very low during cosmic dawn. I…

astro-ph.CO2021★ 17 cited

Revisiting the [C II] line-intensity mapping power spectrum from the EoR using non-uniform line-luminosity scatter

Chandra Shekhar Murmu, Karen P. Olsen, Thomas R. Greve +9

Detecting the line-intensity mapping (LIM) signal from the galaxies of the Epoch of Reionization is an emerging tool to constrain their role in reionization. Ongoing and upcoming e…

astro-ph.HE2021★ 6 cited

A maximum likelihood estimate of the parameters of the FRB population

Siddhartha Bhattacharyya, Himanshu Tiwari, Somnath Bharadwaj +1

We consider a sample of non-repeating FRBs detected at Parkes, ASKAP, CHIME and UTMOST each of which operates over a different frequency range and has a different detection cr…

astro-ph.CO2021★ 13 cited

CII and HI 21-cm line intensity mapping from the EoR: Impact of the light-cone effect on auto and cross-power spectra

Chandra Shekhar Murmu, Suman Majumdar, Kanan K. Datta

CII line intensity mapping (LIM) is a potential technique to probe the early galaxies from the Epoch of Reionization (EoR). Several experiments e.g. CONCERTO, TIME, CCAT-p are unde…

astro-ph.CO2021★ 1 cited

Probing IGM Physics during Cosmic Dawn using the Redshifted 21-cm Bispectrum

Mohd Kamran, Suman Majumdar, Raghunath Ghara +5

With the advent of the first luminous sources at Cosmic Dawn (CD), the redshifted 21-cm signal, from the neutral hydrogen in the Inter-Galactic Medium (IGM), is predicted to underg…

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.CO2021★ 35 cited

Redshifted 21-cm bispectrum II: Impact of the spin temperature fluctuations and redshift space distortions on the signal from the Cosmic Dawn

Mohd Kamran, Raghunath Ghara, Suman Majumdar +5

We present a study of the 21-cm signal bispectrum (which quantifies the non-Gaussianity in the signal) from the Cosmic Dawn (CD). For our analysis, we have simulated the 21-cm sign…