activity
20142026
most citedImproved upper limits on the 21-cm signal power spectrum of neutral hydrogen at from LOFAR

311 citations · 1.7k across the 46 of their papers we have counts for

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40 papers · 1 filter

astro-ph.CO2026

Accurate parameter inference for the Light-cone Epoch of Reionization 21-cm signal

Suman Pramanick, Anoop Krishna, Rajesh Mondal +1

The light-cone (LC) effect introduces line-of-sight (LoS) statistical inhomogeneity into the 21-cm signal. Consequently, the traditional power spectrum (PS) fails to capture the fu…

astro-ph.CO2026

Inferring Cosmology and Astrophysics from the High-redshift 21cm Signal with SKA-Low

Anshuman Acharya, Satadru Bag, Sabrina Berger +29

The Square Kilometre Array's low frequency telescope (SKA-Low) will enable inference of astrophysical and cosmological parameters from the redshifted 21 cm signal, probing the Cosm…

astro-ph.CO2026

Constraining the neutral hydrogen fraction during reionization: Cross-simulation inference using power spectrum and bispectrum

Anoop Krishna, Deepthi Moorkanat, Hiten +1

The redshifted 21-cm signal is a unique probe of the early universe, particularly the Epoch of Reionization (EoR). While the 21-cm power spectrum has been the primary statistic for…

astro-ph.CO2025★ 1 cited

The Evolving Power Spectrum for the light cone Epoch of Reionization (EoR) 21-cm signal

Suman Pramanick, Somnath Bharadwaj, Khandakar Md Asif Elahi +1

The rapid evolution of the cosmological neutral hydrogen (HI) distribution during the EoR is imprinted along the line of sight (LoS) in the redshifted 21-cm signal due to the light…

astro-ph.CO2023★ 15 cited

Constraining exotic dark matter models with the dark ages 21-cm signal

Rajesh Mondal, Rennan Barkana, Anastasia Fialkov

The dark ages 21-cm signal is a powerful tool for precision cosmology and probing new physics. We study two non-standard models: an excess radio background (ERB) model (possibly ge…

astro-ph.CO2023★ 41 cited

Prospects for precision cosmology with the 21 cm signal from the dark ages

Rajesh Mondal, Rennan Barkana

The 21 cm signal from the dark ages provides a potential new probe of fundamental cosmology. While exotic physics could be discovered, here we quantify the expected benefits within…

astro-ph.CO2023★ 16 cited

POLAR -- I: linking the 21-cm signal from the epoch of reionization to galaxy formation

Qing-Bo Ma, Raghunath Ghara, Benedetta Ciardi +5

To self-consistently model galactic properties, reionization of the intergalactic medium, and the associated 21-cm signal, we have developed the algorithm polar by integrating the…

astro-ph.CO2023

Quantifying and mitigating the effect of snapshot interval in light-cone Epoch of Reionization 21-cm simulations

Suman Pramanick, Rajesh Mondal, Somnath Bharadwaj

The Epoch of Reionization (EoR) neutral Hydrogen (HI) 21-cm signal evolves significantly along the line-of-sight (LoS) due to the light-cone (LC) effect. It is important to accurat…

astro-ph.CO2023★ 40 cited

Inflaton phenomenology via reheating in light of primordial gravitational waves and the latest BICEP/ data

Ayan Chakraborty, Md Riajul Haque, Debaprasad Maity +1

We are in the era of precision cosmology which offers us a unique opportunity to investigate beyond standard model physics. Toward this endeavor, inflaton is assumed to be a perfec…

astro-ph.CO2023★ 6 cited

Interpreting the HI 21-cm cosmology maps through Largest Cluster Statistics -- I: Impact of the synthetic SKA1-Low observations

Saswata Dasgupta, Samit Kumar Pal, Satadru Bag +7

We analyse the evolution of the largest ionized region using the topological and morphological evolution of the redshifted 21-cm signal coming from the neutral hydrogen distributio…

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★ 9 cited

Multi-frequency angular power spectrum of the 21~cm signal from the Epoch of Reionisation using the Murchison Widefield Array

Cathryn M. Trott, Rajesh Mondal, Garrelt Mellema +5

The Multi-frequency Angular Power Spectrum (MAPS) is an alternative to spherically-averaged power spectra, and computes local fluctuations in the angular power spectrum without nee…

astro-ph.CO2022★ 13 cited

Redshifted 21-cm bispectrum: Impact of the source models on the signal and the IGM physics from the Cosmic Dawn

Mohd Kamran, Raghunath Ghara, Suman Majumdar +5

The radiations from the first luminous sources drive the fluctuations in the 21-cm signal at Cosmic Dawn (CD) via two dominant astrophysical processes i.e. the Ly coupling and X…

astro-ph.CO2022★ 13 cited

The multi-frequency angular power spectrum in parameter studies of the cosmic 21-cm signal

Rajesh Mondal, Garrelt Mellema, Steven G. Murray +1

The light-cone effect breaks the periodicity and statistical homogeneity (ergodicity) along the line-of-sight direction of cosmological emission/absorption line surveys. The spheri…

astro-ph.CO2021★ 19 cited

The large-scale 21-cm power spectrum from reionization

Ivelin Georgiev, Garrelt Mellema, Sambit K. Giri +1

Radio interferometers, such as the Low-Frequency Array and the future Square Kilometre Array, are attempting to measure the spherically averaged 21-cm power spectrum from the Epoch…

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★ 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…

astro-ph.CO2020★ 40 cited

Redshifted 21-cm Bispectrum I: Impact of the Redshift Space Distortions on the Signal from the Epoch of Reionization

Suman Majumdar, Mohd Kamran, Jonathan R. Pritchard +4

The bispectrum can quantify the non-Gussianity present in the redshifted 21-cm signal produced by the neutral hydrogen (HI) during the epoch of reionization (EoR). Motivated by thi…

astro-ph.CO2020★ 82 cited

Interpreting LOFAR 21-cm signal upper limits at z~9.1 in the context of high-z galaxy and reionisation observations

Bradley Greig, Andrei Mesinger, Léon V. E. Koopmans +11

Using the latest upper limits on the 21-cm power spectrum at from the Low Frequency Array (LOFAR), we explore regions of parameter space which are inconsistent with t…

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.CO2020★ 88 cited

Tight Constraints on the Excess Radio Background at from LOFAR

R. Mondal, A. Fialkov, C. Fling +13

The ARCADE2 and LWA1 experiments have claimed an excess over the Cosmic Microwave Background (CMB) at low radio frequencies. If the cosmological high-redshift contribution to this…

astro-ph.CO2020★ 311 cited

Improved upper limits on the 21-cm signal power spectrum of neutral hydrogen at from LOFAR

F. G. Mertens, M. Mevius, L. V. E Koopmans +23

A new upper limit on the 21-cm signal power spectrum at a redshift of is presented, based on 141 hours of data obtained with the Low-Frequency Array (LOFAR). The an…

astro-ph.CO2020★ 109 cited

Constraining the intergalactic medium at 9.1 using LOFAR Epoch of Reionization observations

R. Ghara, S. K. Giri, G. Mellema +19

We derive constraints on the thermal and ionization states of the intergalactic medium (IGM) at redshift 9.1 using new upper limits on the 21-cm power spectrum measured b…