activity
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

collaborators

62 papers

astro-ph.HE2025

ELAIS-N1 deep field uGMRT Band-2: constraints on diffuse Galactic synchrotron emission power spectrum

Rashmi Sagar, Abhirup Datta, Arnab Chakraborty +13

We present high sensitivity, low radio frequency continuum observations of the ELAIS-N1 field with 32 hours of observations of the uGMRT Band-2 ( MHz) covering $5.86\,\tex…

astro-ph.CO2025★ 1 cited

The Effect of Large Optical Depths on the Non-Gaussian 21-cm signal from Cosmic Dawn

Iffat Nasreen, Kanan K. Datta, Abinash K. Shaw +6

During the Cosmic Dawn (CD), the HI 21-cm optical depth ( ) in the intergalactic medium can become significantly large. Consequently, the second and higher-order terms of ap…

astro-ph.CO2024

The re-markable 21-cm power spectrum I: Probing the HI distribution in the post-reionization era using marked statistics

Mohd Kamran, Martin Sahlén, Debanjan Sarkar +1

The neutral hydrogen (HI) power spectrum, measured from intensity fluctuations in the 21-cm background, offers insights into the large-scale structures (LSS) of our Universe in the…

astro-ph.CO2024

Detecting ionized bubbles around luminous sources during the reionization era using HI 21-cm signal

Arnab Mishra, Chandra Shekhar Murmu, Kanan K. Datta +4

Measuring the properties of the intergalactic medium (IGM) and sources during the Epoch of Reionization (EoR) is of immense importance. We explore the prospects of probing the IGM…

astro-ph.CO2024★ 7 cited

Impact of the Epoch of Reionization sources on the 21-cm bispectrum

Leon Noble, Mohd Kamran, Suman Majumdar +5

The morphology of the 21-cm signal emitted by the neutral hydrogen present in the intergalactic medium (IGM) during the Epoch of Reionization (EoR) depends both on the properties o…

astro-ph.SR2024★ 23 cited

Project Hephaistos - II. Dyson sphere candidates from Gaia DR3, 2MASS, and WISE

Matías Suazo, Erik Zackrisson, Priyatam K. Mahto +5

The search for extraterrestrial intelligence is currently being pursued using multiple techniques and in different wavelength bands. Dyson spheres, megastructures that could be con…

astro-ph.CO2024★ 14 cited

Extracting the Global 21-cm signal from Cosmic Dawn and Epoch of Reionization in the presence of Foreground and Ionosphere

Anshuman Tripathi, Abhirup Datta, Madhurima Choudhury +1

Detection of redshifted \ion{H}{i} 21-cm emission is a potential probe for investigating the Universe's first billion years. However, given the significantly brighter foreground, d…

astro-ph.CO2023★ 6 cited

Impact of astrophysical scatter on the Epoch of Reionization [H I] bispectrum

Chandra Shekhar Murmu, Kanan K. Datta, Suman Majumdar +1

It is believed that the first star-forming galaxies are the main drivers of cosmic reionization. It is usually assumed that there is a one-to-one relationship between the star form…

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.CO2023

The morphology of the redshifted 21-cm signal from the Cosmic Dawn

Raghunath Ghara, Satadru Bag, Saleem Zaroubi +1

The spatial fluctuations in the tomographic maps of the redshifted 21-cm signal from the Cosmic Dawn (CD) crucially depend on the size and distribution of the regions with gas temp…

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.CO2022★ 5 cited

Probing the Epoch of Reionization using synergies of line intensity mapping

Chandra Shekhar Murmu, Raghunath Ghara, Suman Majumdar +1

The Epoch of Reionization (EoR) remains a poorly understood cosmic era for the most part. Yet, efforts are still going on to probe and understand this epoch. We present a review of…

astro-ph.HE2022★ 6 cited

Modelling the energy distribution in CHIME/FRB Catalog-1

Siddhartha Bhattacharyya, Somnath Bharadwaj, Himanshu Tiwari +1

We characterize the intrinsic properties of any FRB using its redshift , spectral index and energy in units of emitted across $2128 - 2848\; {\…

astro-ph.CO2022★ 18 cited

Observing the Reionization : Effect of Calibration and Position Errors on Realistic Observation Conditions

Aishrila Mazumder, Abhirup Datta, Arnab Chakraborty +1

Observation of the redshifted 21-cm signal from Cosmic Dawn and Epoch of Reionization is a challenging endeavor in observational cosmology. Presence of orders of magnitude brighter…

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.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…