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21 cm signal from cosmic dawn: imprints of spin temperature fluctuations and peculiar velocities

Monthly notices of the Royal Astronomical Society, 2015-02, Vol.447 (2), p.1806-1825

2015

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21 cm signal from cosmic dawn – II. Imprints of the light-cone effects

Monthly notices of the Royal Astronomical Society, 2015-11, Vol.453 (3), p.3143-3156

2015

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Bayesian approach to constraining the properties of ionized bubbles during reionization

Monthly notices of the Royal Astronomical Society, 2020-07, Vol.496 (1), p.739-753

2020

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Modelling the cosmic neutral hydrogen from DLAs and 21-cm observations

Monthly notices of the Royal Astronomical Society, 2016-05, Vol.458 (1), p.781-788

2016

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Imaging the redshifted 21 cm pattern around the first sources during the cosmic dawn using the SKA

Monthly notices of the Royal Astronomical Society, 2017-01, Vol.464 (2), p.2234-2234

2017

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Covariance matrices for the Lyman-α forest using the lognormal approximation

Journal of cosmology and astroparticle physics, 2024-04, Vol.2024 (4), p.66

2024

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Studying neutral hydrogen structures during the epoch of reionization using fractal dimensions

Monthly notices of the Royal Astronomical Society, 2017-04, Vol.466 (2), p.2302-2302

2017

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Reionization constraints on primordial magnetic fields

Monthly notices of the Royal Astronomical Society, 2015-08, Vol.451 (2), p.1692-1700

2015

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Cosmic reionization after Planck

Monthly notices of the Royal Astronomical Society. Letters, 2015-11, Vol.454 (1), p.L76-L80

2015

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Probing reionization using quasar near-zones at redshift z ∼ 6

Monthly notices of the Royal Astronomical Society, 2014-10, Vol.443 (4), p.3761-3779

2014

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Experimental constraints on self-consistent reionization models

Monthly notices of the Royal Astronomical Society, 2005-08, Vol.361 (2), p.577-594

2005

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Constraining the reionization history with QSO absorption spectra

Monthly notices of the Royal Astronomical Society, 2006-08, Vol.370 (3), p.1401-1421

2006

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Glimpsing through the high-redshift neutral hydrogen fog

Monthly notices of the Royal Astronomical Society, 2008-05, Vol.386 (1), p.359-369

2008

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Cosmic reionization after Planck II: contribution from quasars

Monthly notices of the Royal Astronomical Society, 2018-01, Vol.473 (1), p.1416-1425

2018

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Studying the Lyman α optical depth fluctuations at z ∼ 5.5 using fast semi-numerical methods

Monthly notices of the Royal Astronomical Society, 2021-03, Vol.501 (4), p.5782-5796

2021

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Theoretical and observational constraints on the H i intensity power spectrum

Monthly notices of the Royal Astronomical Society, 2015-03, Vol.447 (4), p.3745-3745

2015

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Simulating the epoch of helium reionization in photon-conserving semi-numerical code SCRIPT

Journal of cosmology and astroparticle physics, 2024-05, Vol.2024 (5), p.93

2024

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Photon number conserving models of H ii bubbles during reionization

Monthly notices of the Royal Astronomical Society, 2016-08, Vol.460 (2), p.1801-1810

2016

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Constraining thawing dark energy using galaxy cluster number counts

Monthly notices of the Royal Astronomical Society, 2013-06, Vol.432 (2), p.1513-1524

2013

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The escape fraction of ionizing photons from high-redshift galaxies from data-constrained reionization models

Monthly notices of the Royal Astronomical Society. Letters, 2013-01, Vol.428 (1), p.L1-L5

2013

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21-cm signature of the first sources in the Universe: prospects of detection with SKA

Monthly notices of the Royal Astronomical Society, 2016-07, Vol.460 (1), p.827-843

2016

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An improved model of H ii bubbles during the epoch of reionization

Monthly notices of the Royal Astronomical Society, 2014-08, Vol.442 (2), p.1470-1482

2014

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On the use of seminumerical simulations in predicting the 21-cm signal from the epoch of reionization

Monthly notices of the Royal Astronomical Society, 2014-10, Vol.443 (4), p.2843-2861

2014

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A GPR-based emulator for semi-numerical reionization code SCRIPT: parameter inference from 21 cm data

Journal of cosmology and astroparticle physics, 2024-03, Vol.2024 (3), p.27

2024

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Prediction of the 21-cm signal from reionization: comparison between 3D and 1D radiative transfer schemes

Monthly notices of the Royal Astronomical Society, 2018-05, Vol.476 (2), p.1741-1755

2018

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21 cm signal from cosmic dawn: imprints of spin temperature fluctuations and peculiar velocities

21 cm signal from cosmic dawn – II. Imprints of the light-cone effects

Bayesian approach to constraining the properties of ionized bubbles during reionization

Modelling the cosmic neutral hydrogen from DLAs and 21-cm observations

Imaging the redshifted 21 cm pattern around the first sources during the cosmic dawn using the SKA

Covariance matrices for the Lyman-α forest using the lognormal approximation

Studying neutral hydrogen structures during the epoch of reionization using fractal dimensions

Reionization constraints on primordial magnetic fields

Cosmic reionization after Planck

Probing reionization using quasar near-zones at redshift z ∼ 6

Experimental constraints on self-consistent reionization models

Constraining the reionization history with QSO absorption spectra

Glimpsing through the high-redshift neutral hydrogen fog

Cosmic reionization after Planck II: contribution from quasars

Studying the Lyman α optical depth fluctuations at z ∼ 5.5 using fast semi-numerical methods

Theoretical and observational constraints on the H i intensity power spectrum

Simulating the epoch of helium reionization in photon-conserving semi-numerical code SCRIPT

Photon number conserving models of H ii bubbles during reionization

Constraining thawing dark energy using galaxy cluster number counts

The escape fraction of ionizing photons from high-redshift galaxies from data-constrained reionization models

21-cm signature of the first sources in the Universe: prospects of detection with SKA

An improved model of H ii bubbles during the epoch of reionization

On the use of seminumerical simulations in predicting the 21-cm signal from the epoch of reionization

A GPR-based emulator for semi-numerical reionization code SCRIPT: parameter inference from 21 cm data

Prediction of the 21-cm signal from reionization: comparison between 3D and 1D radiative transfer schemes

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