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Shiv K. Sethi

Researcher at Raman Research Institute

Publications -  99
Citations -  2730

Shiv K. Sethi is an academic researcher from Raman Research Institute. The author has contributed to research in topics: Redshift & Reionization. The author has an hindex of 28, co-authored 87 publications receiving 2400 citations. Previous affiliations of Shiv K. Sethi include Institut d'Astrophysique de Paris & Inter-University Centre for Astronomy and Astrophysics.

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FIRST SEASON MWA EOR POWER SPECTRUM RESULTS at REDSHIFT 7

Adam P. Beardsley, +72 more
TL;DR: In this article, the authors introduce several novel analysis techniques, such as cable reflection calibration, hyper-resolution gridding kernels, diffuse foreground model subtraction, and quality control methods, and incorporate the new techniques into a deep integration of 32 hours of MWA data.
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Primordial magnetic fields in the post‐recombination era and early reionization

TL;DR: In this article, the authors explore the ways in which primordial magnetic fields influence the thermal and ionization history of the post-recombination Universe and show that the dissipation effects of magnetic fields, which redshifts to a present value B 0 = 3 x 10 -9 G smoothed on the magnetic Jeans scale and below, can give rise to Thomson scattering optical depths τ? 0.1.
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Foregrounds in Wide-Field Redshifted 21 cm Power Spectra

Nithyanandan Thyagarajan, +66 more
TL;DR: In this article, the authors investigate the signatures of wide-field measurements and an all-sky foreground model using the delay spectrum technique that maps the measurements to foreground object locations through signal delays between antenna pairs.
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The low-frequency environment of the Murchison Widefield Array : radio-frequency interference analysis and mitigation

A. R. Offringa, +67 more
TL;DR: Offringa et al. as discussed by the authors studied the low-frequency environment of the Murchison Widefield Array (MWA) in terms of radio-frequency interference analysis and mitigation.
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The Murchison Widefield Array 21 cm Power Spectrum Analysis Methodology

Daniel C. Jacobs, +70 more
TL;DR: In this paper, the authors compare the outputs of multiple data calibration and reduction pipelines for the purpose of validating statistical limits cosmological hydrogen at redshifts between 6 and 12.