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

311 citations · 2.2k across the 66 of their papers we have counts for

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Showing 2021Show all

8 papers · 1 filter

astro-ph.IM2021★ 12 cited

Degree-Scale Galactic Radio Emission at 122 MHz around the North Celestial Pole with LOFAR-AARTFAAC

B. K. Gehlot, L. V. E. Koopmans, A. R. Offringa +11

Aims: Contamination from bright diffuse Galactic thermal and non-thermal radio emission poses crucial challenges in experiments aiming to measure the 21-cm signal of neutral hydrog…

astro-ph.CO2021★ 30 cited

A numerical study of 21-cm signal suppression and noise increase in direction-dependent calibration of LOFAR data

M. Mevius, F. Mertens, L. V. E. Koopmans +14

We investigate systematic effects in direction dependent gain calibration in the context of the Low-Frequency Array (LOFAR) 21-cm Epoch of Reionization (EoR) experiment. The LOFAR…

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★ 10 cited

Astrophysical information from the Rayleigh-Jeans Tail of the CMB

Raghunath Ghara, Garrelt Mellema, Saleem Zaroubi

One of the explanations for the recent EDGES-LOW band 21-cm measurements of a strong absorption signal around 80~MHz is the presence of an excess radio background to the Cosmic Mic…

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★ 60 cited

Constraining the state of the intergalactic medium during the Epoch of Reionization using MWA 21-cm signal observations

Raghunath Ghara, Sambit K. Giri, Benedetta Ciardi +2

The Murchison Widefield Array (MWA) team has derived new upper limits on the spherically averaged power spectrum of the 21-cm signal at six redshifts in the range $z \approx 6.5-8.…

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.CO2021★ 34 cited

Prospects of constraining reionization model parameters using Minkowski tensors and Betti numbers

Akanksha Kapahtia, Pravabati Chingangbam, Raghunath Ghara +2

We explore the possibility of constraining model parameters of the Epoch of Reionization (EoR) from 21cm brightness temperature maps, using a combination of morphological descripto…