The cosmological evolution of baryons through recombination and reionization are predicted to manifest as faint spectral features in the cosmic radio background. Pathfinder experiments that aim to detect global phase transitions in the ionization state of the gas in redshifted 21-cm may well be the first radio wavelength constraints on the astrophysics that drive the thermal evolution during reionization and the timing of critical events as first stars and galaxies form. This challenging problem is a motivation for innovative design in radio astronomy receivers. We present progress at the Raman Research Institute in the system design of precision radiometers for detecting spectral deviations in the radio background, design and test measurem...
This thesis presents instrumentation with which to measure the abundance of neutral hydrogen gas in ...
The Epoch of Reionization (EoR) is the transitional period in the universe's evolution which starts ...
We explore the possibility of detecting hydrogen radio recombination lines from 0 < z < 10 qua...
Cosmic evolution in the hydrogen content of the Universe through recombination and up to the end of ...
The challenging goal of detecting faint and wideband spectral features arising from cosmological evo...
Emission and absorption features in the spectrum of the diffuse radio background below 200 MHz due t...
Photons emitted during cosmological hydrogen (500 ≲ z ≲ 1600) and helium recombination (...
In spite of the great recent results from the Planck satellite supporting cosmological reionization ...
Observations of the 21-cm line from primordial hydrogen promise to be one of the best tools to study...
The reionization of the Universe is expected to have left a signal in the form of a sharp step in th...
The global 21-cm signal from Cosmic Dawn (CD) and the Epoch of Reionization (EoR), at redshifts , pr...
The observation of space-time variations in fundamental constants would provide strong evidence for ...
International audienceCosmological and astrophysical surveys in various wavebands, in particular fro...
The epoch of reionization (EoR) corresponds to a 'cosmic phase transition', when the neutral interga...
Long-wavelength spectral distortions in the cosmic microwave background arising from the 21 cm trans...
This thesis presents instrumentation with which to measure the abundance of neutral hydrogen gas in ...
The Epoch of Reionization (EoR) is the transitional period in the universe's evolution which starts ...
We explore the possibility of detecting hydrogen radio recombination lines from 0 < z < 10 qua...
Cosmic evolution in the hydrogen content of the Universe through recombination and up to the end of ...
The challenging goal of detecting faint and wideband spectral features arising from cosmological evo...
Emission and absorption features in the spectrum of the diffuse radio background below 200 MHz due t...
Photons emitted during cosmological hydrogen (500 ≲ z ≲ 1600) and helium recombination (...
In spite of the great recent results from the Planck satellite supporting cosmological reionization ...
Observations of the 21-cm line from primordial hydrogen promise to be one of the best tools to study...
The reionization of the Universe is expected to have left a signal in the form of a sharp step in th...
The global 21-cm signal from Cosmic Dawn (CD) and the Epoch of Reionization (EoR), at redshifts , pr...
The observation of space-time variations in fundamental constants would provide strong evidence for ...
International audienceCosmological and astrophysical surveys in various wavebands, in particular fro...
The epoch of reionization (EoR) corresponds to a 'cosmic phase transition', when the neutral interga...
Long-wavelength spectral distortions in the cosmic microwave background arising from the 21 cm trans...
This thesis presents instrumentation with which to measure the abundance of neutral hydrogen gas in ...
The Epoch of Reionization (EoR) is the transitional period in the universe's evolution which starts ...
We explore the possibility of detecting hydrogen radio recombination lines from 0 < z < 10 qua...