We introduce a novel technique, called “granulometry", to characterize and recover the mean size and the size distribution of H II regions from 21-cm tomography. The technique is easy to implement, but places the previously not very well defined concept of morphology on a firm mathematical foundation. The size distribution of the cold spots in 21-cm tomography can be used as a direct tracer of the underlying probability distribution of H II region sizes. We explore the capability of the method using large-scale reionization simulations and mock observational data cubes while considering capabilities of SKA1-low and a future extension to SKA2. We show that the technique allows the recovery of the H II region size distribution with a mod...
abstract: One of the most fundamental questions in astronomy is how the Universe evolved to become t...
© 2019 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Societ...
Masters of ScienceUpcoming and ongoing 21cm surveys, such as the Square Kilometre Array (SKA), Hydro...
We introduce a novel technique, called ‘granulometry’, to characterize and recover the mean size an...
The upcoming SKA1-Low radio interferometer will be sensitive enough to produce tomographic imaging d...
The 21-cm power spectrum (PS) has been shown to be a powerful discriminant of reionization and cosmi...
The formation of the first luminous sources in the Universe, such as the first generation of stars a...
Detecting the 21-cm hyperfine transition from neutral hydrogen in the intergalactic medium is our be...
Observations of the epoch of reionization (EoR) using the 21-cm hyperfine emission of neutral hydrog...
High-redshift 21-cm observations will provide crucial insights into the physical processes of the Ep...
Intensity mapping of the 21 cm signal of neutral hydrogen will yield exciting insights into the Epoc...
Measurements of the one-point probability distribution function and higher-order moments (variance, ...
abstract: One of the most fundamental questions in astronomy is how the Universe evolved to become t...
© 2019 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Societ...
Masters of ScienceUpcoming and ongoing 21cm surveys, such as the Square Kilometre Array (SKA), Hydro...
We introduce a novel technique, called ‘granulometry’, to characterize and recover the mean size an...
The upcoming SKA1-Low radio interferometer will be sensitive enough to produce tomographic imaging d...
The 21-cm power spectrum (PS) has been shown to be a powerful discriminant of reionization and cosmi...
The formation of the first luminous sources in the Universe, such as the first generation of stars a...
Detecting the 21-cm hyperfine transition from neutral hydrogen in the intergalactic medium is our be...
Observations of the epoch of reionization (EoR) using the 21-cm hyperfine emission of neutral hydrog...
High-redshift 21-cm observations will provide crucial insights into the physical processes of the Ep...
Intensity mapping of the 21 cm signal of neutral hydrogen will yield exciting insights into the Epoc...
Measurements of the one-point probability distribution function and higher-order moments (variance, ...
abstract: One of the most fundamental questions in astronomy is how the Universe evolved to become t...
© 2019 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Societ...
Masters of ScienceUpcoming and ongoing 21cm surveys, such as the Square Kilometre Array (SKA), Hydro...