Abstract
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 Square
Kilometre Array 1 (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 moderate signal-to-noise ratio from wide-field
imaging (SNR ≲ 3), for which the statistical uncertainty is sample
variance dominated. We address the observational requirements on the
angular resolution, the field of view, and the thermal noise limit for a
successful measurement. To achieve a full scientific return from 21-cm
tomography and to exploit a synergy with 21-cm power spectra, we suggest
an observing strategy using wide-field imaging (several tens of square
degrees) by an interferometric mosaicking/multibeam observation with
additional intermediate baselines ( ∼ 2-4 km) in an SKA phase 2.
Original language | English |
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Pages (from-to) | 1936-1954 |
Number of pages | 19 |
Journal | Monthly Notices of the Royal Astronomical Society |
Volume | 471 |
Issue number | 2 |
DOIs | |
Publication status | Published - Oct-2017 |
Keywords
- radiative transfer
- methods: data analysis
- techniques: image processing
- intergalactic medium
- dark ages
- reionization
- first stars
- cosmology: theory
- NEUTRAL HYDROGEN
- HIGH-REDSHIFT
- SIMULATING COSMIC REIONIZATION
- DETECTING IONIZED BUBBLES
- 21 CENTIMETER TOMOGRAPHY
- POWER-SPECTRUM
- LARGE SCALES
- COSMOLOGICAL REIONIZATION
- HYDROGEN REIONIZATION
- INTERGALACTIC MEDIUM