Présidents de session
Contributed Talks 2: MeerKLASS & SKA
- Stefano Camera (University of Turin)
- Matilde Barberi Squarotti (Università degli Studi di Milano)
- Wenkai Hu (University of the Western Cape)
In this talk, I shall review the prospects for neutral hydrogen (HI) intensity mapping with the SKA Observatory (SKAO). HI intensity mapping will be highly complementary to traditional cosmological probes such as galaxy clustering and weak lensing, allowing us to test the foundations of our concordance cosmological model - an especially timely endeavour, in the view of the newest results but...
Neutral hydrogen (HI) intensity mapping is emerging as a revolutionary probe of the Large Scale Structure of the Universe and the MeerKLASS collaboration (MeerKAT Large Area Synoptic Survey) is currently running precursor analyses aiming to test the single-dish technique for mapping the cosmological 21cm signal using MeerKAT data. This signal, originating from the line emission at 1420MHz of...
HI intensity mapping is a promising technique for overcoming telescope sensitivity limits by capturing the large-scale distribution of HI, which is essential for studying the large-scale structures. Significant progress has been made in detecting the HI cross-correlation power spectrum using intensity mapping survey utilizing MeerKAT’s L-band receiver, and there is a good prospect of detecting...
