The H i intensity mapping bispectrum including observational effects
The H i intensity mapping bispectrum including observational effects
复制标题
H i 强度映射双谱,包括观察效应
DOI:
10.1093/mnras/stab2200
复制
发表时间:
2021
影响因子:
4.8
通讯作者:
Cunnington S
中科院分区:
文献类型:
--
作者:
Cunnington S
The bispectrum is a three-point statistic with the potential to provide additional information beyond power spectra analyses of survey data sets. Radio telescopes that broadly survey the 21-cm emission from neutral hydrogen (Hi) are a promising way to probe LSS and in this work we present an investigation into the Hiintensity mapping (IM) bispectrum using simulations. We present a model of the redshift space HiIM bispectrum including observational effects from the radio telescope beam and 21-cm foreground contamination. We validate our modelling prescriptions with measurements from robust IM simulations, inclusive of these observational effects. Our foreground simulations include polarization leakage, on which we use a principal component analysis cleaning method. We also investigate the effects from a non-Gaussian beam including side-lobes. For a MeerKAT-like single-dish IM survey atz= 0.39, we find that foreground removal causes anreduction in the equilateral bispectrum’s signal-to-noise ratio, whereas the beam reduces it by. We find our models perform well, generally providing, indicating a good fit to the data. Whilst our focus is on post-reionization, single-dish IM, our modelling of observational effects, especially foreground removal, can also be relevant to interferometers and reionization studies.