Public repository of the Cosmic Linear Anisotropy Solving System (master for the most recent version of the standard code; GW_CLASS to include Cosmic Gravitational Wave Background anisotropies; classnet branch for acceleration with neutral networks; ExoCLASS branch for exotic energy injection; class_matter branch for FFTlog)
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Selection Function Normalization for HI Intensity Mapping #444
I'm Rahul Kothari, a postdoc at UWC, South Africa. First of all, I thank you very much for developing such a useful code. I wish to ask you a question related to the selection function normalization in the context of HI Intensity mapping.
Specifically, I wish to normalize the selection function wrt to mean HI temperature
\bar{T}(z) = .056 + 0.232z−0.024z^2 mK
i.e., to make
int \bar{T}(z) W(z,z_i) A dz = 1
where A is some constant and W is the tophat window function.
I would highly appreciate any help in this regard.
Dear Developers,
I'm Rahul Kothari, a postdoc at UWC, South Africa. First of all, I thank you very much for developing such a useful code. I wish to ask you a question related to the selection function normalization in the context of HI Intensity mapping.
Specifically, I wish to normalize the selection function wrt to mean HI temperature \bar{T}(z) = .056 + 0.232z−0.024z^2 mK
i.e., to make int \bar{T}(z) W(z,z_i) A dz = 1 where A is some constant and W is the tophat window function.
I would highly appreciate any help in this regard.