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Cross-correlation Forecast of CSST Spectroscopic Galaxy and MeerKAT Neutral Hydrogen Intensity Mapping Surveys
Cross-correlating the data on neutral hydrogen (H i ) 21 cm intensity mapping with galaxy surveys is an effective method to extract astrophysical and cosmological information. In this work, we investigate the cross-correlation of MeerKAT single-dish mode H i intensity mapping and China Space Station...
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Published in: | Research in astronomy and astrophysics 2023-07, Vol.23 (7), p.75003-36 |
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Main Authors: | , , , , , , , , |
Format: | Article |
Language: | English |
Subjects: | |
Citations: | Items that this one cites Items that cite this one |
Online Access: | Get full text |
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Summary: | Cross-correlating the data on neutral hydrogen (H
i
) 21 cm intensity mapping with galaxy surveys is an effective method to extract astrophysical and cosmological information. In this work, we investigate the cross-correlation of MeerKAT single-dish mode H
i
intensity mapping and China Space Station Telescope (CSST) spectroscopic galaxy surveys. We simulate a survey area of ∼300 deg
2
of MeerKAT and CSST surveys at
z
= 0.5 using Multi-Dark
N
-body simulation. The PCA algorithm is applied to remove the foregrounds of H
i
intensity mapping, and signal compensation is considered to solve the signal loss problem in H
i
-galaxy cross power spectrum caused by the foreground removal process. We find that from CSST galaxy auto and MeerKAT-CSST cross power spectra, the constraint accuracy of the parameter product Ω
H I
b
H I
r
H I,
g
can reach ∼1%, which is about one order of magnitude higher than the current results. After performing the full MeerKAT H
i
intensity mapping survey with 5000 deg
2
survey area, the accuracy can be enhanced to |
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ISSN: | 1674-4527 2397-6209 |
DOI: | 10.1088/1674-4527/accdc0 |