摘要: 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 deg2 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 H IbH IrH 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 deg2 survey area, the accuracy can be enhanced to
can be a powerful tool to probe the cosmic H I property and the evolution of galaxies and the Universe.
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