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Line intensity mapping (LIM) proposes to efficiently observe distant faint galaxies and map the matter density field at high redshift.
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N. Kaiser, Clustering in real space and in redshift space , MNRAS 227
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M. Tegmark, Measuring Cosmological Parameters with Galaxy Surveys , Phys. Rev. Lett. 79
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G. L. Bryan and M. L. Norman, Statistical Properties of X-Ray Clusters: Analytic and Numerical Comparisons , ApJ 495
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A. J. S. Hamilton, Linear Redshift Distortions: a Review , in The Evolving Universe , D. Hamilton, ed., vol. 231 of Astrophysics and Space Science Library , p. 185, 1998, DOI [ astro-ph/9708102 ]
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X. Yang, H. J. Mo and F. C. van den Bosch, Constraining galaxy formation and cosmology with the conditional luminosity function of galaxies , MNRAS 339
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U. Seljak, Extracting Primordial Non-Gaussianity without Cosmic Variance , Phys. Rev. Lett. 102
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A. Crites, J. Bock, M. Bradford, B. Bumble, T.-C. Chang, Y.-T. Cheng et al., Measuring the Epoch of Reionization using [CII] Intensity Mapping with TIME-Pilot , in American Astronomical Society Meeting Abstracts #229 , vol. 229 of American Astronomical Society Meeting Abstracts , p. 125.01, Jan., 2017
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E. Switzer, “Measuring the Cosmological Evolution of Gas and Galaxies with the EXperiment for Cryogenic Large-aperture Intensity Mapping (EXCLAIM).” NASA APRA Proposal, Jan., 2017
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M. White and N. Padmanabhan, Matched filtering with interferometric 21 cm experiments , MNRAS 471
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B. R. Dinda, A. A. Sen and T. R. Choudhury, Dark energy constraints from the 21 c
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