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We forecast ability of dedicated 21 cm intensity mapping experiments to constraint primordial non-Gaussianity using power spectrum and bispectrum.
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E. Sefusatti, M. Crocce, S. Pueblas and R. Scoccimarro, Cosmology and the bispectrum , Phys. Rev. D 74
2006
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Y. Wang, Dark Energy Constraints from Baryon Acoustic Oscillations , ApJ 647
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S. Matarrese and L. Verde, The Effect of Primordial Non-Gaussianity on Halo Bias , ApJ 677
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V. Desjacques, D. Jeong and F. Schmidt, Large-scale galaxy bias , Phys. Rep. 733
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