Non-Gaussianity from Large-Scale Structure Surveys

Table 3

Forecasted non-Gaussianity constraints: (A) [20] (B) [63] (C) [69, 70] (E) [57]) (F) e.g., [15].

	CMB Bispectrum		Halo bias
type NG	Planck	BPol	Euclid	LSST
	1−𝜎 errors
Local	3^(A)	2^(A)	1.5^(B)	0.7^(B)
Equilateral	25^(C)	14^(C)	—	—
Enfolded	𝒪10	𝒪10	39^(E)	18^(E)
	#𝜎 detection
GR	N/A	N/A	1^(E)	2^(E)
secondaries	3^(F)	5^(F)	N/A	N/A