KiDS+VIKING+GAMA: Halo occupation distributions and correlations of satellite numbers with a new halo model of the galaxy-matter bispectrum for galaxy-galaxy-galaxy lensing

Open Access

Table C.3.

best fit values for halo model parameters for stellar-mass-selected lenses in KV450 × GAMA for each stellar mass sample a.

		From correlation	From correlation	From correlation	From correlation	From correlation
		with m1	with m2	with m3	with m4	with m5
a = m1	α^a
	σ^a
	[10¹¹M_⊙]
	β^a
	M^′a[10¹³ M_⊙]
	f^a

a = m2	α^a
	σ^a
	[10¹¹M_⊙]
	β^a
	M^′a[10¹³ M_⊙]
	f^a

a = m3	α^a
	σ^a
	[10¹¹M_⊙]
	β^a
	M^′a[10¹³ M_⊙]
	f^a

a = m4	α^a
	σ^a
	[10¹¹M_⊙]
	β^a
	M^′a[10¹³ M_⊙]
	f^a

a = m5	α^a
	σ^a
	[10¹¹M_⊙]
	β^a
	M^′a[10¹³ M_⊙]
	f^a

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