The slippery slope of dust attenuation curves - Correlation of dust attenuation laws with star-to-dust compactness up to z = 4

Open Access

Table 4.

Summary of the results of the best fits using the same SED method on the fluctuated photometry preferring the same attenuation law (average of ten realizations) and the best attenuation laws for the real galaxies.

	Mock
Real	C00	CF00	LF17
C00	94%	5%	1%
CF00	0%	97%	3%
LF17	0%	3%	97%

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