**Table 3:** Parameter values of the fit of the mid-IR Luminosity Functions.
	Type-1			Type-2			All
	${\rm\alpha}$	$\!\beta$	$\! {\rm log}~L_{15}^{*}$	$\alpha$	$\beta$	${{\rm log} ~ L_{15}^*}$	$\alpha$	$\beta$	${{\rm log} ~ L_{15}^*}$
RMS^a	0.0	2.1	42.8	0.0	2.5	43.2	0.3	2.1	43.4
Xu03^{a, b}	-	-	-	-	-	-	0.3	1.7	43.4
Here (low-z)^c	1.3	2.8	44.8	0.9	2.7	44.1	-	-	-
Here (int-z)^{c, d}	0.7	2.8	45.4	0.0	2.7	44.6	-	-	-

^a Luminosities have been converted to 15 $~\mu$ m using the adopted SEDs. ^b From Xu et al. (2003).
^c Best fit solutions for type-1 (model "B'') and type-2 (Circinus SED, model "F'').
^d Intermediate redshift, z=0.6.

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