Table 1: Number of counterparts of our SiO targets.
   2MASS DENIS ISOGAL MSX IRAS

   all sky data release bulge PSC PSC 1.0 PSC 1.2 PSC 2.0

   (Cutri et al. 2003) (Simon 2003) (Schuller et al. 2003) (Egan et al. 1999) (Beichman et al. 1988)

J H $K_{\rm S}$ I J $K_{\rm S}$

ISO    (253) 252 252 252 53 217 253 253 191 43

MSX  (188) 187 187 187 42 149 188 14 188 122

Total  (441) $^{\rm + }$ 439 $^{\rm ++ }$ 439 439 95 $^{{\rm *}}$ 366 $^{\rm **}$ 441 267 379 165

**Table 1:** Number of counterparts of our SiO targets.
	2MASS	DENIS	ISOGAL	MSX	IRAS
	all sky data release	bulge PSC	PSC 1.0	PSC 1.2	PSC 2.0
	(Cutri et al. 2003)	(Simon 2003)	(Schuller et al. 2003)	(Egan et al. 1999)	(Beichman et al. 1988)
	J	H	$K_{\rm S}$	I	J	$K_{\rm S}$
ISO (253)	252	252	252	53	217	253	253	191	43
MSX (188)	187	187	187	42	149	188	14	188	122
Total (441)	$^{\rm + }$ 439	$^{\rm ++ }$ 439	439	95	$^{{\rm *}}$ 366	$^{\rm **}$ 441	267	379	165

: $^{\rm + }$ 72 are upper limits. $^{{\rm *}}$ 16 have magnitudes above saturation limits.
: $^{\rm ++ }$ 13 are upper limits. $^{\rm **}$ 104 have magnitudes above saturation limits.

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