Table 4: Comparison of DIB strengths (in mÅ) toward SN2006X in M 100, the Galaxy and LMC. Upper limits for $\lambda \lambda$ 6379 and 6613 obtained from weight averaged spectra at phase -2 and +14. Equivalent widths for DIBs toward $\beta ^1$ Sco and $\rho$ Oph from Sollerman et al. (2005) and for Sk-69 223 from Cox et al. (2006). Taurus dark cloud toward HD 283809 from Adamson et al. (1991).
DIB SN2006X MW $\beta ^1$ Sco $\rho$ Oph Sk-69 223 HD 283809

E_B-V $\sim$ 1 1.0 0.22 0.32 0.35 1.6

6196 14 $\pm$ 4 53 20 10 10 46

6283 177 $\pm$ 25 900 390 111 225 312

6379 $\la$ 8 88 14 24 55 -

6613 $\la$ 18 210 40 43 19 -

**Table 4:** Comparison of DIB strengths (in mÅ) toward SN2006X in M 100, the Galaxy and LMC. Upper limits for $\lambda \lambda$ 6379 and 6613 obtained from weight averaged spectra at phase -2 and +14. Equivalent widths for DIBs toward $\beta ^1$ Sco and $\rho$ Oph from Sollerman et al. (2005) and for Sk-69 223 from Cox et al. (2006). Taurus dark cloud toward HD 283809 from Adamson et al. (1991).
DIB	SN2006X	MW	$\beta ^1$ Sco	$\rho$ Oph	Sk-69 223	HD 283809
E_B-V	$\sim$ 1	1.0	0.22	0.32	0.35	1.6
6196	14 $\pm$ 4	53	20	10	10	46
6283	177 $\pm$ 25	900	390	111	225	312
6379	$\la$ 8	88	14	24	55	-
6613	$\la$ 18	210	40	43	19	-

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