Table 3: Fluxes for the entire galaxy used to model the global ISRF. The values are corrected for Galactic extinction. ^a Israel (1988), ^b De Vaucouleurs et al. (1991).
Wavelength Flux density

(Å) (10^-14 erg s^-1 cm^-1 Å^-1)

1500 $(152\pm 48)^a$

1800 $(208\pm 25)^a$

2200 $(146\pm 25)^a$

2500 $(100\pm 18)^a$

3650 $(108\pm 10)^b$

4400 $(101\pm 9)^b$

5500 $(70\pm 6)^b$

**Table 3:** Fluxes for the entire galaxy used to model the global ISRF. The values are corrected for Galactic extinction. ^a Israel (1988), ^b De Vaucouleurs et al. (1991).
Wavelength	Flux density
(Å)	(10^-14 erg s^-1 cm^-1 Å^-1)
1500	$(152\pm 48)^a$
1800	$(208\pm 25)^a$
2200	$(146\pm 25)^a$
2500	$(100\pm 18)^a$
3650	$(108\pm 10)^b$
4400	$(101\pm 9)^b$
5500	$(70\pm 6)^b$

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