**Table 4:** Photometry of (0-0) lines observed with ISOCAM.
Term	$\lambda$	F $\pm$ $\Delta F$ (10^-13 erg cm^-2 s^-1)
		C, L	B, M	A	E, K, J
	( $\mu$ m)	(135 arcsec²)	(207 arcsec²)	(155 arcsec²)	(173 arcsec²)
0-0S(2)	12.3	5.5 $\pm$ 0.2	5.5 $\pm$ 0.3	1.4 $\pm$ 0.2	5.9 $\pm$ 0.2
0-0S(3)	9.6	3.9 $\pm$ 0.3	6.1 $\pm$ 0.4	3.0 $\pm$ 0.3	7.0 $\pm$ 0.4
0-0S(4)	8.0	3.4 $\pm$ 0.3	4.3 $\pm$ 0.3	1.2 $\pm$ 0.3	3.6 $\pm$ 0.4
0-0S(5)	6.9	3.6 $\pm$ 0.3	6.5 $\pm$ 0.3	3.1 $\pm$ 0.3	7.7 $\pm$ 0.4
0-0S(6)	6.1	1.9 $\pm$ 0.3	3.9 $\pm$ 0.4	1.4 $\pm$ 0.3	3.5 $\pm$ 0.4
0-0S(7)	5.5	1.3 $\pm$ 0.4	2.2 $\pm$ 0.6	1.3 $\pm$ 0.4	3.3 $\pm$ 0.5

Note: Due to transient effects at low signal levels, the fluxes could be underestimated by a factor 1.3-1.6 (relative fluxes, excitation temperatures, and o/p ratios would remain unaffected).

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