Table 1:

Irradiances in W m^-2.

Spectral lines	(nm)	PEVE	P	SN	S
He II (bl Si XI)	30.400	309	663	502	395
Si VIII	31.983	8.2	11.7	12.5	7.6
Fe XVI (bl Mg VIII)	33.530	2.7	2.0	1.8	1.2
Mg VIII (bl)	33.901	1.9	1.8	1.8	1.1
Si X (bl)	34.750	5.6	6.3	6.8	4.3
Si IX (bl)	34.987	5.1	5.6	5.9	3.7
Si X (bl)	35.601	3.3	4.0	3.7	2.3
Mg IX (bl Mg VII)	36.800	42.	39.4	41.5	28.3
He I	51.562	1.2	1.0	1.3	0.87
Si XII	52.066	0.67	0.82	0.93	0.70
He I (bl)	52.221	1.9	1.5	1.7	1.3
O III	52.600	2.6	2.2	2.3	1.9
He I (bl)	53.703	5.2	4.9	4.6	4.0
Ne IV	54.207	0.66	0.51	0.46	0.34
Ne IV (sbl)	54.400	1.1	0.84	0.74	0.52
O IV (sbl)	55.450	26.4	25.4	21.6	20.8
Ne VI (2) (bl)	56.280	2.3	2.1	1.9	1.5
Ne V (2)	56.982	0.80	0.62	0.61	0.44
Ne V (3)	57.233	1.2	1.1	1.1	0.81
C III (bl Ca X)	57.420	1.1	1.0	1.0	0.75
He I	58.400	48.	36.	33.	78.
Ar VII	58.575	0.89	0.60	0.55	1.3
O III	60.000	5.2	4.8	4.0	3.0
Mg X (bl O IV)	61.000	16.	14.3	11.5	9.6
Mg X (bl)	62.500	6.6	5.8	5.1	3.9
O V	63.000	56.	35.	33.	35.

Notes. PEVE are the irradiances from the prototype-EVE, Apr 14, 2008. P are the irradiances from the full-Sun NIS observation of Mar 17, 2008, obtained with the Del Zanna (2001) scaled responsivities and the present long-term corrections; SN are the NIS irradiances of the same observation obtained with the current standard CDS responsivities (version 4, 2002) and the present long-term corrections; S are the same NIS irradiances obtained with the current standard CDS responsivities (version 4, 2002) and the standard long-term corrections.