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Table 3

DIB equivalent widths.

DIB 23180 24398 203532 149757 185418 170740 147889 169454
(Å) (mÅ)
C2-DIBs

4363 a <0.3 4.3 ± 0.2 1.3 ± 0.4 <0.4 <0.2 11.1 ± 0.4 4.4 ± 0.2
4727a 46.7 ± 0.9 38.3 ± 0.7 55.3 ± 1.1 17.0 ± 1.0 35.8 ± 1.0 45.3 ± 1.0 155.4 ± 2.9 95.0 ± 1.1
4734 2.3 ± 0.8 <0.5 6.5 ± 0.7 <0.6 <4 <0.5 15.2 ± 0.9 3.2 ± 0.4
4963 12.0 ± 0.8 9.6 ± 0.3 21.2 ± 0.4 3.8 ± 0.6 11.6 ± 0.7 11.2 ± 0.3 51.9 ± 0.9 24.8 ± 1.0
4969 3.8 ± 0.3 2.5 ± 0.2 2.8 ± 0.2 1.4 ± 0.5 1.5 ± 0.3 2.2 ± 0.3 9.7 ± 0.8 6.4 ± 0.3
4979 3.0 ± 0.3 2.5 ± 0.3 3.6 ± 0.3 1.3 ± 0.4 1.9 ± 0.3 2.0 ± 0.3 14.1 ± 0.9 3.9 ± 0.3
4984 6.6 ± 0.3 3.6 ± 0.3 8.2 ± 0.4 2.4 ± 0.5 4.0 ± 0.3 3.6 ± 0.2 24.4 ± 1.1 11.2 ± 0.3
5003 a a 4.1 ± 0.2 2.6 ± 0.5 a a 5.6 ± 0.5 a
5170 4.5 ± 0.4 1.6 ± 0.2 3.2 ± 0.5 1.3 ± 0.5 1.9 ± 0.3 1.9 ± 0.3 11.1 ± 0.8 5.3 ± 0.2
5175 2.3 ± 0.2 13.5 ± 0.4 7.9 ± 0.3 2.8 ± 0.8 2.3 ± 0.5 6.2 ± 0.5 31.7 ± 1.0 16.1 ± 0.8
5418 10.3 ± 0.4 5.1 ± 0.3 12.3 ± 0.3 3.7 ± 0.4 5.4 ± 0.4 5.1 ± 0.3 40.8 ± 0.9 16.4 ± 0.3
5512 7.5 ± 0.3 5.0 ± 0.2 10.6 ± 0.3 2.2 ± 0.4 3.8 ± 0.4 4.5 ± 0.3 18.2 ± 0.5 14.6 ± 0.3
5541 4.5 ± 0.3 2.1 ± 0.2 4.7 ± 0.2 1.4 ± 0.3 3.3 ± 0.3 1.7 ± 0.2 10.9 ± 0.8 9.3 ± 0.3
5546 4.0 ± 0.4 2.0 ± 0.3 4.7 ± 0.3 1.5 ± 0.4 1.9 ± 0.3 1.7 ± 0.1 8.2 ± 0.8 5.7 ± 0.3
5762 4.6 ± 0.3 2.7 ± 0.2 4.1 ± 0.3 2.8 ± 0.5 7.2 ± 0.5 2.3 ± 0.3 11.6 ± 1.0 8.1 ± 0.3
5769 4.8 ± 0.4 1.5 ± 0.3 5.2 ± 0.3 <2 <4.5 1.2 ± 0.2 20.6 ± 0.8 5.4 ± 0.3
5793b 6.3 ± 0.7 5.3 ± 0.6 5.3 ± 0.4 1.7 ± 0.4 3.9 ± 0.5 3.3 ± 0.4 15.8 ± 1.0 8.7 ± 0.3
6729 4.2 ± 0.6 5.1 ± 1.5 3.5 ± 0.7 <5 <4 <4 15.5 ± 1.5 6.6 ± 1

New C2-DIB candidates

4737.5 0.8 ± 0.3 <0.4 1.2 ± 0.2 <0.5 <0.5 blenda 3.0 ± 0.7 0.5 ± 0.2
5547.4 0.7 ± 0.2 0.9 ± 0.2 0.8 ± 0.1 <0.7 1.3 ± 0.2 0.9 ± 0.1 2.5 ± 0.6 2.0 ± 0.3
5769.8 1.0 ± 0.2 0.7 ± 0.2 0.7 ± 0.2 <1.3 <1.5 0.7 ± 0.1 1.9 ± 0.7 1.8 ± 0.2

Selected strong DIBs

5850 31.1 ± 0.6 20.4 ± 0.7 28.0 ± 0.3 10.9 ± 0.6 27.6 ± 0.6 21.0 ± 0.4 64.6 ± 1.0 61.0 ± 0.7
5797 58.6 ± 1.0 51.4 ± 0.6 53.1 ± 1.1 28.3 ± 0.9 80.3 ± 1.2 61.2 ± 0.9 143.5 ± 2.5 158.4 ± 2.3
5780 80.0 ± 0.9 97.2 ± 0.8 108.6 ± 0.9 65.6 ± 1.3 266.1 ± 1.8 237.0 ± 1.6 346.9 ± 2.9 463.9 ± 2.2
6196 12.6 ± 0.6 13.6 ± 0.7 12.7 ± 0.6 8.5 ± 0.7 33.7 ± 2.1 23.7 ± 0.9 34.8 ± 1.6 52.4 ± 0.6
6234 5.9 ± 0.7 5.9 ± 0.5 4.7 ± 0.3 2.2 ± 1.0 9.1 ± 0.7 11.6 ± 0.4 14.4 ± 1.4 15.1 ± 1.2
6376 7.8 ± 0.6 7.7 ± 0.6 7.7 ± 0.7 5.0 ± 0.7 17.3 ± 1.2 10.4 ± 0.9 34.1 ± 2.4 20.0 ± 1.5
6379 37.6 ± 0.6 57.4 ± 0.7 43.2 ± 0.4 15.2 ± 0.7 71.5 ± 0.7 55.6 ± 0.7 82.4 ± 1.8 93.3 ± 1.4
6614 45.3 ± 0.7 60.2 ± 0.6 57.7 ± 0.6 41.4 ± 1.0 166.3 ± 0.9 120.0 ± 0.6 160.6 ± 2.1 182.6 ± 1.1

Notes. (a) blended with stellar lines, (b)possible telluric residuals.

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