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Table A.1

Characterisation of the detected DIBs and new DIB candidates.

DIB Ref. Lab frame HD 183143 HD 165784 HD 92207 HD 111613




λ0,air λvac EW Ac FWHM λvac EW Ac FWHM λvac EW Ac FWHM λvac EW Ac FWHM
(Å) (Å) (mÅ) (%) (Å) (Å) (mÅ) (%) (Å) (Å) (mÅ) (%) (Å) (Å) (mÅ) (%) (Å)
9632a 2 9632.6 ± 0.8 9634.6 316 ± 99 12.0 ± 11.6 2.7 9635.8 77 ± 14 3.9 ± 2.1 2.5
9880 5 9880.4 ± 0.1 9883.1 44 ± 6 2.9 ± 0.9 1.3 9883.2 21 ± 3 1.2 ± 0.3 1.4
10125 6 10125.1 ± 1.1 10128.6 9 ± 3 1.0 ± 0.7 0.6 10127.2 3 ± 2 0.5 ± 0.6 0.6
10262 6 10262.5 ± 0.2 10265.4 9 ± 3 1.1 ± 0.5 0.8 10265.3 5 ± 3 0.6 ± 0.5 1.2
10361 4 10361.0 ± 0.1 10363.6 30 ± 3 1.9 ± 0.4 1.3 10363.9 24 ± 5 1.1 ± 0.6 1.9
10393 4 10392.5 ± 1.5 10395.9 17 ± 4 1.8 ± 0.8 1.0 10393.7 18 ± 7 1.3 ± 1.2 1.6 10396.3 18 ± 5 0.5 ± 0.7 1.5
10438 4 10438.4 ± 0.1 10441.2 64 ± 4 1.7 ± 0.4 3.7 10441.3 32 ± 4 0.9 ± 0.4 3.3
10504b.c 4 10504.3 ± 0.2 10507.2 50 ± 4 4.1 ± 0.8 1.1 10507.2 28 ± 3 2.2 ± 0.4 I.I
10507e 4 10507.6 ± 0.7 10509.8 41 ± 10 3.4 ± 0.4 1.2 10511.0 11 ± 2 1.0 ± 0.4 1.1
10697 4 10696.8 ± 0.4 10700.0 186 ± 7 4.6 ± 0.8 4.0 10699.5 133 ± 4 3.7 ± 0.5 3.9 10699.4 94 ± 8 2.0 ± 0.6 4.0 10700.1 91 ± 6 2.1 ± 0.7 4.4
10735 6 10734.7 ± 0.5 10737.9 20 ± 2 1.9 ± 0.4 1.2 10737.4 13 ± 2 1.0 ± 0.4 1.2
10780 3 10780.4 ± 0.2 10783.4 154 ± 6 10.4 ± 0.8 1.3 10783.3 108 ± 5 6.5 ± 0.5 1.5 10783.5 62 ± 6 2.7 ± 0.7 1.8 10783.3 83 ± 6 4.5 ± 0.6 1.7
10792 3 10791.9 ± 0.1 10794.8 39 ± 4 1.7 ± 0.5 2.0 10795.0 48 ± 5 1.3 ± 0.6 3.3 10794.7 39 ± 5 1.4 ± 0.6 2.2
10884 6 10884.2 ± 0.3 10887.5 38 ± 2 1.8 ± 0.3 2.0 10887.3 28 ± 2 2.0 ± 0.4 1.4 10886.9 11 ± 4 0.7 ± 0.5 2.0 10887.3 22 ± 7 1.1 ± 0.7 2.1
11048d 6 11048.3 ± 0.4 11051.5 39 ± 4 1.7 ± 0.6 2.6 11051.7 13 ± 4 0.6 ± 0.5 2.2 11051.1 19 ± 4 0.9 ± 0.5 1.5 11050.9 16 ± 3 0.9 ± 0.4 1.5
11695 6 11695.2 ± 0.2 11698.4 32 ± 11 2.1 ± 1.8 1.7 11698.4 9 ± 2 1.3 ± 0.3 0.8
11699 6 11698.7 ± 0.3 11702.0 35 ± 12 1.8 ± 1.8 2.1 11702.0 28 ± 5 1.2 ± 0.7 2.4 11701.5 19 ± 4 1.1 ± 0.5 1.6
11721 6 11720.5 ± 0.3 11723.9 46 ± 3 2.2 ± 0.4 2.5 11723.5 39 ± 3 1.7 ± 0.4 2.3 11724.0 28 ± 4 1.0 ± 0.5 3.3 11723.6 22 ± 4 0.9 ± 0.5 2.5
11792 6 11792.7 ± 0.1 11795.8 17 ± 2 1.5 ± 0.3 1.1 11795.9 10 ± 2 0.9 ± 0.3 1.4 11796.1 9 ± 4 0.6 ± 0.6 1.4
11797e 1 11797.3 ± 0.2 11800.6 133 ± 3 8.5 ± 0.3 1.5 11800.5 116 ± 3 5.3 ± 0.3 1.7 11800.6 59 ± 5 2.7 ± 0.5 2.2 11800.4 115 ± 4 5.3 ± 0.4 1.8
11970f 6 11970.1 ± 0.2 11973.5 105 ± 3 5.6 ± 0.3 1.4 11973.3 105 ± 4 4.3 ± 0.3 1.6 11973.5 66 ± 3 2.2 ± 0.4 2.2 11973.3 84 ± 4 3.8 ± 0.5 2.0
12222 6 12222.4 ± 0.2 12225.8 45 ± 2 2.6 ± 0.3 1.5 12225.7 28 ± 3 1.7 ± 0.4 1.6
12293 5 12293.9 ± 0.1 12297.2 24 ± 2 1.4 ± 0.3 1.7 12297.3 12 ± 3 0.9 ± 0.4 1.5
12518 5 12519.4 ± 0.1 12522.6 16 ± 2 0.8 ± 0.3 2.0 12523.0 30 ± 4 0.5 ± 0.3 3.8
12623 5 12623.6 ± 0.2 12626.8 105 ± 3 3.1 ± 0.3 3.4 12627.3 56 ± 2 1.3 ± 0.2 3.7
12799 5 12799.3 ± 0.4 12802.5 50 ± 4 3.4 ± 0.5 1.5 12802.5 18 ± 3 1.5 ± 0.5 1.3 12803.4 21 ± 5 1.2 ± 0.6 2.1 12802.6 33 ± 3 1.5 ± 0.3 2.2
12838 6 12837.6 ± 0.9 12840.4 72 ± 3 1.4 ± 0.3 4.6 12840.7 35 ± 6 0.9 ± 0.6 3.7 12842.5 28 ± 3 0.6 ± 0.3 5.8 12840.6 23 ± 4 0.8 ± 0.5 2.5
13027 4 13027.0 ± 0.7 13031.0 134 ± 3 1.9 ± 0.2 4.7 13030.2 48 ± 6 1.2 ± 0.4 5.6
13175 1 13175.1 ± 0.1 13178.5 647 ± 20 13.7 ± 0.2 4.1 13178.9 466 ± 21 9.0 ± 0.5 4.2

References. (1) Joblin et al. (1990); (2) Foing & Ehrenfreund (1994); (3) Groh et al. (2007); (4) Cox et al. (2014); (5) Hamano et al. (2015); (6) This work

Notes. All wavelengths are measured in the barycentric rest frame. The rest wavelengths are given in Col. 3 with a statistical error. Rest wavelengths have a systematic error of ± 0.3 A due to the double K I components (see Section 5). Non-detection of DIBs are a result either of a strength too low for detection or of missing spectral coverage. Stellar blends:(a) Mg II, λair = 9631.891, 9632.430Å(b) Fen, λair = 10501.504Å(c) N I, λair=10506.997 He I, λair = 11044.983 Å(e) Cl, λair= 11801.098Å (f) He I, λair = 11969.060, 11969.464Å.

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