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Table A.3

Previously published Serkowski parameters for sightlines in common with LIPS.

Best-fit parameters
STAR Reference Instrument K λ max (nm) P max (%)

HD 37903 (This work) HPOL 0.73 ± 0.11 657 ± 10 1.95 ± 0.01
Efimov (2009) 1.35 680 2.00
This work FORS2 1.51 ± 0.23 646 ± 8 1.82 ± 0.01
HD 38087 (This work) HPOL 1.25 ± 0.21 585 ± 12 2.79 ± 0.02
This work FORS2 1.18 ± 0.04 572 ± 5 2.59 ± 0.01
HD 43384 Wilking et al. (1980) FORS2 0.97 ± 0.04 560 ± 10 3.00 ± 0.04
This work FORS2 0.92 ± 0.03 566 ± 2 3.06 ± 0.01
Walker 67 Wilking et al. (1980) 1.39 ± 0.09 810 ± 2 5.31 ± 0.06
This work FORS2 1.40 ± 0.05 826 ± 3 5.20 ± 0.04
HD 108639 Heiles (2000) 0.87 ± 0.13 520 ± 10 1.91 ± 0.02
This work FORS2 1.29 ± 0.23 550 ± 5 1.92 ± 0.04
HD 147888 Wilking et al. (1982) 1.29 ± 0.05 720 ± 10 3.75 ± 0.07
Martin et al. (1992) 1.28 ± 0.04 700 ± 10 3.63 ± 0.04
(This work) HPOL 1.51 ± 0.04 672 ± 20 3.53 ± 0.01
This work FORS2 1.43 ± 0.02 662 ± 4 3.49 ± 0.01
HD 147889 Wilking et al. (1980) 1.32 ± 0.05 800 ± 10 4.09 ± 0.07
Martin et al. (1992) 1.25 ± 0.03 780 ± 10 4.02 ± 0.04
This work FORS2 (2015-05-13) 1.32 ± 0.02 809 ± 4 4.22 ± 0.01
This work FORS2 (2015-05-25) 1.37 ± 0.04 798 ± 7 4.18 ± 0.01
This work FORS2 (2016-01-28) 1.18 ± 0.09 815 ± 13 4.18 ± 0.01
HD 161056 Wilking et al. (1980) 0.96 ± 0.09 560 ± 2 3.8 ± 0.1
(This work) HPOL 1.3 ± 0.02 578 ± 1 4.08 ± 0.01
This work FORS2 1.43 ± 0.05 572 ± 2 4.02 ± 0.04
HD 164740 Wilking et al. (1982) 1.24 ± 0.12 670 ± 20 7.75 ± 0.15
Martin et al. (1992) 1.24 ± 0.07 670 ± 10 7.45 ± 0.14
This work FORS2 1.72 ± 0.02 657 ± 2 7.20 ± 0.02
HD 210121 Larson (1999) 0.66 ± 0.09 380 ± 30 1.32 ± 0.04
(This work) HPOL 0.65 ± 0.15 402 ± 50 1.37 ± 0.06
This work FORS2 0.55 ± 0.12 434 ± 21 1.38 ± 0.02
HD 251204 (This work) HPOL 1.25 ± 0.11 584 ± 7 4.95 ± 0.03
This work FORS2 1.00 ± 0.02 575 ± 2 5.00 ± 0.01

Notes. Wilking et al. (1980) and Martin et al. (1992) report updated Serkowski parameters from compilations of broad-band polarimetric data. The best-fit parameters from HPOL were obtained in this work using data made available at the Mikulski Archive for Space Telescopes (MAST).

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