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Table 1

Polarization parameters of standard stars monitored by RoboPol, as reported in the literature.

Source RA Dec Band PD (%) EVPA (°) References
polarized
BD+57.2615 22:47:49.6 +58:08:50 R 2.02 ± 0.05 41.0 ± 1.0 Whittet et al. (1992)
BD+59.389(c) 02:02:42.1 +60:15:26 R 6.430 ± 0.022 98.14 ± 0.10 Schmidt et al. (1992)
BD+64.106 00:57:36.7 +64:51:35 R 5.150 ± 0.098 96.74± 0.54 Schmidt et al. (1992)
CMaR1 24 07:04:47.4 −10:56:18 R 3.18 ± 0.09 86.0±1.0 Whittet et al. (1992)
CygOB2 14 20:32:16.6 +41:25:36 R 3.13 ± 0.05 86.0±1.0 Whittet et al. (1992)
16:21:57.7 −24:29:44 R 1.59 ± 0.03 174.0 ± 1.0(*) Whittet et al. (1992)
–″– –″– R 1.81 176.0 Carrasco et al. (1973)
HD147343 16:22:19.9 −24:21:48 R 0.43 ± 0.05 151.0 ± 3.0 Whittet et al. (1992)
HD150193 16:40:17.9 −23:53:45 R 5.19 ± 0.05 56.0±1.0 Whittet et al. (1992)
17:05:32.3 −00:53:31 R 3.683 ± 0.072 88.91 ± 0.56 Schmidt et al. (1992)
–″– −″− R 3.63 ± 0.01 90.0 ± 0.1(*) Hsu & Breger (1982)
HD155197(c) 17:10:15.8 −04:50:04 R 4.274 ± 0.027 102.88 ± 0.18 Schmidt et al. (1992)
HD161056 17:43:47.0 −07:04:47 R 4.012 ± 0.032 67.33 ± 0.23 Schmidt et al. (1992)
19:27:26.6 +18:17:45 R 5.90 ± 0.05 179.2 ± 0.2(*) Hsu & Breger (1982)
—″— −″− R 5.7 ± 0.04 178.0±1.0 Bailey & Hough (1982)
21:28:57.8 +58:44:23 R 4.893 ± 0.029 59.10 ± 0.17(*) Schmidt et al. (1992)
—″— −″− R 4.86 ± 0.05 60.0±1.0 Bailey & Hough (1982)
−″− −″− R 4.99 ± 0.05 59.9 ± 0.1 Hsu & Breger (1982)
HD215806 22:46:40.2 +58:17:44 R 1.83 ± 0.04 66.0±1.0 Whittet et al. (1992)
HD236633 01:09:12.3 +60:37:41 R 5.376 ± 0.028 93.04 ± 0.15 Schmidt et al. (1992)
Hiltner960(a) 20:23:28.5 +39:20:59 R 5.210 ± 0.029 54.54 ± 0.16 Schmidt et al. (1992)
20:32:41.0 +41:14:29 R 7.97 ± 0.05 117.0 ± 1.0 Whittet et al. (1992)
—″— −″− R 7.893 ± 0.037 116.23 ± 0.14(*) Schmidt et al. (1992)
—″— −″− R 7.18 ± 0.04 117.0 ± 1.0 Hsu & Breger (1982)

unpolarized
BD+28.4211 21:51:11.0 +28:51:50 V 0.054 ± 0.027 54.22 Schmidt et al. (1992)
BD+32.3739(c) 20:12:02.1 +32:47:44 V 0.025 ± 0.017 35.79 Schmidt et al. (1992)
BD+33.2642 15:51:59.9 +32:56:54 R 0.20 ± 0.15 78 ± 20 Skalidis et al. (2018)
BD+40.2704 13:54:07.2 +39:37:59 ? 0.07 ± 0.02 57 ± 9 Berdyugin & Teerikorpi (2002)
G191B2B 05:05:30.6 +52:49:52 V 0.061 ± 0.038 147.65 Schmidt et al. (1992)
HD14069 02:16:45.2 +07:41:11 V 0.022 ± 0.019 156.57 Schmidt et al. (1992)
HD154892 17:07:41.3 +15:12:38 B 0.05 ± 0.03 Turnshek et al. (1990)
HD212311(c) 22:21:58.6 +56:31:53 V 0.034 ± 0.021 50.99 Schmidt et al. (1992)
HD21447 03:30:00.2 +55:27:07 V 0.051 ± 0.020 171.49 Schmidt et al. (1992)
HD94851 10:56:44.3 —20:39:53 B 0.057 ± 0.018 Turnshek et al. (1990)
WD2149+021 21:52:25.4 +02:23:20 R 0.050 ± 0.006 −63 ± 3 Cikota et al. (2017)

Notes. (a)Possibly variable You et al. (2017); (b)variable in RoboPol data and/or in Hsu & Breger (1982); Dolan & Tapia (1986); (c)possibly variable Breus et al. (2021). For stars with multiple literature values, (*)flags the value used for the EVPA zero point calibration in Sect. 3.1.

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