Table 1.

Properties of high polarization standard stars.

StandardRADec.Plx.SpTBV|$E_{(B-V)}$||$R_{\rm V}$||$p_{\rm max}$||$\lambda _{\rm max}$|K|$\theta _{\rm g^\prime }$||$\Delta \theta /\Delta \lambda$|GCVS
(HD)(Alt.)(ICRS J2000)(mas)(mag)(mag)(mag)(mag)(per cent)(⁠|$\mu$|m)(⁠|$^{\circ }$|⁠)(⁠|$^{\circ }/\mu$|m)
7927|$\phi$| Cas01 20 04.9|$+$|58 13 540.21F0 Ia5.664.980.513.113.310.5070.8593.0|$-$|5.7
23512BD|$+$|23 52403 46 34.2|$+$|23 37 267.33A0 V8.448.090.373.272.290.6001.0130.4|$-$|3.6
433849 Gem06 16 58.7|$+$|23 44 270.55B3 Iab6.706.250.573.063.060.5660.97170.0|$+$|2.6|$\alpha$| Cyg
80558LR Vel09 18 42.4|$-$|51 33 380.54B6 Ia6.475.930.593.253.340.5971.00163.3|$+$|1.4|$\alpha$| Cyg
84810|$\ell$| Car09 45 14.8|$-$|62 30 281.98G5 Iab5.093.750.183.721.620.5700.96100.00.0|$\delta$| Cep
111613DS Cru12 51 18.0|$-$|60 19 470.45A1 Ia6.105.720.403.723.140.5600.9480.80.0|$\alpha$| Cyg:
147084o Sco16 20 38.2|$-$|24 10 103.71A4 II5.404.570.753.674.410.6841.1531.80.0
149757|$\zeta$| Oph16 37 09.5|$-$|10 34 028.91O9.5 Vn2.582.560.322.931.450.6021.17127.2|$-$|5.0|$\gamma$| Cas
154445HR 635317 05 32.3|$-$|00 53 314.02B1 V5.735.610.403.033.660.5690.9590.00.0
160529V905 Sco17 41 59.0|$-$|33 30 140.54A2 Ia7.876.661.292.947.310.5430.9120.0|$+$|3.5|$\alpha$| Cyg:
161056HR 660117 43 47.0|$-$|07 04 472.44B1.5 V6.686.320.603.114.010.5840.9667.3|$-$|1.5
161471|$\iota ^1$| Sco17 47 35.1|$-$|40 07 371.69F2 Ia3.492.990.262.422.280.5600.942.4|$-$|1.1
183143HT Sge19 27 26.6|$+$|18 17 450.43B7 Iae8.086.861.243.166.160.5501.15179.20.0|$\alpha$| Cyg:
187929|$\eta$| Aql19 52 28.4|$+$|01 00 203.67F6 Ib|$^+$|4.613.800.163.101.730.5520.9393.7|$-$|7.3|$\delta$| Cep
19847855 Cyg20 48 56.3|$+$|46 06 510.54B3 Ia5.284.860.542.892.750.5150.883.00.0|$\alpha$| Cyg
203532HR 817621 33 54.6|$-$|82 40 593.44B3 IV6.516.380.323.051.390.5740.86126.9|$+$|2.4
210121HIP 109 26522 08 11.9|$-$|03 31 533.00B7 II7.847.680.352.221.380.4340.73155.1|$+$|8.6
StandardRADec.Plx.SpTBV|$E_{(B-V)}$||$R_{\rm V}$||$p_{\rm max}$||$\lambda _{\rm max}$|K|$\theta _{\rm g^\prime }$||$\Delta \theta /\Delta \lambda$|GCVS
(HD)(Alt.)(ICRS J2000)(mas)(mag)(mag)(mag)(mag)(per cent)(⁠|$\mu$|m)(⁠|$^{\circ }$|⁠)(⁠|$^{\circ }/\mu$|m)
7927|$\phi$| Cas01 20 04.9|$+$|58 13 540.21F0 Ia5.664.980.513.113.310.5070.8593.0|$-$|5.7
23512BD|$+$|23 52403 46 34.2|$+$|23 37 267.33A0 V8.448.090.373.272.290.6001.0130.4|$-$|3.6
433849 Gem06 16 58.7|$+$|23 44 270.55B3 Iab6.706.250.573.063.060.5660.97170.0|$+$|2.6|$\alpha$| Cyg
80558LR Vel09 18 42.4|$-$|51 33 380.54B6 Ia6.475.930.593.253.340.5971.00163.3|$+$|1.4|$\alpha$| Cyg
84810|$\ell$| Car09 45 14.8|$-$|62 30 281.98G5 Iab5.093.750.183.721.620.5700.96100.00.0|$\delta$| Cep
111613DS Cru12 51 18.0|$-$|60 19 470.45A1 Ia6.105.720.403.723.140.5600.9480.80.0|$\alpha$| Cyg:
147084o Sco16 20 38.2|$-$|24 10 103.71A4 II5.404.570.753.674.410.6841.1531.80.0
149757|$\zeta$| Oph16 37 09.5|$-$|10 34 028.91O9.5 Vn2.582.560.322.931.450.6021.17127.2|$-$|5.0|$\gamma$| Cas
154445HR 635317 05 32.3|$-$|00 53 314.02B1 V5.735.610.403.033.660.5690.9590.00.0
160529V905 Sco17 41 59.0|$-$|33 30 140.54A2 Ia7.876.661.292.947.310.5430.9120.0|$+$|3.5|$\alpha$| Cyg:
161056HR 660117 43 47.0|$-$|07 04 472.44B1.5 V6.686.320.603.114.010.5840.9667.3|$-$|1.5
161471|$\iota ^1$| Sco17 47 35.1|$-$|40 07 371.69F2 Ia3.492.990.262.422.280.5600.942.4|$-$|1.1
183143HT Sge19 27 26.6|$+$|18 17 450.43B7 Iae8.086.861.243.166.160.5501.15179.20.0|$\alpha$| Cyg:
187929|$\eta$| Aql19 52 28.4|$+$|01 00 203.67F6 Ib|$^+$|4.613.800.163.101.730.5520.9393.7|$-$|7.3|$\delta$| Cep
19847855 Cyg20 48 56.3|$+$|46 06 510.54B3 Ia5.284.860.542.892.750.5150.883.00.0|$\alpha$| Cyg
203532HR 817621 33 54.6|$-$|82 40 593.44B3 IV6.516.380.323.051.390.5740.86126.9|$+$|2.4
210121HIP 109 26522 08 11.9|$-$|03 31 533.00B7 II7.847.680.352.221.380.4340.73155.1|$+$|8.6

Notes:|$+\, \eta$| Aql has an SB companion classified computationally as B9.8 V. Photometric data and astrometric data, presented in sexagesimal IRCS J2000, are taken directly from SIMBAD. For the origin/derivation of position angle data see Appendix  A. Note that |$\theta$| is given for the SDSS |$g^\prime$| band and a 2020 equinox. For the origin of Serkowski fit parameters, reddening data and spectral type references see Appendix  B. The final column has the variability type as given in the General Catalogue of Variable Stars (GCVS; Samus’ et al. 2017), where a colon indicates some uncertainty; HD 160 529 is elsewhere classified as a Luminous Blue Variable (LBV) star (e.g. Stahl et al. 2003), and HD 149 757 as an Oe star (e.g. Negueruela, Steele & Bernabeu 2004) and a |$\beta$| Cep star (e.g. Hubrig, Oskinova & Schöller 2011).

Table 1.

Properties of high polarization standard stars.

StandardRADec.Plx.SpTBV|$E_{(B-V)}$||$R_{\rm V}$||$p_{\rm max}$||$\lambda _{\rm max}$|K|$\theta _{\rm g^\prime }$||$\Delta \theta /\Delta \lambda$|GCVS
(HD)(Alt.)(ICRS J2000)(mas)(mag)(mag)(mag)(mag)(per cent)(⁠|$\mu$|m)(⁠|$^{\circ }$|⁠)(⁠|$^{\circ }/\mu$|m)
7927|$\phi$| Cas01 20 04.9|$+$|58 13 540.21F0 Ia5.664.980.513.113.310.5070.8593.0|$-$|5.7
23512BD|$+$|23 52403 46 34.2|$+$|23 37 267.33A0 V8.448.090.373.272.290.6001.0130.4|$-$|3.6
433849 Gem06 16 58.7|$+$|23 44 270.55B3 Iab6.706.250.573.063.060.5660.97170.0|$+$|2.6|$\alpha$| Cyg
80558LR Vel09 18 42.4|$-$|51 33 380.54B6 Ia6.475.930.593.253.340.5971.00163.3|$+$|1.4|$\alpha$| Cyg
84810|$\ell$| Car09 45 14.8|$-$|62 30 281.98G5 Iab5.093.750.183.721.620.5700.96100.00.0|$\delta$| Cep
111613DS Cru12 51 18.0|$-$|60 19 470.45A1 Ia6.105.720.403.723.140.5600.9480.80.0|$\alpha$| Cyg:
147084o Sco16 20 38.2|$-$|24 10 103.71A4 II5.404.570.753.674.410.6841.1531.80.0
149757|$\zeta$| Oph16 37 09.5|$-$|10 34 028.91O9.5 Vn2.582.560.322.931.450.6021.17127.2|$-$|5.0|$\gamma$| Cas
154445HR 635317 05 32.3|$-$|00 53 314.02B1 V5.735.610.403.033.660.5690.9590.00.0
160529V905 Sco17 41 59.0|$-$|33 30 140.54A2 Ia7.876.661.292.947.310.5430.9120.0|$+$|3.5|$\alpha$| Cyg:
161056HR 660117 43 47.0|$-$|07 04 472.44B1.5 V6.686.320.603.114.010.5840.9667.3|$-$|1.5
161471|$\iota ^1$| Sco17 47 35.1|$-$|40 07 371.69F2 Ia3.492.990.262.422.280.5600.942.4|$-$|1.1
183143HT Sge19 27 26.6|$+$|18 17 450.43B7 Iae8.086.861.243.166.160.5501.15179.20.0|$\alpha$| Cyg:
187929|$\eta$| Aql19 52 28.4|$+$|01 00 203.67F6 Ib|$^+$|4.613.800.163.101.730.5520.9393.7|$-$|7.3|$\delta$| Cep
19847855 Cyg20 48 56.3|$+$|46 06 510.54B3 Ia5.284.860.542.892.750.5150.883.00.0|$\alpha$| Cyg
203532HR 817621 33 54.6|$-$|82 40 593.44B3 IV6.516.380.323.051.390.5740.86126.9|$+$|2.4
210121HIP 109 26522 08 11.9|$-$|03 31 533.00B7 II7.847.680.352.221.380.4340.73155.1|$+$|8.6
StandardRADec.Plx.SpTBV|$E_{(B-V)}$||$R_{\rm V}$||$p_{\rm max}$||$\lambda _{\rm max}$|K|$\theta _{\rm g^\prime }$||$\Delta \theta /\Delta \lambda$|GCVS
(HD)(Alt.)(ICRS J2000)(mas)(mag)(mag)(mag)(mag)(per cent)(⁠|$\mu$|m)(⁠|$^{\circ }$|⁠)(⁠|$^{\circ }/\mu$|m)
7927|$\phi$| Cas01 20 04.9|$+$|58 13 540.21F0 Ia5.664.980.513.113.310.5070.8593.0|$-$|5.7
23512BD|$+$|23 52403 46 34.2|$+$|23 37 267.33A0 V8.448.090.373.272.290.6001.0130.4|$-$|3.6
433849 Gem06 16 58.7|$+$|23 44 270.55B3 Iab6.706.250.573.063.060.5660.97170.0|$+$|2.6|$\alpha$| Cyg
80558LR Vel09 18 42.4|$-$|51 33 380.54B6 Ia6.475.930.593.253.340.5971.00163.3|$+$|1.4|$\alpha$| Cyg
84810|$\ell$| Car09 45 14.8|$-$|62 30 281.98G5 Iab5.093.750.183.721.620.5700.96100.00.0|$\delta$| Cep
111613DS Cru12 51 18.0|$-$|60 19 470.45A1 Ia6.105.720.403.723.140.5600.9480.80.0|$\alpha$| Cyg:
147084o Sco16 20 38.2|$-$|24 10 103.71A4 II5.404.570.753.674.410.6841.1531.80.0
149757|$\zeta$| Oph16 37 09.5|$-$|10 34 028.91O9.5 Vn2.582.560.322.931.450.6021.17127.2|$-$|5.0|$\gamma$| Cas
154445HR 635317 05 32.3|$-$|00 53 314.02B1 V5.735.610.403.033.660.5690.9590.00.0
160529V905 Sco17 41 59.0|$-$|33 30 140.54A2 Ia7.876.661.292.947.310.5430.9120.0|$+$|3.5|$\alpha$| Cyg:
161056HR 660117 43 47.0|$-$|07 04 472.44B1.5 V6.686.320.603.114.010.5840.9667.3|$-$|1.5
161471|$\iota ^1$| Sco17 47 35.1|$-$|40 07 371.69F2 Ia3.492.990.262.422.280.5600.942.4|$-$|1.1
183143HT Sge19 27 26.6|$+$|18 17 450.43B7 Iae8.086.861.243.166.160.5501.15179.20.0|$\alpha$| Cyg:
187929|$\eta$| Aql19 52 28.4|$+$|01 00 203.67F6 Ib|$^+$|4.613.800.163.101.730.5520.9393.7|$-$|7.3|$\delta$| Cep
19847855 Cyg20 48 56.3|$+$|46 06 510.54B3 Ia5.284.860.542.892.750.5150.883.00.0|$\alpha$| Cyg
203532HR 817621 33 54.6|$-$|82 40 593.44B3 IV6.516.380.323.051.390.5740.86126.9|$+$|2.4
210121HIP 109 26522 08 11.9|$-$|03 31 533.00B7 II7.847.680.352.221.380.4340.73155.1|$+$|8.6

Notes:|$+\, \eta$| Aql has an SB companion classified computationally as B9.8 V. Photometric data and astrometric data, presented in sexagesimal IRCS J2000, are taken directly from SIMBAD. For the origin/derivation of position angle data see Appendix  A. Note that |$\theta$| is given for the SDSS |$g^\prime$| band and a 2020 equinox. For the origin of Serkowski fit parameters, reddening data and spectral type references see Appendix  B. The final column has the variability type as given in the General Catalogue of Variable Stars (GCVS; Samus’ et al. 2017), where a colon indicates some uncertainty; HD 160 529 is elsewhere classified as a Luminous Blue Variable (LBV) star (e.g. Stahl et al. 2003), and HD 149 757 as an Oe star (e.g. Negueruela, Steele & Bernabeu 2004) and a |$\beta$| Cep star (e.g. Hubrig, Oskinova & Schöller 2011).

Close
This Feature Is Available To Subscribers Only

Sign In or Create an Account

Close

This PDF is available to Subscribers Only

View Article Abstract & Purchase Options

For full access to this pdf, sign in to an existing account, or purchase an annual subscription.

Close