Table A4.

Coordinates, proper motions, parallax, and radial velocity (where known) of NGC 7826 members from the literature. Not a single pair of stars can be found with matching parameters. The magnitudes of the stars extend from V = 9.72 to V = 16.67.

αδμα cos (δ)μδϖ|$v$|r
°°|$\mathrm{mas\, yr^{-1}}$||$\mathrm{mas\, yr^{-1}}$|mas|$\mathrm{km\, s^{-1}}$|
Membersa in Dias et al. (2002, 2014)
1.3897–20.858812.26 ± 0.122.83 ± 0.070.72 ± 0.07
1.1267–20.697046.70 ± 0.09–5.49 ± 0.063.22 ± 0.06–1.1 ± 0.2b
1.2085–20.656725.99 ± 0.06–11.67 ± 0.041.30 ± 0.03
1.2711–20.634715.25 ± 0.07–8.40 ± 0.050.36 ± 0.0477.3 ± 0.1c
1.2949–20.741314.65 ± 0.101.17 ± 0.061.18 ± 0.05
1.2976–20.602019.74 ± 0.056.47 ± 0.030.79 ± 0.03–17.8 ± 0.1c
1.3595–20.722638.34 ± 0.125.27 ± 0.063.39 ± 0.0516.3 ± 0.7b
1.3745–20.605627.03 ± 0.07–5.63 ± 0.043.53 ± 0.04–2.9 ± 0.1c
1.4658–20.704816.05 ± 0.05–5.44 ± 0.040.92 ± 0.04
1.2480–20.562318.41 ± 0.07–8.65 ± 0.051.99 ± 0.0412.9 ± 1.1b
1.4210–20.588312.84 ± 0.081.43 ± 0.042.54 ± 0.04
αδμα cos (δ)μδϖ|$v$|r
°°|$\mathrm{mas\, yr^{-1}}$||$\mathrm{mas\, yr^{-1}}$|mas|$\mathrm{km\, s^{-1}}$|
Membersa in Dias et al. (2002, 2014)
1.3897–20.858812.26 ± 0.122.83 ± 0.070.72 ± 0.07
1.1267–20.697046.70 ± 0.09–5.49 ± 0.063.22 ± 0.06–1.1 ± 0.2b
1.2085–20.656725.99 ± 0.06–11.67 ± 0.041.30 ± 0.03
1.2711–20.634715.25 ± 0.07–8.40 ± 0.050.36 ± 0.0477.3 ± 0.1c
1.2949–20.741314.65 ± 0.101.17 ± 0.061.18 ± 0.05
1.2976–20.602019.74 ± 0.056.47 ± 0.030.79 ± 0.03–17.8 ± 0.1c
1.3595–20.722638.34 ± 0.125.27 ± 0.063.39 ± 0.0516.3 ± 0.7b
1.3745–20.605627.03 ± 0.07–5.63 ± 0.043.53 ± 0.04–2.9 ± 0.1c
1.4658–20.704816.05 ± 0.05–5.44 ± 0.040.92 ± 0.04
1.2480–20.562318.41 ± 0.07–8.65 ± 0.051.99 ± 0.0412.9 ± 1.1b
1.4210–20.588312.84 ± 0.081.43 ± 0.042.54 ± 0.04

aOnly members with probability >0.9.

b|$v$|r from Gaia DR2.

c|$v$|r from GALAH.

Table A4.

Coordinates, proper motions, parallax, and radial velocity (where known) of NGC 7826 members from the literature. Not a single pair of stars can be found with matching parameters. The magnitudes of the stars extend from V = 9.72 to V = 16.67.

αδμα cos (δ)μδϖ|$v$|r
°°|$\mathrm{mas\, yr^{-1}}$||$\mathrm{mas\, yr^{-1}}$|mas|$\mathrm{km\, s^{-1}}$|
Membersa in Dias et al. (2002, 2014)
1.3897–20.858812.26 ± 0.122.83 ± 0.070.72 ± 0.07
1.1267–20.697046.70 ± 0.09–5.49 ± 0.063.22 ± 0.06–1.1 ± 0.2b
1.2085–20.656725.99 ± 0.06–11.67 ± 0.041.30 ± 0.03
1.2711–20.634715.25 ± 0.07–8.40 ± 0.050.36 ± 0.0477.3 ± 0.1c
1.2949–20.741314.65 ± 0.101.17 ± 0.061.18 ± 0.05
1.2976–20.602019.74 ± 0.056.47 ± 0.030.79 ± 0.03–17.8 ± 0.1c
1.3595–20.722638.34 ± 0.125.27 ± 0.063.39 ± 0.0516.3 ± 0.7b
1.3745–20.605627.03 ± 0.07–5.63 ± 0.043.53 ± 0.04–2.9 ± 0.1c
1.4658–20.704816.05 ± 0.05–5.44 ± 0.040.92 ± 0.04
1.2480–20.562318.41 ± 0.07–8.65 ± 0.051.99 ± 0.0412.9 ± 1.1b
1.4210–20.588312.84 ± 0.081.43 ± 0.042.54 ± 0.04
αδμα cos (δ)μδϖ|$v$|r
°°|$\mathrm{mas\, yr^{-1}}$||$\mathrm{mas\, yr^{-1}}$|mas|$\mathrm{km\, s^{-1}}$|
Membersa in Dias et al. (2002, 2014)
1.3897–20.858812.26 ± 0.122.83 ± 0.070.72 ± 0.07
1.1267–20.697046.70 ± 0.09–5.49 ± 0.063.22 ± 0.06–1.1 ± 0.2b
1.2085–20.656725.99 ± 0.06–11.67 ± 0.041.30 ± 0.03
1.2711–20.634715.25 ± 0.07–8.40 ± 0.050.36 ± 0.0477.3 ± 0.1c
1.2949–20.741314.65 ± 0.101.17 ± 0.061.18 ± 0.05
1.2976–20.602019.74 ± 0.056.47 ± 0.030.79 ± 0.03–17.8 ± 0.1c
1.3595–20.722638.34 ± 0.125.27 ± 0.063.39 ± 0.0516.3 ± 0.7b
1.3745–20.605627.03 ± 0.07–5.63 ± 0.043.53 ± 0.04–2.9 ± 0.1c
1.4658–20.704816.05 ± 0.05–5.44 ± 0.040.92 ± 0.04
1.2480–20.562318.41 ± 0.07–8.65 ± 0.051.99 ± 0.0412.9 ± 1.1b
1.4210–20.588312.84 ± 0.081.43 ± 0.042.54 ± 0.04

aOnly members with probability >0.9.

b|$v$|r from Gaia DR2.

c|$v$|r from GALAH.

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