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Table 1

Test spectra.

Star Prog. ID R = λ/ Δλ Slit width (′′) S/Na Ref. Avb E(B−V) c Dd (pc) Ref.
NGC 2682 Sanders1092 66.D-0457 87 410 0.̋4 ~80 S09 0.094 0.06 986 P10
NGC 2682 Sanders1048 66.D-0457 87 410 0.̋4 ~80 S09 0.094 0.06 986 P10
NGC 2682 No164 079.C-0131 45 990 0.̋9 100–200 S09 0.094 0.06 986 P10
NGC 2682 No266 079.C-0131 45 990 0.̋9 100–200 S09 0.094 0.06 986 P10
IC 4651 AMC1109 66.D-0457 87 410 0.̋4 ~80 S09 0.663 0.12 888 K05
IC 4651 AMC4226 66.D-0457 87 410 0.̋4 ~80 S09 0.663 0.12 888 K05
NGC 6705 No1111 383.C-0170 107 200 0.̋3 200 S12 2.521 0.43 1877 K05
NGC 6705 No1184 383.C-0170 107 200 0.̋3 200 S12 2.521 0.43 1877 K05

Notes.

(a)

Signal-to-noise ratio as provided in the reference quoted in the sixth column.

(b)

Total galactic extinction as provided by the NED using the Schlafly & Finkbeiner (2011) recalibration of the Schlegel et al. (1998) infrared-based dust map.

(c)

Reddening of the cluster as provided in the reference quoted in the last column.

(d)

Distance to the cluster as provided in the reference quoted in the last column.

Reference. S09: Santos et al. (2009); S12: Santos et al. (2012); P10: Pandey et al. (2010); K05: Kharchenko et al. (2005).

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