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Table 1:

Intrinsic parameters, mean NIR magnitudes, and mean radial velocities for the target Cepheids.

NAME
$\alpha$(J2000)a $\delta$(J2000)a $\log P$ E(B-V)b $\langle J\rangle$c $\pm$ $\sigma(J)$ $\langle H\rangle $c $\pm$ $\sigma(H)$ $\langle K\rangle $c $\pm$ $\sigma(K)$ $N_{\rm s}$d $\langle v_{\rm r}\rangle$e $\Delta v_{\rm r}$e
V340 Ara 16 45 19 -51 20 33 1.32 0.574 $7.382\pm0.011$ $6.809\pm0.007$ $6.619\pm0.008$ 25+2 $-80.8\pm1.2$ 59.1
UZ Sct 18 31 22 -12 55 00 1.17 1.071 $7.502\pm0.049$ $6.818\pm0.042$ $6.564\pm0.045$ 25+2 $40.2\pm0.5$ 49.4
AV Sgr 18 04 49 -22 43 00 1.19 1.267 $6.909\pm0.040$ $6.081\pm0.035$ $5.758\pm0.033$ 25+1 $19.3\pm1.8$ 59.3
VY Sgr 18 12 05 -20 42 00 1.13 1.283 $7.174\pm0.069$ $6.375\pm0.046$ $6.068\pm0.040$ 25+2 $16.0\pm1.8$ 59.2

Notes. (a) Cepheid coordinates: units of right ascension are hours, minutes, and seconds; units of declination are degrees, arcminutes, and arcseconds. (b) Reddening according to Fernie et al. (1995). (c) Mean NIR magnitudes. (d) Number of spectra collected with FEROS at the 2.2 m MPG/ESO telescope. (e) Mean radial velocity and velocity amplitude (km s-1).


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