All Tables

• Table 3: Description of used instruments during the exploratory program. FOV (i.e. Col. 4) stands for "Field Of View''.
• Table 6: Fitting zones used to derive the projected rotation velocity and effective temperature.
• Table 7: Stellar parameters of the targets. Remarks: "VAR" are the short-term variables; "ell.'' means ellipsoidal variations are detected in the CCD photometry. The spectra of the 3 framed SB2 targets were analysed accounting for the contribution of two components. Numbers between brackets represent the number of measurements used to compute the average radial velocity (Col. 6).
• Table 8: Adopted frequency-solution based on the weighted analyses of the sets "B All'' and "V All''.
• Table 9: Amplitude(s) (ratios) and phase(s) (differences) in two filters for the adopted frequency-solution. All the phases are computed with respect to the initial epoch of set "B All''. The standard errors on the derived parameters are also shown.
• Table 10: Derived pulsation constants for the frequencies of the adopted solution and possibly corresponding mode identification.
• Table 11: Orbital parameters of HD 11190 assuming a circular orbit.
• Table 12: List of interesting targets.
• Table 1: Target description. Nref is the number of references in SIMBAD at present. The spectral type is from Grenier et al. (1999).
• Table 2: Journal of spectroscopic observations at NAO, OHP and TBL.
• Table 4: Journal of CCD photometric exploratory observations of the variable candidates. Observations were made at the Beersel Hills Observatory (BHO) and the Hoher List Observatory from the Argelander Institute for Astronomy, Bonn (HLO).
• Table 5: Log of the CCD differential multi-site photometric campaign conducted for HD 217860.