Table 1
Fundamental parameters and computed asteroseismic characteristics of the campaign targets.
| Star | Sp. | RA | Dec | V | π | vsini | Teff | [Fe/H] | Lum | Radius | Mass | νmax | Δν | Prot | |
| name | typ | [h m] | [°′] | [mag] | [mas] | [km s-1] | [K] | [dex] | [L⊙] | [R⊙] | [M⊙] | [μHz] | [μHz] | [days] | |
|
|
|||||||||||||||
| γ Psc | G9III | 23 17 | +03 17 | 3.7 | 23.6 ± 0.2 | 4.7 | 4940 | –0.62 | 63 | 10.4 | 1.87 | 60 | 5.7 | 112.6 | |
| θ1 Tau | K0III | 04 29 | +15 58 | 3.8 | 21.1 ± 0.3 | 4.2 | 5000 | +0.10 | 69 | 11.4 | 2.8 ± 0.5 | 76 | 6.1 | 138.2 | |
Notes. The coordinates (RA, Dec) are listed for the epoch 2000.0. The spectral type (Sp), luminosity class were adopted from the Hipparcos catalogue; parallaxes from van Leeuwen (2007). The effective temperature (Teff), projected rotational surface velocity (vsini) was taken from Hekker & Meléndez (2007), the metallicity [Fe/H] from Takeda et al. (2008). The luminosity (Lum) and stellar radius were obtained from the photometric calibration following Flower (1996). The mass for γ Psc and θ1 Tau were taken from Luck & Heiter (2007) and Lebreton et al. (2001), respectively. The estimated frequency of the maximum oscillation power excess, νmax, the large frequency separation Δν and surface rotation period Prot were calculated, based on the radius from the photometric calibration and the mass estimates from the literature. Uncertainties for all values from literature are given when provided.
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