Title: Stromgren survey for Asteroseismology and Galactic Archaeology: let the SAGA begin Authors: Casagrande L., Silva Aguirre V., Stello D., Huber D., Serenelli A.M., Cassisi S., Dotter A., Milone A.P., Hodgkin S., Marino F.A., Lund M.N., Pietrinferni A., Asplund M., Feltzing S., Flynn C., Grundahl F., Nissen P.E., Schoenrich R., Schlesinger K.J., Wang W. Table: SAGA Asteroseismic Catalog ================================================================================ Byte-by-byte Description of file: star_prop_uvby.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 7 A7 --- KICID Kepler Input Catalog designation 8 A1 --- f_KICID [*] Flag on KICID (1) 10- 15 F6.1 uHz numax Frequency of maximum oscillations power 17- 21 F5.1 uHz e_numax Uncertainty in numax 23- 28 F6.2 uHz dnu Large frequency separation 30- 33 F4.2 uHz e_dnu Uncertainty in dnu 35- 39 F5.2 [Sun] [Fe/H] Stroemgren metallicity (2) 41- 44 F4.2 [Sun] e_[Fe/H] Uncertainty in Stroemgren metallicity 46- 49 I4 K Teff Effective temperature from the IRFM 51- 53 I3 K e_Teff Error in Teff 55- 59 F5.2 solRad Radius Radius from seismology 61- 65 F5.2 solRad E_Radius Upper error in Radius 67- 71 F5.2 solRad e_Radius Lower error in Radius 73- 76 F4.2 solMass Mass Mass from seismology 78- 81 F4.2 solMass E_Mass Upper error in Mass 83- 86 F4.2 solMass e_Mass Lower error in Mass 88- 92 F5.3 [cm/s2] log(g) Log surface gravity from seismology 94- 98 F5.3 [cm/s2] E_log(g) Upper error in log(g) 100-104 F5.3 [cm/s2] e_log(g) Lower error in log(g) 106-114 F9.7 Sun Den Stellar density (3) 116-124 F9.7 Sun E_Den Upper error in Den 126-134 F9.7 Sun e_Den Lower error in Den 136-139 I4 pc Dis Distance from the Sun 141-144 I4 pc E_Dis Upper error in Dis 146-149 I4 pc e_Dis Lower error in Dis 151-155 A5 --- Class Asteroseismic classification (4) 157 I1 --- Mflg Metallicity flag (5) 159 I1 --- Pflg Stroemgren photometry flag (5) 161-165 F5.3 mag b-y Stroemgren b-y index 167-171 F5.3 mag m1 Stroemgren m1 index 173-177 F5.3 mag c1 Stroemgren c1 index -------------------------------------------------------------------------------- Note (1): * = indicates the presence of a second oscillation signal in the Kepler data, indicating a likely binary (see discussion in Section 3.6 of the paper). Note (2): Determined as described in Section 3.2 of the paper for stars having classification 'RGB', 'RC', 'NO'. For stars classified as 'Dwarf' the Stroemgren metallicity calibration of Casagrande et al. (2011) has been used (with the exception of 5629080 and 7107778, classified as Dwarf but at the base of the RGB, and for which the same calibration of RGB/RC/NO has been used instead). Notice that [Fe/H] > 0.5 dex should not be trusted. Only stars having both Mflg and Pflg equal 0 should be trusted (see Note 5). Note (3): In units of solar density (1.4084 g cm-3). Note (4): Seismic classification as described in Section 3.4 of the paper. RGB = certain Red Giant Branch. RC = certain Red Clump. NO = no reliable distinction between RGB and RC could be made. Dwarf = dwarf star (from Chaplin et al. 2014, ApJS, 210, 1). Note (5): Quality flags identifying stars with most reliable Stroemgren metallicities. Mflg = 0 if the Stroemgren metallicity calibration is applied within its range of applicability (Section 3.2 of the paper). Pflg = 0 if photometric errors of Stroemgren u,v,b,y magnitudes are below photometric fiducials (Section 2.3 and Figure 4 of the paper). Unreliable Stroemgren u,v,b,y imply unreliable photometric metallicities. Stars with both Mflg and Pflg equal 0 have more reliable [Fe/H].