Oscillations of red giants observed by Kepler (Mosser+, 2012)

Asymptotic mixed-modes parameters of the red giant oscillation spectra shown in the paper. Dnu is the large separation. numax indicates the central frequency of the oscillation power excess. DPi1 is the gravity period spacing, eDPi1 its uncertainty, assuming that {epsilon}g_ is fixed to 1/2. If Dpi1 changes too much along the mixed-mode spectrum, DPi1b gives the second possible value. q is the coupling factor, e_q its uncertainty. Mass and Rad are the asteroseismic estimates of the stellar mass and radius from scaling relations, using Teff from the Kepler Input Catalog (Brown et al. 2011, Cat. V/133). The division between RGB and clump stars is derived from Fig. 3; the limit between the primary and secondary clump stars is set at 1.8 solar mass. Note: table1.dat 218x63 Characteristic parameters of the red giants.