Asteroseismic measurement of core and envelope rotation rates for 2006 red giant branch stars

We provide mode identifications of all the ~2500 RGB stars and a table that includes all the fitting results.

In the file "mode_ID_for_2500_RGB.zip", you can find a lot of folders with KIC number in their folder names. In each folder, the files "KIC*l*n*fitting_detail.dat" show the Lorentzian profile fitting for l=0 or 2 modes (see l value in the file name). The first row is the fitting result (the frequency value is in the second column) and the second row is uncertainty.

for l=1 mixed modes, you can find them in the files "KIC*bin_points*for_l_1_m*.dat". This is just an approximation of the mode frequencies. You should run a Lorentzian profile fitting using these frequencies as initial guess to obtain a precise mode frequency.

For the table "all_red_giants_table.csv"

Column 1: KIC

Column 2: nu_max in microHz

Column 3 and 4: large separation Delta_nu and uncertainty, in microHz

Column 5 and 6: p-mode phase and uncertainty.

Column 7 and 8: second order coefficient of p-mode asymptotic relation.

Column 9 and 10: the term D related to the small separation, in microHz.

Column 11 and 12: period spacing Delta Pi 1 and the uncertainty, in seconds.

Column 13 and 14: coupling factor q and its uncertainty.

Column 15 and 16: g-mode phase and uncertainty.

Column 17 and 18: frequency shift and uncertainty, in microHz.

Coumn 19 and 20: angular frequency of core rotation, in microHz. Note to divided by 2pi.

Coumn 21 and 22: angular frequency of envelope rotation, in microHz. Note to divided by 2pi.

Column 23 and 24: effective temperature and uncertainty, in Kelvin.

Column 25 and 26: luminosity and uncertainty, in solar luminosity

Column 27 and 28: Fe/H and uncertainty.

Column 29 and 30: stellar mass and uncertainty, in solar mass.

Column 31 and 32: stellar radius and uncertainty, in solar radius.

Column 33 and 34: inclination of rotational axis and uncertainty, in degree.

Column 35 and 36: linewidth_0 and uncertainty, in microHz.

Column 37 and 38: age and uncertainty, in Gyr.

Column 39: Gaia ruwe.