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Table 2.

Comparison of the common catalogs of the surveys.

APOGEE-GALAH APOGEE-GES GALAH-GES
No. common stars (a) 37 770 (15 537) 2502 (804) 1510 (441)
Common parameters Teff, log g, vrad, [Fe/H], [α/Fe], vmicro Teff, log g, vrad, [Fe/H], vmicro Teff, log g, vrad, [Fe/H], vmicro
Common elements C, O, Na, Mg, Al, Si, K, Ca, Ti, Ti II, V, Cr, Mn, Co, Ni, Cu C, C I, O, Na, Mg, Al, Si, S, Ca, Ti, Ti II, V, Cr, Mn, Co, Ni, Cu Li, C, O, Na, Mg, Al, Si, Ca, Sc, Sc II, Ti, Ti II, V, Cr, Cr II, Mn, Co, Ni, Cu, Zn, Sr, Zr, Mo, Ba II, La II, Ce II, Nd II, Sm II, Eu II
S/N cut (b) SNR > 100 & snr_c3_iraf> 30 SNR> 100 & SNR​​ > ​​50 snr_c3_iraf > 30 & SNR​​ > ​​50
Other quality cuts (b) vbroad​​ < ​​15 & flag_sp​​ = =​​0 & flag_fe_h​​ = =​​0 & VSCATTER​​ < ​​1 & VSINI​​ < ​​15 & VERR​​ < ​​1, flags VSCATTER​​ < ​​1 & VSINI​​ < ​​15 & VERR​​ < ​​1 & ERROR_TEFF/TEFF​​ < ​​5% & E_VRAD​​ < ​​1, flags ERROR_TEFF/TEFF​​ < ​​5% & flag_sp​​ = =​​0 & flag_fe_h​​ = =​​0 & vbroad​​ < ​​15 & VSINI​​ < ​​15 & E_VRAD​​ < ​​1, flags

μ ± σ μ ± σ μ ± σ μ ± σ μ ± σ μ ± σ
dwarfs giants dwarfs giants dwarfs giants

ΔTeff(K) 43.6 ± 137.3 −54.3 ± 91.7 −15.0 ± 114.7 −64.3 ± 117.2 −60.4 ± 112.8 21.2 ± 111.3
overall −5.4 ± 126.6 −57.4 ± 118.1 −12.0 ± 125.5
Δlog g(dex) 0.01 ± 0.13 0.09 ± 0.22 −0.03 ± 0.17 −0.03 ± 0.33 −0.02 ± 0.16 −0.14 ± 0.22
overall 0.05 ± 0.19 −0.03 ± 0.31 −0.09 ± 0.20
Δ[M/H](c) 0.006 ± 0.082 0.039 ± 0.121 −0.020 ± 0.077 −0.014 ± 0.102 −0.010 ± 0.080 −0.107 ± 0.165
overall 0.023 ± 0.105 −0.015 ± 0.099 −0.072 ± 0.170
Δ[α/H](dex) −0.014 ± 0.082 0.005 ± 0.107 ... .... ... ...
overall −0.005 ± 0.096 ... ...
Δvmicro(km s−1) −0.34 ± 0.42 −0.03 ± 0.36 −0.44 ± 0.37 −0.09 ± 0.35 −0.10 ± 0.23 −0.18 ± 0.19
overall −0.18 ± 0.43 −0.16 ± 0.38 −0.14 ± 0.22
Δvrad(km s−1) −0.01 ± 4.10 −0.04 ± 2.81 0.49 ± 1.26 0.09 ± 2.69 0.69 ± 4.37 −0.21 ± 4.09
overall −0.02 ± 3.51 0.15 ± 2.54 0.11 ± 4.18

Notes. The quality cuts, common parameters, and abundances are listed for the APOGEE−GALAH, APOGEE−Gaia-ESO, and GALAH−Gaia-ESO stellar catalogs. The average and scatter of differences are calculated overall, and after separating MS and GB stars. No data is given in the table cell if there is no available corresponding data. The confidence interval is ±1σ. Overall means do not differentiate between MS and RGB stars.

(a)

The number of common stars refers to the data sets before (after) the cuts.

(b)

For more information about each filtering criterion, see Sect. 2.2.

(c)

For APOGEE we use [M/H] rather than [Fe/H].

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