  The K2 eclipsing binary candidates EPIC 211982753 (hereinafter called
EPIC2753) and EPIC 211915147 (hereinafter called EPIC5147) are characterized
with the help of photometric and high-resolution spectroscopic data. The light
curve analysis uses the R-band photometric data from the 1.3-m Devasthal Fast
Optical Telescope (DFOT, India), ASAS-3 and K2 observations. High-resolution
echelle spectra are collected using the HERMES spectrograph at the 1.2-m
MERCATOR telescope (La Palma, Spain). The synthetic light and radial velocity
curves are generated with the help of the modeling package PHOEBE 1.0. The
orbital period analysis based on the ~3.2 years of K2 observations does not
show any change in the orbital period of both targets. The component masses
M1,2 are estimated as 1.69(0.02) and 1.59(0.02) solar mass for EPIC2753, and
1.48(0.01) and 1.27(0.01) solar mass for EPIC5147. Both systems are high
mass-ratio eclipsing binaries with q>0.85. The component radii R1,2 are found
to be 1.66(0.02) and 1.53(0.02) solar radius for EPIC2753, and 1.80(0.05) and
1.42(0.05) solar radius for EPIC5147. The distances of EPIC2753 and EPIC5147
are determined as 238(4) and 199(5) pc, respectively. MESA Isochrones and
Stellar Tracks are used to understand the evolutionary status of both systems.
