  Using the Wide Field Grism Spectrograph 2 (WFGS2), we have carried out
slit-less spectroscopy, g'r'i' photometry, and slit spectroscopy on the L1014
dense core. We detected three Halpha emission line stars. We interpret one as
weak-line T Tauri star (WTTS) and the others as classical T Tauri stars (CTTS).
Since their g'-i' colors and/or classified spectral types are consistent with
those of T Tauri stars and two of them show less extinction than the cloud,
these three stars are likely to be T Tauri stars associated with L1014.
Adopting an age range for T Tauri stars, 1-10 Myr, the color-magnitude diagram
suggests a distance of ~400-900 pc, rather than the previously assumed
distance, 200 pc. This could strongly affect on the mass estimate of L1014-IRS,
which is thought to be either a very young protostar or proto-brown dwarf.
