Lyman Break Galaxies at z$\sim$5: Rest-Frame UV Spectra. II

We present spectroscopy results of Lyman break galaxies (LBGs) at z$$\sim$$5 in the J0053$$+$$1234 field. Among five bright candidates with z$$'$$ $$\;<\;$$25.0 mag, two objects are confirmed to be at z$$\;\sim\;$$5. The equivalent widths (EWs) of Ly$$\alpha$$ emission of the 2 LBGs are not so strong as to be detected as Ly$$\alpha$$ emitters, and one of them shows strong low-ionization interstellar (LIS) metal absorption lines. Two faint objects with z$$'$$ $$\geq$$25.0 mag are also confirmed to be at z$$\;\sim\;$$5, and their spectra show strong Ly$$\alpha$$ emission in contrast to bright ones. These results suggest a deficiency of strong Ly$$\alpha$$ emission in bright LBGs at z$$\;\sim\;$$5, as discussed in our previous paper. Combined with our previous spectra of LBGs at z$$\;\sim\;$$5, obtained around the Hubble Deep Field-North (HDF-N), we made a composite spectrum of luminous ($$M_{1400} \leq -$$21.5 mag) LBGs at z$$\;\sim\;$$5. The resultant spectrum shows weak Ly$$\alpha$$ emission and strong LIS absorptions, which suggest that the bright LBGs at z$$\;\sim\;$$5 have chemically evolved at least to $$\sim$$0.1 solar metallicity. For a part of our sample in the HDF-N region, we obtained near-to-mid infrared data, which constrain the stellar masses of these objects. With the stellar mass and the metallicity estimated from the LIS absorptions, the metallicities of the LBGs at z$$\;\sim\;$$5 tend to be lower than those of galaxies with the same stellar mass at z$$\lesssim 2$$, although the uncertainty is very large.