We report infrared (IR) spectra of HSCS, c-HSCS, HCS, and other species produced on electron bombardment of a mixture of CS and para-hydrogen (p-H) during deposition at 3.2 K. After maintenance of the deposited matrix in darkness for 12 h, the intensities of the absorption lines of HSCS at 2477.2 (ν), 1525.6 (ν), and 919.6 cm (ν) decreased through neutralization of HSCS with trapped electrons. During this period, the intensities of the lines of HCS at 2875.7 (ν), 1249.9 (ν), 1003.2 (ν), and 814.3 cm (ν) increased due to reaction between H and CS. The intensities of the lines observed at 2312.7 and 889.0 cm, which are assigned to the c-HSCS radical, increased after maintenance in darkness and greatly diminished after irradiation at 373 nm. The IR spectra of HSCS, HCS, and c-HSCS are reported for the first time. The IR absorption lines of the t-HSCS radical, t-HC(S)SH, and c-HC(S)SH were also identified; their wavenumbers are similar to those reported for these species in an Ar matrix. The corresponding spectra of the C,S, and D isotopic variants of these species were observed. The assignments were made according to the expected chemical behavior, predicted potential energies of associated reactions, and a comparison of observed and predicted wavenumbers and their C,S, and D isotopic ratios. In contrast to the observed significant red shifts of the OH-stretching wavenumbers of HOCO and HOCS in solid p-H compared to those in the gaseous phase due to proton sharing with H, the wavenumber of the HS-stretching mode of HSCS in solid p-H (2477.2 cm) is similar to the anharmonic wavenumber of HSCS (2424 cm) predicted with the B3LYP/aug-cc-pVTZ method, indicating that the sharing of a proton between HSCS and neighboring H molecules is insignificant.