Biosignature Anisotropy Modeled on Temperate Tidally Locked M-dwarf Planets

Howard Chen, Eric T. Wolf, Ravi Kopparapu +2

A planet's atmospheric constituents (e.g., O${}_2$, O${}_3$, H${}_2$O${}_v$, CO${}_2$, CH${}_4$, N${}_2$O) can provide clues to its surface habitability, and may offer biosignature targets for r…