Metal Pipe

Metal Pipe is a code for determining stellar parameters and abundances, which is designed for use across a wider range of spectral types than many commonly used codes. It combines the widely-used package MOOG with photometric stellar parameters, a user-supplied high-resolution spectrum, and a newly curated list of spectral lines. Metal Pipe outputs values for Teff , log (g), M∗, R∗, and L∗ from isochrones, and abundances of C, O, Na, Mg, Al, Si, S, Ca, Ti, and Fe from MOOG.