For theoretical work, we use the Stampede supercomputer at the Texas Advanced Computing Center (TACC). This NSF-supported community facility provides the computing power behind our Asteroseismic Modeling Portal (AMP). We are currently updating AMP to utilize the MESA stellar evolution code with GYRE for non-adiabatic oscillations. |
For observational work, we use data from the Las Cumbres Observatory Global Telescope (LCOGT) network, 21 robotic telescopes at 8 sites around the world working together as a single instrument. Community access to this facility is currently organized through the National Optical Astronomy Observatory (NOAO) with support from NSF. |