fitting lines in spectra

In between various writing projects, Wu and I inspected and modified some of her fits of emission lines in our Spitzer spectroscopy of SDSS galaxies. We also had a chat with Schiminovich about them. Wu's project is to understand the mid-infrared and optical lines in general, and also assess whether we can use them to measure the abundances of molecular hydrogen from its direct line emission.

No comments:

Post a Comment