Interesting survey images will be posted here as they become available.

Thermal infrared emission from starlight-heated dust particles in the gas I-GALFA will observe. IRIS 100 micron brightness (Miville-Deschênes & Lagache 2005) is shown on a logarithmic intensity scale from 1 to 105 MJy sr-1. The red and yellow emission is in from dust near the Galactic plane; the blank area was not observed. The red lines mark I-GALFA survey boundaries.

We are currently working on H I maps of our first survey field. Stay tuned!