HAWC+ for SOFIA: Two Years of Flying, and First Science Results

I first give a brief summary of instrument activities since the last HAWC+ tele-talk in January 2017, including the acceptance as a facility by NASA.  The rest of the talk focuses on the ongoing analysis and interpretation of GTO science data.  Featured topics include the fine-scale magnetic field structure of the Orion Molecular Cloud, dust grain alignment, the magnetic field in the Galactic center Circum-Nuclear Ring, and extragalactic polarimetry.