The infrared (IR) astronomy program includes observations of astronomical sources between approximately 1 and 200 micrometers using both spectroscopic and broadband instruments, as well as multiwavelength observations and analysis for understanding the formation and evolution of stars, planets, and galaxies and their associated central black holes, as well as the infrared cosmic background. This program includes observations from ground-based telescopes and from airborne or spacecraft platforms, as well as the development of instrumentation. Current programs are 5-200 micron spectroscopy of infrared-bright galaxies, near- and mid-infrared spectroscopy of young stars and protoplanetary disks, modeling of emission lines from accretion disks, and abundance analysis of late-type stars. We encourage participation in national and international collaborations and the use of all national and international observing facilities, ground- and space-based, at IR and other wavelengths.

Additional Benefits

Awardees who reside more than 50 miles from their host laboratory and remain on tenure for at least six months are eligible for paid relocation to within the vicinity of their host laboratory.

A group health insurance program is available to awardees and their qualifying dependents in the United States.