Status of the Stratospheric Observatory for Infrared Astronomy (SOFIA)
R. D. Gehrz, E. E. Becklin, J. de Buizer, T. Herter, L. D. Keller, A., Krabbe, P. M. Marcum, T. L. Roellig, G. H. L. Sandell, P. Temi, W. D. Vacca,, E. T. Young, and H. Zinnecker

TL;DR
SOFIA is a joint U.S./German airborne infrared observatory on a Boeing 747, capable of high-altitude observations from 0.3 μm to 1.6 mm, with ongoing operations and diverse scientific instruments since 2010.
Contribution
This paper provides a comprehensive overview of SOFIA's status, instrumentation, operational capabilities, and initial scientific results, highlighting its unique airborne infrared observation platform.
Findings
First light images obtained at wavelengths from 5.4 to 37 μm.
Operational status and instrument performance summarized.
Future observation opportunities outlined.
Abstract
The Stratospheric Observatory for Infrared Astronomy (SOFIA), a joint U.S./German project, is a 2.5-meter infrared airborne telescope carried by a Boeing 747-SP that flies in the stratosphere at altitudes as high as 45,000 feet (13.72 km). This facility is capable of observing from 0.3 {\mu}m to 1.6 mm with an average transmission greater than 80 percent. SOFIA will be staged out of the NASA Dryden Flight Research Center aircraft operations facility at Palmdale, CA. The SOFIA Science Mission Operations (SMO) will be located at NASA Ames Research Center, Moffett Field, CA. First science flights began in 2010 and a full operations schedule of up to one hundred 8 to 10 hour flights per year will be reached by 2014. The observatory is expected to operate until the mid 2030's. SOFIAs initial complement of seven focal plane instruments includes broadband imagers, moderate-resolution…
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