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Our objective is to develop techniques to manufacture x-ray telescopes with five characteristics: high angular resolution, high throughput, light weight, low cost, and efficient production. Two independent technologies are in development. We have pioneered an epoxy replication technique that enabled the manufacture of the lightweight, high throughput optics that flew on ASCA and Suzaku. We are improving this technology further to enable both better angular resolution and higher throughput for the upcoming Astro-H mission, scheduled for launch in 2014. We have also pioneered a precision glass mirror forming technique that we have used for manufacturing the mirrors for the upcoming NuSTAR mission, scheduled for launch in 2012. We are developing the glass mirror technology and a corresponding alignment and integration technology to meet the 5 arc-second angular resolution requirement of the International X‑ray Observatory. We have the laboratory and engineering resources for making, measuring, and testing high quality x-ray mirrors to advance these technologies for missions in this decade as well as future missions with unprecedented angular resolution (better than 0.5 arc‑seconds) and photon collection areas (larger than one square meter). We seek postdoctoral fellows interested in working on state‑of‑the‑art x-ray optics.
Goddard Space Flight Center, Greenbelt, Maryland
Astrophysics
11/1/2026 6:00:59 PM Eastern Time Zone
Applications with citizens from Designated Countries will not be accepted at this time, unless they are Legal Permanent Residents of the United States.
Eligibility is currently open to:
Please email npp@orau.org
Mikeala