Optical Sensor Development for Astrophysics
Develop optical sensors for astrophysics, combining nano-fabrication and observational astronomy to study variables and transients using multi-spectral imaging and more.
This grant is no longer accepting proposals
NRC Research Associateship Programs has archived this opportunity.
Funder: NRC Research Associateship Programs
Due Dates: February 1, 2025 | May 1, 2025 | August 1, 2025 | November 1, 2025
Funding Amounts: Stipend approximately $99,200 per year with $3,000 travel allowance; typical tenure 2-3 years.
Summary: Postdoctoral fellowship to develop advanced optical and ultraviolet sensors for astrophysics, combining nano-fabrication and observational astronomy to study astrophysical variables and transient sources.
Key Information: Open to U.S. citizens and permanent residents; requires contacting a Research Adviser prior to application; relocation and health insurance benefits included.
Description
This NRC Research Associateship Program opportunity at the Naval Research Laboratory (NRL) focuses on the development of optical and ultraviolet sensors for astrophysics applications. The program integrates nano-fabrication techniques with observational astrophysics to create sensors capable of multi-spectral imaging, polarization measurements, and high-timing resolution. These sensors aim to characterize astrophysical variables and transient sources such as galactic and extragalactic phenomena.
Candidates may engage in all stages of research including design, fabrication, data acquisition, and analysis. Nano-fabrication work involves the use of the NRL NanoScience Institute (NSI) facilities to produce focal plane devices such as Fabry-Perot etalons and on-chip micropolarizers, as well as flat lens optics operating across infrared, optical, and ultraviolet wavelengths. Techniques include electron beam lithography and metal reactive ion etching. While experience in these methods is desirable, it is not mandatory as associates can gain skills during tenure.
On the observational side, research includes monitoring and characterizing galactic and extragalactic variables and transients using spectroscopy, multi-band photometry, and polarimetry. Candidates will have opportunities to test prototype devices and commercially available sensors mounted on small telescopes (8-inch to 16-inch), with an emphasis on remote operation.
