
PI: Paul Scowen (ASU)
Last Updated: April 22, 2009
The Star Formation Camera (SFC) is a wide-field (~15'x19', >~280 arcmin^2), high-resolution (18x18 mas pixels) UV/optical dichroic camera for a 4-m space-based telescope concept. SFC will deliver diffraction-limited images at lambda > 300 nm in both a Blue (190--517nm) and a Red (517--1075nm) Channel simultaneously. Our aim is to conduct a comprehensive and systematic study of the astrophysical processes and environments relevant for the births and life cycles of stars and their planetary systems, and to investigate and understand the range of environments, feedback mechanisms, and other factors that most affect the outcome of the star and planet formation process. We present the design and performance specifications resulting from an implementation study of the camera. The result is a lightweight, low-cost instrument that will provide deep, high-resolution imaging across a wide angular field enabling a wide variety of community science as well as completing the core science that drives the design of the camera. The technology associated with the camera is next generation but still relatively high TRL, allowing a low-risk solution with moderate technology development investment over the next 10 years.
Science Whitepapers Submitted to the 2010 NAS Decadal Survey on Astronomy and Astrophysics that support the SFC concept:
Technology and Mission Activity Whitepapers also submitted to the Decadal Survey as part of this work:
Appendices to the Final Report submitted to NASA April 24, 2009 on the results of the instrument study:
Mission Design Poster Papers presented at the 213th Meeting of the AAS in Long Beach, CA, Jan 4-8, 2009: