Abstract
The Advanced Compton Telescope (ACT), the next major step in gamma-ray astronomy, will probe the fires where chemical elements are formed by enabling high-resolution spectroscopy of nuclear emission from supernova explosions. During the past two years, our collaboration has been undertaking a NASA mission concept study for ACT. This study was designed to (1) transform the key scientific objectives into specific instrument requirements, (2) to identify the most promising technologies to meet those requirements, and (3) to design a viable mission concept for this instrument. We present the results of this study, including scientific goals and expected performance, mission design, and technology recommendations.
Original language | English (US) |
---|---|
Title of host publication | Space Telescopes and Instrumentation II |
Subtitle of host publication | Ultraviolet to Gamma Ray |
DOIs | |
State | Published - 2006 |
Event | Space Telescopes and Instrumentation II: Ultraviolet to Gamma Ray - Orlando, FL, United States Duration: May 24 2006 → May 31 2006 |
Publication series
Name | Proceedings of SPIE - The International Society for Optical Engineering |
---|---|
Volume | 6266 II |
ISSN (Print) | 0277-786X |
Other
Other | Space Telescopes and Instrumentation II: Ultraviolet to Gamma Ray |
---|---|
Country/Territory | United States |
City | Orlando, FL |
Period | 5/24/06 → 5/31/06 |
Keywords
- Gamma-ray astronomy
- Gamma-ray imaging
- Gamma-ray spectrometry
- High energy astrophysics
- Satellite missions
- X-ray/gamma-ray detectors
ASJC Scopus subject areas
- Electronic, Optical and Magnetic Materials
- Condensed Matter Physics
- Computer Science Applications
- Applied Mathematics
- Electrical and Electronic Engineering