Abstract
The Advanced Compton Telescope (ACT), the next major step in γ-ray astronomy, will probe the fires where chemical elements are formed by enabling high resolution spectroscopy of nuclear emission from supernova explosions. ACT requires two orders of magnitude improvement in sensitivity over current gamma- ray observatories to achieve this goal, and will operate primarily in survey mode – covering 80% of the sky on every orbit. ACT will also enable new classes of compact object and GRB observations, including all-sky monitoring for transients and rapid localizations, high resolution spectra, high sensitivity to positron annihilation emission and other line features, and novel sensitivity to polarization. ACT was chosen by NASA for a 1-year Vision Mission concept study, with the primary goals of identifying the key technologies and developing the detailed mission concept. We discuss the scientific goals and capabilities of ACT, and an overview of the science mission.
Sign-in/Register to access full text options 
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Schedule a callDisclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.
