Technology requirements for a square meter, arcsecond resolution telescope for x-rays: the SMART-X mission

Daniel A. Schwartz; Ryan Allured; Jay A. Bookbinder; Vincenzo Cotroneo; William R. Forman; Mark D. Freeman; Stuart McMuldroch; Paul B. Reid; Harvey Tananbaum; Alexey A. Vikhlinin; Raegan L. Johnson-Wilke; Susan E. Trolier-McKinstry; Rudeger H. T. Wilke; Thomas N Jackson; J. Israel Ramirez; Mikhail V. Gubarev; Jeffery J. Kolodziejczak; Stephen L. O'Dell; Brian D. Ramsey

doi:10.1117/12.2063469

17 September 2014 Technology requirements for a square meter, arcsecond resolution telescope for x-rays: the SMART-X mission

Daniel A. Schwartz, Ryan Allured, Jay A. Bookbinder, Vincenzo Cotroneo, William R. Forman, Mark D. Freeman, Stuart McMuldroch, Paul B. Reid, Harvey Tananbaum, Alexey A. Vikhlinin, Raegan L. Johnson-Wilke, Susan E. Trolier-McKinstry, Rudeger H. T. Wilke, Thomas N Jackson, J. Israel Ramirez, Mikhail V. Gubarev, Jeffery J. Kolodziejczak, Stephen L. O'Dell, Brian D. Ramsey

Author Affiliations +

Proceedings Volume 9208, Adaptive X-Ray Optics III; 920806 (2014) https://doi.org/10.1117/12.2063469
Event: SPIE Optical Engineering + Applications, 2014, San Diego, California, United States

Abstract

Addressing the astrophysical problems of the 2020’s requires sub-arcsecond x-ray imaging with square meter effective area. Such requirements can be derived, for example, by considering deep x-ray surveys to find the young black holes in the early universe (large redshifts) which will grow into the first super-massive black holes. We have envisioned a mission, the Square Meter Arcsecond Resolution Telescope for X-rays (SMART-X), based on adjustable x-ray optics technology, incorporating mirrors with the required small ratio of mass to collecting area. We are pursuing technology which achieves sub-arcsecond resolution by on-orbit adjustment via thin film piezoelectric “cells” deposited directly on the non-reflecting sides of thin, slumped glass. While SMART-X will also incorporate state-of-the-art x-ray cameras, the remaining spacecraft systems have no requirements more stringent than those which are well understood and proven on the current Chandra X-ray Observatory.

Citation Download Citation

Daniel A. Schwartz, Ryan Allured, Jay A. Bookbinder, Vincenzo Cotroneo, William R. Forman, Mark D. Freeman, Stuart McMuldroch, Paul B. Reid, Harvey Tananbaum, Alexey A. Vikhlinin, Raegan L. Johnson-Wilke, Susan E. Trolier-McKinstry, Rudeger H. T. Wilke, Thomas N Jackson, J. Israel Ramirez, Mikhail V. Gubarev, Jeffery J. Kolodziejczak, Stephen L. O'Dell, and Brian D. Ramsey "Technology requirements for a square meter, arcsecond resolution telescope for x-rays: the SMART-X mission", Proc. SPIE 9208, Adaptive X-Ray Optics III, 920806 (17 September 2014); https://doi.org/10.1117/12.2063469

ACCESS THE FULL ARTICLE

INSTITUTIONAL
Select your institution to access the SPIE Digital Library.

SELECT YOUR INSTITUTION

PERSONAL
Sign in with your SPIE account to access your personal subscriptions or to use specific features such as save to my library, sign up for alerts, save searches, etc.

PERSONAL SIGN IN

No SPIE Account? Create one

PURCHASE THIS CONTENT

SUBSCRIBE TO DIGITAL LIBRARY

50 downloads per 1-year subscription

Members: $195

Non-members: $335 ADD TO CART

25 downloads per 1 - year subscription

Members: $145

Non-members: $250 ADD TO CART

PURCHASE SINGLE ARTICLE

Includes PDF, HTML & Video, when available