An X-ray interferometry concept for the ESA Voyage 2050 programme
The result's identifiers
Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F21%3A00549987" target="_blank" >RIV/67985815:_____/21:00549987 - isvavai.cz</a>
Result on the web
<a href="http://dx.doi.org/10.1117/12.2562523" target="_blank" >http://dx.doi.org/10.1117/12.2562523</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1117/12.2562523" target="_blank" >10.1117/12.2562523</a>
Alternative languages
Result language
angličtina
Original language name
An X-ray interferometry concept for the ESA Voyage 2050 programme
Original language description
We have proposed the development of X-ray interferometry as part of ESA's Voyage 2050 programme, to reveal the universe at high energies with ultra-high spatial resolution. With only a 1 m baseline, which could be accommodated on a single spacecraft, X-ray interferometry can reach 100 mu as resolution at 10 angstrom (1.24 keV) and exceed that of the Event Horizon Telescope at 2 angstrom (6.2 keV). A multi-spacecraft 'constellation' interferometer would resolve well below 1 mu as. Here we focus on the single-spacecraft interferometer design and discuss the process of fringe detection and image reconstruction from multiple baselines, showing simulated images of test cases from our Voyage 2050 White Paper. We also discuss the challenges and feasibility of reaching the technical requirements needed for a single-spacecraft interferometer. Most key requirements are already feasible or within easy reach. Besides a ground-based testbed, covered elsewhere in these proceedings, the most important areas for development include large format, small-pixel X-ray detectors and pointing which is stable or can be reconstructed to tens of mu as precision.
Czech name
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Czech description
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Classification
Type
D - Article in proceedings
CEP classification
—
OECD FORD branch
10308 - Astronomy (including astrophysics,space science)
Result continuities
Project
—
Continuities
I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace
Others
Publication year
2021
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů
Data specific for result type
Article name in the collection
Space Telescopes and Instrumentation 2020: Ultraviolet to Gamma Ray
ISBN
978-1-5106-3676-7
ISSN
1996-756X
e-ISSN
1996-756X
Number of pages
17
Pages from-to
114441E
Publisher name
SPIE
Place of publication
Bellingham
Event location
online
Event date
Dec 14, 2020
Type of event by nationality
WRD - Celosvětová akce
UT code for WoS article
000674737700015