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Proceedings Paper

X-ray Lobster Eye all-sky monitor for rocket experiment
Author(s): V. Dániel; A. Inneman; L. Pína; V. Zadražil; T. Báča; V. Stehlíková; O. Nentvich; M. Urban; V. Maršíková; R. McEntaffer; J. Tutt; T. Schulz
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Paper Abstract

This paper presents a Lobster Eye (LE) X-ray telescope developed for the Water Recovery X-ray Rocket (WRX-R) experiment. The primary payload of the rocket experiment is a soft X-ray spectroscope developed by the Pennsylvania State University (PSU), USA. The Czech team participates by hard LE X-ray telescope as a secondary payload. The astrophysical objective of the rocket experiment is the Vela Supernova of size about 8deg x 8deg. In the center of the nebula is a neutron star with a strong magnetic field, roughly the mass of the Sun and a diameter of about 20 kilometers forming the Vela pulsar.

The primary objective of WRX-R is the spectral measurement of the outer part of the nebula in soft X-ray and FOV of 3.25deg x 3.25deg. The secondary objective (hard LE X-ray telescope) is the Vela neutron star observation. The hard LE telescope consists of two X-ray telescopes with the Timepix detector. First telescope uses 2D LE Schmidt optics (2DLE- REX) with focal length over 1m and 4 Timepix detectors (2x2 matrix). The telescope FOV is 1.5deg x 1.5deg with spectral range from 3keV to 60keV. The second telescope uses 1D LE Schmidt optics (1D-LE-REX) with focal length of 25 cm and one Timepix detector. The telescope is made as a wide field with FOV 4.5deg x 3.5deg and spectral range from 3keV to 40keV. The rocket experiment serves as a technology demonstration mission for the payloads. The LE X-ray telescopes can be in the future used as all‐sky monitor/surveyor. The astrophysical observation can cover the hard X-ray observation of astrophysical sources in time-domain, the GRBs surveying or the exploration of the gravitational wave sources.

Paper Details

Date Published: 31 May 2017
PDF: 7 pages
Proc. SPIE 10235, EUV and X-ray Optics: Synergy between Laboratory and Space V, 1023503 (31 May 2017); doi: 10.1117/12.2277515
Show Author Affiliations
V. Dániel, Aerospace Research and Test Establishment (Czech Republic)
A. Inneman, Rigaku Innovative Technologies Europe (Czech Republic)
Czech Technical Univ. in Prague (Czech Republic)
L. Pína, Rigaku Innovative Technologies Europe (Czech Republic)
Czech Technical Univ. in Prague (Czech Republic)
V. Zadražil, Aerospace Research and Test Establishment (Czech Republic)
T. Báča, Czech Technical Univ. in Prague (Czech Republic)
V. Stehlíková, Czech Technical Univ. in Prague (Czech Republic)
O. Nentvich, Czech Technical Univ. in Prague (Czech Republic)
M. Urban, Czech Technical Univ. in Prague (Czech Republic)
V. Maršíková, Rigaku Innovative Technologies Europe (Czech Republic)
Czech Technical Univ. in Prague (Czech Republic)
R. McEntaffer, Pennsylvania State Univ. (United States)
J. Tutt, Pennsylvania State Univ. (United States)
T. Schulz, Pennsylvania State Univ. (United States)


Published in SPIE Proceedings Vol. 10235:
EUV and X-ray Optics: Synergy between Laboratory and Space V
René Hudec; Ladislav Pina, Editor(s)

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