posted on 2016-12-07, 15:35authored byMartin A. Barstow, Nigel P. Bannister, R. G. Cruddace, M. P. Kowalski, K. S. Wood, D. J. Yentis, H. Gursky, T. W. Barbee, W. H. Goldstein, J. F. Kordas, G. G. Fritz, J. L. Culhane, J. S. Lapington
We report on the successful sounding rocket flight of the high resolution (R=3000-4000) J-PEX EUV spectrometer. J-PEX is a novel normal incidence instrument, which combines the focusing and dispersive elements of the spectrometer into a single optical element, a multilayer-coated grating. The high spectral resolution achieved has had to be matched by unprecedented high spatial resolution in the imaging microchannel plate detector used to record the data. We illustrate the performance of the complete instrument through an analysis of the 220-245Å spectrum of the white dwarf G191-B2B obtained with a 300 second exposure. The high resolution allows us to detect a low-density ionized helium component along the line of sight to the star and individual absorption lines from heavier elements in the photosphere.
Funding
The University of Leicester and the Mullard Space Science Laboratory acknowledge the support they received for
this project from the Particle Physics and Astronomy Research Council in the UK. The Naval Research Laboratory
(NRL) was supported by NASA in this work, under grant NDPR S-47440F, and by the Office of Naval Research
under NRL work unit 3641 (Application of Multilayer Coated Optics to Remote Sensing).
History
Citation
Proceedings of SPIE 4854, Future EUV/UV and Visible Space Astrophysics Missions and Instrumentation, 654 (February 26, 2003);
Author affiliation
/Organisation/COLLEGE OF SCIENCE AND ENGINEERING/Department of Physics and Astronomy
Source
Conference on Future EUV/UV and Visible Space Astrophysics Missions and Instrumentation, WAIKOLOA, HI
Version
AM (Accepted Manuscript)
Published in
Proceedings of SPIE 4854
Publisher
Society of Photo-optical Instrumentation Engineers (SPIE)