Observation of He-like Satellite Lines of the H-like Potassium K xix Emission
Author(s) -
M. E. Weller,
P. Beiersdörfer,
T. Lockard,
G. V. Brown,
Andrew McKelvey,
Joseph Nilsen,
R. Shepherd,
V. Soukhanovskii,
M. P. Hill,
L. M. R. Hobbs,
D. Burridge,
D. J. Hoarty,
John Morton,
L. A. Wilson,
S. J. Rose,
Peter Hatfield
Publication year - 2019
Publication title -
the astrophysical journal
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.376
H-Index - 489
eISSN - 1538-4357
pISSN - 0004-637X
DOI - 10.3847/1538-4357/ab2dff
Subject(s) - physics , satellite , wavelength , spectrometer , emission spectrum , astrophysics , atomic physics , spectral line , astronomy , optics
We present measurements of the H-like potassium (K xix) X-ray spectrum and its He-like (K xviii) satellite lines, which are situated in the wavelength region between 3.34 and 3.39 A, which has been of interest for the detection of dark matter. The measurements were taken with a high-resolution X-ray spectrometer from targets irradiated by a long-pulse (2 ns) beam from the Orion laser facility. We obtain experimental wavelength values of dielectronic recombination satellite lines and show that the ratio of the Lyα lines and their dielectronic satellite lines can be used to estimate the electron temperature, which in our case was about 1.5 ± 0.3 keV.
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