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Spectroscopy in the vacuum-ultraviolet

Spectroscopy in the vacuum-ultraviolet correspondence De Oliveira et al. reply: First, we would 20 nm (~60 eV). Note that scanning that not only has unprecedented resolving like to apologize for not mentioning control could be achieved by exactly the power and multiplex wavelength the results presented by Agåker et al. same system as in the present instrument. detection, but also is available to a large 2 9,10 in our recently published Letter . Provided that the optical elements meet user community for investigating Although we mentioned the theoretical the tight optical specifications required photoabsorption processes involving 3 4 study of Yin et al. in a previous paper , to reach such a wavelength, the expected valence and inner-valence shell excitation we were unaware of these recent resolving power would be, as in the present in the vacuum-ultraviolet range. This range experimental achievements. vacuum-ultraviolet instrument, in the 10 is of great interest to those conducting Agåker et al. raise some interesting range. This could be used, for example, to research in astrophysics and upper- points that we would like to clarify here. provide data on doubly excited helium. atmosphere-related sciences. ❐ Concerning the reflectivity of the roof- Another challenge is linked with the References http://www.deepdyve.com/assets/images/DeepDyve-Logo-lg.png Nature Photonics Springer Journals

Spectroscopy in the vacuum-ultraviolet

Spectroscopy in the vacuum-ultraviolet

Abstract

correspondence De Oliveira et al. reply: First, we would 20 nm (~60 eV). Note that scanning that not only has unprecedented resolving like to apologize for not mentioning control could be achieved by exactly the power and multiplex wavelength the results presented by Agåker et al. same system as in the present instrument. detection, but also is available to a large 2 9,10 in our recently published Letter . Provided that the optical elements meet user community for investigating Although...
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References (10)

Publisher
Springer Journals
Copyright
Copyright © Springer Nature Limited 2011
Subject
Physics; Physics, general; Applied and Technical Physics; Quantum Physics
ISSN
1749-4885
eISSN
1749-4893
DOI
10.1038/nphoton.2011.59
Publisher site
See Article on Publisher Site

Abstract

correspondence De Oliveira et al. reply: First, we would 20 nm (~60 eV). Note that scanning that not only has unprecedented resolving like to apologize for not mentioning control could be achieved by exactly the power and multiplex wavelength the results presented by Agåker et al. same system as in the present instrument. detection, but also is available to a large 2 9,10 in our recently published Letter . Provided that the optical elements meet user community for investigating Although we mentioned the theoretical the tight optical specifications required photoabsorption processes involving 3 4 study of Yin et al. in a previous paper , to reach such a wavelength, the expected valence and inner-valence shell excitation we were unaware of these recent resolving power would be, as in the present in the vacuum-ultraviolet range. This range experimental achievements. vacuum-ultraviolet instrument, in the 10 is of great interest to those conducting Agåker et al. raise some interesting range. This could be used, for example, to research in astrophysics and upper- points that we would like to clarify here. provide data on doubly excited helium. atmosphere-related sciences. ❐ Concerning the reflectivity of the roof- Another challenge is linked with the References

Journal

Nature PhotonicsSpringer Journals

Published: May 1, 2011

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