No CrossRef data available.
Article contents
Antarctica – a case for 3D-spectroscopy
Published online by Cambridge University Press: 01 August 2006
Extract
Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.
DS or Integral-Field Spectroscopy (IFS) provides multiple spectra for each point of a 2-D field, rather than along a narrow, 1-D spectrograph slit only. Therefore, IFS does not require very accurate telescope pointing, nor do pre-assumptions about slit or aperture sizes have to be made. It avoids any ‘slit-losses’ due to seeing or atmospheric dispersion, which eliminates the need for any parallactic alignment or a dispersion compensator (see Fig. 1).
- Type
- Contributed Papers
- Information
- Proceedings of the International Astronomical Union , Volume 2 , Highlights of Astronomy 14: Highlights of Astronomy , August 2006 , pp. 707 - 708
- Copyright
- Copyright © International Astronomical Union 2007
References
Ashley, M. C. B., Burton, M. G., Lawrence, J. S., & Storey, J. W. V. 2004, AN, 325, 619Google Scholar
You have
Access