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Antarctica – a case for 3D-spectroscopy

Published online by Cambridge University Press:  01 August 2006

Andreas Kelz*
Affiliation:
Astrophysikalisches Institut Potsdam, An der Sternwarte 16, D-14482 Potsdam, Germany email: akelz@aip.de
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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
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
Becker, T., Fabrika, S., & Roth, M. M. 2004, AN, 325, 155Google Scholar
Bland-Hawthorn, J. 2006, New Astron. Revs., 50, 237CrossRefGoogle Scholar
Burton, M. G., Lawrence, J. S., Ashley, M. C. B., et al. 2005, PASA, 22, 199CrossRefGoogle Scholar
Kelz, A., & Roth, M. M. 2006, New Astron. Revs., 50, 355CrossRefGoogle Scholar
Kelz, A., Verheijen, M., Roth, M. M., et al. 2006, PASP, 118, 129CrossRefGoogle Scholar
Kelz, A. 2004, AN, 325, 673Google Scholar
Roth, M. M., Kelz, A., Fechner, T. et al. 2005, PASP, 117, 620CrossRefGoogle Scholar
Roth, M. M., Becker, T., Kelz, A., & Schmoll, J. 2004, ApJ, 603, 531CrossRefGoogle Scholar
Roth, M. M., Fechner, T., Wolter, D., et al. 2002, Exp. Astron., 14, 99CrossRefGoogle Scholar
Storey, J. W. V., Ashley, M. C. B., Burton, M. G., & Lawrence, J. 2005, EAS-PS, 14, 7Google Scholar