Antarctica – a case for 3D-spectroscopy

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 an...

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Bibliographic Details
Published in:Proceedings of the International Astronomical Union
Main Author: Kelz, Andreas
Format: Article in Journal/Newspaper
Language:English
Published: Cambridge University Press (CUP) 2006
Subjects:
Astronomy and Astrophysics
Space and Planetary Science
Antarc*
Antarctica
Online Access:http://dx.doi.org/10.1017/s1743921307012355
https://www.cambridge.org/core/services/aop-cambridge-core/content/view/S1743921307012355
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spelling crcambridgeupr:10.1017/s1743921307012355 2023-05-15T14:12:50+02:00 Antarctica – a case for 3D-spectroscopy Kelz, Andreas 2006 http://dx.doi.org/10.1017/s1743921307012355 https://www.cambridge.org/core/services/aop-cambridge-core/content/view/S1743921307012355 en eng Cambridge University Press (CUP) https://www.cambridge.org/core/terms Proceedings of the International Astronomical Union volume 2, issue 14, page 707-708 ISSN 1743-9213 1743-9221 Astronomy and Astrophysics Space and Planetary Science journal-article 2006 crcambridgeupr https://doi.org/10.1017/s1743921307012355 2022-04-07T08:08:09Z 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). Article in Journal/Newspaper Antarc* Antarctica Cambridge University Press (via Crossref) Proceedings of the International Astronomical Union 2 14 707 708
institution Open Polar
collection Cambridge University Press (via Crossref)
op_collection_id crcambridgeupr
language English
topic Astronomy and Astrophysics
Space and Planetary Science
spellingShingle Astronomy and Astrophysics
Space and Planetary Science
Kelz, Andreas
Antarctica – a case for 3D-spectroscopy
topic_facet Astronomy and Astrophysics
Space and Planetary Science
description 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).
format Article in Journal/Newspaper
author Kelz, Andreas
author_facet Kelz, Andreas
author_sort Kelz, Andreas
title Antarctica – a case for 3D-spectroscopy
title_short Antarctica – a case for 3D-spectroscopy
title_full Antarctica – a case for 3D-spectroscopy
title_fullStr Antarctica – a case for 3D-spectroscopy
title_full_unstemmed Antarctica – a case for 3D-spectroscopy
title_sort antarctica – a case for 3d-spectroscopy
publisher Cambridge University Press (CUP)
publishDate 2006
url http://dx.doi.org/10.1017/s1743921307012355
https://www.cambridge.org/core/services/aop-cambridge-core/content/view/S1743921307012355
genre Antarc*
Antarctica
genre_facet Antarc*
Antarctica
op_source Proceedings of the International Astronomical Union
volume 2, issue 14, page 707-708
ISSN 1743-9213 1743-9221
op_rights https://www.cambridge.org/core/terms
op_doi https://doi.org/10.1017/s1743921307012355
container_title Proceedings of the International Astronomical Union
container_volume 2
container_issue 14
container_start_page 707
op_container_end_page 708
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