Adoptive-optics-assisted integral field spectroscopy with OASIS and NAOMI
被引:4
作者:
McDermid, R
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机构:
Leiden Univ, NL-2300 RA Leiden, NetherlandsLeiden Univ, NL-2300 RA Leiden, Netherlands
McDermid, R
[1
]
Bacon, R
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机构:
Leiden Univ, NL-2300 RA Leiden, NetherlandsLeiden Univ, NL-2300 RA Leiden, Netherlands
Bacon, R
[1
]
Adam, G
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机构:
Leiden Univ, NL-2300 RA Leiden, NetherlandsLeiden Univ, NL-2300 RA Leiden, Netherlands
Adam, G
[1
]
Benn, C
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机构:
Leiden Univ, NL-2300 RA Leiden, NetherlandsLeiden Univ, NL-2300 RA Leiden, Netherlands
Benn, C
[1
]
Cappellari, M
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机构:
Leiden Univ, NL-2300 RA Leiden, NetherlandsLeiden Univ, NL-2300 RA Leiden, Netherlands
Cappellari, M
[1
]
机构:
[1] Leiden Univ, NL-2300 RA Leiden, Netherlands
来源:
GROUND-BASED INSTRUMENTATION FOR ASTRONOMY, PTS 1-3
|
2004年
/
5492卷
关键词:
integral-field spectroscopy;
adaptive optics;
galaxy evolution;
black holes;
kinematics;
D O I:
10.1117/12.552912
中图分类号:
V [航空、航天];
学科分类号:
08 ;
0825 ;
摘要:
By incorporating spatial coverage with the spectral dimension, integral-field spectroscopy is uniquely suited for exploiting the capabilities of adaptive optics (AO) systems. OASIS is a lenslet-based integral-field spectrograph designed to perform high-resolution observations on AO-corrected sources, operating at visible wavelengths. This instrument was commissioned at the William Herschel Telescope, La Palma, in July 2003 to work with the ING's AO system, NAOMI. Here we present an overview of the capabilities of the OASIS+NAOMI system, and show results obtained using this technique. The science presented here is a small preview of what will be possible for a large number of objects when the GLAS laser guide system is operational.