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Volumn 50, Issue 4-5, 2006, Pages 392-397

A scientific overview of requirements for IFU data reduction and analysis

Author keywords

Instrumentation: spectrographs; Methods: data analysis

Indexed keywords


EID: 33744920589     PISSN: 13876473     EISSN: None     Source Type: Journal    
DOI: 10.1016/j.newar.2006.02.007     Document Type: Review
Times cited : (2)

References (9)
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  • 2
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    • Differential atmospheric refraction in integral-field spectroscopy: effects and correction
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    • (1999) A&AS , vol.136 , pp. 189-192
    • Arribas, S.1    Mediavilla, E.2    García-Lorenzo, B.3    del Burgo, C.4    Fuensalida, J.J.5
  • 3
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    • Adaptive spatial binning of integral-field spectroscopic data using Voronoi tessellations
    • Cappellari M., and Copin Y. Adaptive spatial binning of integral-field spectroscopic data using Voronoi tessellations. MNRAS 342 (2003) 345-354
    • (2003) MNRAS , vol.342 , pp. 345-354
    • Cappellari, M.1    Copin, Y.2
  • 4
    • 33645069672 scopus 로고    scopus 로고
    • GMOS IFU observations of the stellar and gaseous kinematics in the centre of NGC 1068
    • Gerssen J., Allington-Smith J.R., Miller B.W., Turner J.E.H., and Walker A. GMOS IFU observations of the stellar and gaseous kinematics in the centre of NGC 1068. MNRAS 365 (2005) 29
    • (2005) MNRAS , vol.365 , pp. 29
    • Gerssen, J.1    Allington-Smith, J.R.2    Miller, B.W.3    Turner, J.E.H.4    Walker, A.5
  • 5
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    • Microslit nod-shuffle spectroscopy: a technique for achieving very high densities of spectra
    • Glazebrook K., and Bland-Hawthorn J. Microslit nod-shuffle spectroscopy: a technique for achieving very high densities of spectra. PASP 113 (2001) 197-214
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    • Glazebrook, K.1    Bland-Hawthorn, J.2
  • 7
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    • Turner, J.E.H. 2001. Astronomy with integral field spectroscopy: observation, data analysis and results, Ph.D., University of Durham.
  • 8
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    • Turner, J.E.H. 2005. Support for IFU data in the Gemini IRAF package. In: Proceedings of the ING Workshop on AO-assisted IFS. NewAR, 49, 655.


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.