Integral-field spectroscopy at the resolution limit of large telescopes: The science program of OSIRIS at keck

Proceedings of SPIE - The International Society for Optical Engineering

Volumn 4841, Issue 3, 2002, Pages 1493-1502

  Quirrenbach, A ^a   Larkin, J E ^b   Krabbe, A ^c   Barczys, M ^b   LaFreniere, D ^b  

^a UNIVERSITY OF CALIFORNIA   (United States)

^b UNIVERSITY OF CALIFORNIA   (United States)

^c UNIVERSITY OF CALIFORNIA   (United States)

Author keywords

Active galactic nuclei; Adaptive optics; Galaxies; Integral field spectroscopy; Near infrared; OH suppression; Planets; Spectrographs; Star formation; Stellar clusters

Indexed keywords

ADAPTIVE OPTICS; INFRARED RADIATION; PLANETS; SPECTROGRAPHS; SPECTROSCOPIC ANALYSIS;

INTEGRAL-FIELD SPECTROSCOPY;

TELESCOPES;

EID: 0037737938     PISSN: 0277786X     EISSN: None     Source Type: Conference Proceeding    
DOI: 10.1117/12.461445     Document Type: Conference Paper

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