Using adaptive optics to probe the dynamics and star formation in active galactic nuclei

Proceedings of SPIE - The International Society for Optical Engineering

Volumn 5490, Issue PART 1, 2004, Pages 473-482

  Davies, Richard ^a   Tacconi, Linda ^a   Genzel, Reinhard ^a   Ott, Thomas ^a   Rabien, Sebastian ^a  

^a MAX PLANCK INSTITUT FÜR EXTRATERRESTRISCHE PHYSIK   (Germany)

Author keywords

Active Galactic Nuclei; Adaptive Optics; Convolution; Point Spread Function; Spectroscopy

Indexed keywords

ASTRONOMY; GALAXIES; INFRARED RADIATION; MATHEMATICAL MODELS; SENSORS; SIGNAL TO NOISE RATIO; SPACE TELESCOPES; SPECTROSCOPIC ANALYSIS; WAVEFRONTS;

ACTIVE GALACTIC NUCLEI (AGN); POINT SPREAD FUNCTION (PSF); STAR FORMATION; STARBURST MODELS;

ADAPTIVE OPTICS;

EID: 11144320634     PISSN: 0277786X     EISSN: None     Source Type: Conference Proceeding    
DOI: 10.1117/12.568135     Document Type: Conference Paper

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