Performance of the Keck long wavelength spectrometer

Advances in Space Research

Volumn 34, Issue 3, 2004, Pages 499-503

  Campbell, R D ^a   Jones, B ^b  

^a W M KECK OBSERVATORY   (United States)

^b UNIVERSITY OF CALIFORNIA   (United States)

Author keywords

Keck telescope; Long Wavelength Spectrometer; Mid infrared instrument; Titan atmosphere

Indexed keywords

IMAGING SYSTEMS; SOLAR SYSTEM; SPECTROMETERS; TELESCOPES;

BLOCKED IMPURITY BAND (BIB); TELESCOPE EMISSIVITY;

SPACE RESEARCH;

PLANETARY ATMOSPHERE; SPECTROMETER; TITAN;

EID: 3042559822     PISSN: 02731177     EISSN: None     Source Type: Journal    
DOI: 10.1016/j.asr.2003.04.036     Document Type: Article

References (4)

1. Agol E. Jones B. Blaes O. Keck mid-infrared imaging of QSO 2237+305 Astrophys. J. 545 2000 657-663
2. Gehrz R.D. Smith N. Jones B. Puetter R. Yahil A. Keck LWS images of the compact nebula around RY Scuti in the thermal infrared Astrophys. J. 559 2001 395-401
3. Jones, B., Puetter, R.C. Keck long wavelength spectrometer, in: Fowler, A.M. (Ed.), Infrared Detectors and Instrumentation, Proceeding of SPIE, vol. 1946, 610-621, 1993
4. Roe, H.G. Titan's atmosphere at high resolution, PhD Thesis, University of California at Berkeley, Berkeley, CA, USA, 2002