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CRIRES  Science Verification Observations
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Topic  : Life, the Universe and everything

Authors: Douglas Adams and Deep Thought
         affiliation and email, who is PI?
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We propose observations to answer the mathematical equation 7 x 6
which is a challenging test of the spectral resolution of CRIRES and
its overall concept


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Project 
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Abstract: 
Describe here in ~20-30 lines what it is you want to do and why?
Describe why you consider this a science verification project


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Target List and Table
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name      | alfa 2000 delta 2000 | lambda range | Fnue or Fline | exp. time 
          |                      | wavelength ID|               | DIT, NDIT
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eps Eri   |03 32 55.1 -09 27 29  | 1800-1820nm  | 100 mJy       |  
          |                      | 31/-1/n      |               |  50s, 3
          |                      | 31/-1/i      |               |  50s, 3
          |                      | 31/ 1/n      |               |  50s, 3
          |                      | 31/ 1/i      |               |  50s, 3

beta Pic  |05 47 17.1 -51 03 59  | 3950-4120nm  | 20 W/m^2      |  
          |                      | 14/-2/n      |               |  30s, 3
          |                      | 14/-2/i      |               |  30s, 3
          |                      | 14/-1/n      |               |  30s, 3
          |                      | 14/-1/i      |               |  50s, 3
          |                      | 14/ 1/n      |               |  50s, 3
          |                      | 14/ 1/i      |               |  50s, 3


Fnue or Fline according to CRIRES-ETC;
consider width of spectral features relative to pixels 
DIT, NDIT per wavelength ID !!!
DIT, NDIT from ETC
wavelength ID from CRIRES manual, appendix A 


if appropriate give angular size, slit width and postion angle
(recommended slit is ~ 0.4 arcsec for the moment


Note: from the manual and the ETC you select the relevant numbers;
      you must check, how your spectral features are mapped on the
      detector array

adaptive optics notes:  
      reference star alpha, delta; V/R-magnitude, 
      relative location: distance in arcsec, position angle
                        

finding chart attached (if appropriate)


comments: don't panic 


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Detailed description of Suggested observations:
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write whatever you think is necessary that the ESO-SV-team can understand what
they should do exactly (complementing the above table); please specify what
the minimum data set must comprise of to be scientifically useful 


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SCIENCE GOALS:
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any additional information and links to references not to exceed ~1 page; how
would you reduce the data? E.g. we will use the context long in MIDAS and will
compare the absorption spectra to Mozart's all singing and dancing radiation
transfer code for Waltzer dancing stars.