README web version of /home/usg/OPS/MTS/readme_xml/readme_79045000

Principal Investigator Email Address

• arecio@oca.eu

Estimated Total Execution Time (hours, including overheads)

• 09:58:35

General Description

• The goal of this proposal is to derive the fluorine abundance (from the
   HF2.335microns line) in neighbour stars
  of the Sun.
  
  Since the targets are really bright (they are satured in the DSS images), 
  it is useless to provide finding charts.
  We have also checked that all the targets are the brightest sources in K
  from the 2MASS images (field 50"x50").
  
  Please observe one telluric star  after each scientific target star
  (the OB name of the telluric refers to the corresponding scientific target)
  
  We expect a SNR~200 for the science and telluric stars.

Waiver Requests

• We asked for using adaptive optics => accepted
  
  Task                      : Phase II
  inst/sub task             : Waiver request
  Resolution                : 
     02/06/07 17:51:20     mhilker
        Dear Patrick,
        
        sorry for the late answer to you waiver request. I am pleased to inform you
        that your waiver has been granted. You can use adaptive optics for your observations.
   Please go ahead with the completion of your Phase2 preparation.
        
        With best regards,
        Michael Hilker
        ESO User Support Department

Critical Observing Condition Constraints

• None

Time-Critical Aspects

• None

Special Execution Requirements

• ---(Empty)---

Special Calibration Information

• We request the observation of one telluric star (we provide the OBs) after
   each scientific target

ToO Information

• ---(Empty)---

ToO Activators List

• ---(Empty)---

Do the README file and the instrument comments of the telluric stars
 OBs include the required S/N/pixel of the spectrum of the telluric star, its spectral
 type and allowed spectral range?

• YES

Do any OBs include wavelength or flatfield calibrations?

• NO

If you are observing Moving Targets, have you attached suitable ephemeris
 files to your OBs?

• N/A

If the slit viewer guide star is different from the target, are the RA
 and DEC offsets accurate to within 0.05 arcsec and do they take into account the
 relative proper motion between the two objects?

• N/A

If you have preferences which OBs should be executed first for objects
 at similar RA, did you make use of the User Priority field in the OBs?

• YES