README web version of /home/usg/OPS/MTS/readme_xml/readme_83041600

Principal Investigator Email Address

• laverny@oca.eu

Estimated Total Execution Time (hours, including overheads)

• 19:59:33

General Description

• The goal of this program is to collect CRIRES spectra of RGB stars
  found in two globular clusters with different metallicity.
  From these spectra, we will derive the 12C/13C ratio at the surface
  of these RGB stars in order to better understand the internal mixing
  characterising low-mass stars.
  
  All the finding charts are in the I-band since all targets are always very bright
   and very easy to find (even in the K band).
  They are the brightest and central source in the K-band.

Waiver Requests

• No Waiver Request was submitted

Critical Observing Condition Constraints

• No

Time-Critical Aspects

• After each science OB, we request that a telluric OB is observed immediately
   after
  in order to remove the telluric lines.
  Each OB of a telluric standard is named with the name of the its corresponding science
   OB.
  For instance, the OB "Telluric for N6397_65146" has to be executed immediately after
  the OB "N6397 AboveBump_65146 K8.8 + AO"

Special Execution Requirements

• After each science OB, we request that a telluric OB is observed immediately
   after
  in order to remove the telluric lines.
  Each OB of a telluric standard is named with the name of the its corresponding science
   OB.
  For instance, the OB "Telluric for N6397_65146" has to be executed immediately after
  the OB "N6397 AboveBump_65146 K8.8 + AO"

Special Calibration Information

• Telluric have to be observed immediatyl after each science OB.

ToO Information

• No

ToO Activators List

• No

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