README web version of /home/usg/OPS/MTS/readme_xml/readme_83018301

Principal Investigator Email Address

• Ansgar.Reiners@phys.uni-goettingen.de

Estimated Total Execution Time (hours, including overheads)

• 3.0

General Description

• This is a program to observe the molecular FeH band in low-mass objects
   with CRIRES.
  The main goal of this run is to observe the low-mass companion of HR7329A, HR7329B.
  The A-component is an A0 about 7mag brighter in J than the B-component. Only component
   B should be put under the slit (see finding chart). 
  
  The three OBs are identical and can be executed at any time.
  
  Two finding charts are provided:
  
  - one showing the field from a 2MASS J-band image from 1999 identifying the system
  - one showing a detailed NACO Ks-image of HR7329A and B (obtained with a ND-filter,
   HR7329B should be easily visible during CRIRES acquisition).
  
  No telluric standard star is required.

Waiver Requests

• Waiver granted to use free wavelength settings in our observing runs 383.D-0183(A)
   and 383.D-0183(B).

Critical Observing Condition Constraints

• N/A

Time-Critical Aspects

• N/A

Special Execution Requirements

• ---(Empty)---

Special Calibration Information

• ---(Empty)---

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?

• N/A

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?

• YES

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?

• N/A