README web version of /home/usg/OPS/MTS/readme_xml/readme_83018300
Principal Investigator Email Address
Estimated Total Execution Time (hours, including overheads)
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 TWA5A, TWA5B.
The A-component is about 5mag brighter than the B-component. Both components should
be put under the slit (see finding chart).
At 300s DITs, the A-component is well below the linearity limit according to the
ETC.
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 TWA 5A and B from 2007.
Currently, the system should appear close to that configuration (i.e., the secondary
has not moved much).
No telluric standard star is required.
Waiver Requests
Critical Observing Condition Constraints
Time-Critical Aspects
Special Execution Requirements
Special Calibration Information
ToO Information
ToO Activators List
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?
Do any OBs include wavelength or flatfield calibrations?
If you are observing Moving Targets, have you attached suitable ephemeris
files to your OBs?
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?
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?
Last creation of page: Tue Oct 6 15:40:29 2009
If you have comments, please contact usd-help@eso.org