README web version of /home/usg/OPS/MTS/readme_xml/readme_77083103
Principal Investigator Email Address
Estimated Total Execution Time (hours, including overheads)
General Description
This is a simple spectroscopic programme consisting of
two independent OBs for two different targets in Chamaeleon,
which should be executed in June or July 2006 (the later, the better),
whenever the relaxed seeing conditions are met.
The later the observations can be carried out in June/July, the
better it is for the science program, which requires a time offset
to another run of several weeks (see Time critical aspects).
However, the airmass should be below 2.
Waiver Requests
Critical Observing Condition Constraints
Time-Critical Aspects
The OBs of this run D should be executed in June or July
in order to make sure that there is a time offset of a few weeks
to another run (077.C-0831(A)) of this program, which is carried
out in April.
The larger the timely separation between run A and D, the better.
However, the airmass should be below 2.
Explanation: Run D consists of identical OBs as run A. A timely
spacing of a few weeks of the two runs will allow a repeated
measurement of the radial velocities with a long enough time base
for orbital period sampling of the two companion candidates.
Special Execution Requirements
Special Calibration Information
A wavelength calibration (ThAr lamp) is needed on the same day with exactly
the same settings
as the observations (readout 50kHz,2x2,high, slit width 1.0", central wlgt 860nm)
and with
* an exposure time of ~0.1 sec * (otherwise there will be too many lines saturated!).
ToO Information
ToO Activators List
Is this a Pre-imaging run ?
Pre-imaging Requirements
Source(s) of Pre-imaging
Pre-imaging sources not listed above
Do all your OBs comply with the instrument-specific requirements listed
on the instrument-specific Phase 2 web page ?
If this is a pre-imaging run, did you select PRE-IMAGING for the Observing
Category for each Observing Template ?
Do all your finding charts comply with both the general and instrument-specific
Phase 2 Web Pages ?
If you submitted OBs for standard stars, did you specify the magnitude
and spectral type of all standard stars in the OBs ?
Have you included OBs for any calibrations that you need but which are
not part of the Calibration Plan ?
If you are observing Moving Targets, have you attached suitable ephemeris
files to your OBs?
If you have preferences which OBs should be executed first, did you make
use of the User Priority field in the OBs ?
If this is a run that requires coordinated observations with other facilities,
did you give proper instructions in the Time-Critical Aspects Section ?
If you need secondary guiding, are there suitable objects within 30 arcsec
from your target ?
Last creation of page: Tue Oct 6 15:40:14 2009
If you have comments, please contact usd-help@eso.org