README web version of /home/usg/OPS/MTS/readme_xml/readme_76001000
Principal Investigator Email Address
Estimated Total Execution Time (hours, including overheads)
General Description
The aim of the project is to search for extra-solar planets by means of
precise RV-measurements with HARPS (simultaneous ThAr
calibration). Thus, standard calibrations for high precision
RV-measurements are needed (As described in the HARPS manual page
14). The aim of this project is to take during the semester many
spectra (up to 10) of the candidates found in semester 74 and 75 in order to
derive the orbits of the companions. For this, it is best to carry out
the OBs at random times during the semester. Any spacing between the OBs
for one star down to one night is fine, as the orbital periods can be as
short as 3 days. The RV-variations are often as large as 100
m/s! There are only 5 OBs for those stars that can only be observed at
the beginning, or at the end of the semester.
(priority: 1: high)
Waiver Requests
Critical Observing Condition Constraints
Time-Critical Aspects
Special Execution Requirements
Special Calibration Information
Just standard calibrations for high precision RV-measurements are
needed (As described in the HARPS manual page 14). That is at the
beginning of the night: 1xbias, Flat fiber A, Flat fiber B, 5xFlat fiber
AB, 2xThAr fiber AB.
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 ?
Last creation of page: Tue Oct 6 15:40:09 2009
If you have comments, please contact usd-help@eso.org