README web version of /home/usg/OPS/MTS/readme_xml/readme_78083300
Principal Investigator Email Address
Estimated Total Execution Time (hours, including overheads)
General Description
This program is the continuation of a long-term radial velocity survey
for
extrasolar planets begun in 1992. Goal is to look for long-period
extrasolar planets. To this end the radial velocity of each program star
is repeatedly measured over time.
HARPS is used in standard mode for highly accurate RV measurements with
the simultaneous ThAr technique.
Since all our program stars are bright (V > 6 mag) finding charts do not
make any sense and are not attached. Our stars are always the brightest
stars in the field. In a few cases a visual binary is seen in the field,
then the target is the brighter component. Only exception to this: Alpha
Centauri A and B (HR5459 and HR5450) for which BOTH components are to be
observed using the appropriate OBs: HR5459 (ALpCenA) is the brighter
component, HR5460 (AlpCenB) the fainter one.
Waiver Requests
Critical Observing Condition Constraints
Time-Critical Aspects
Special Execution Requirements
For stars that have more than one OB prepared:
(a) In a given night, do not execute more than one OB for the same star.
(b) The idea is to have the OBs distributed over the semester as much as
possible, i.e. to reobserve the star several times with gaps of (ideally)
several weeks between individual observations.
Special Calibration Information
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 15:40:17 2009
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