README web version of /home/usg/OPS/MTS/readme_xml/readme_83026900
Principal Investigator Email Address
Estimated Total Execution Time (hours, including overheads)
General Description
Our aim is to measure radial velocities in the outer parts of the three
ultrafaint dwarf spheroidals: Hercules, Leo IV and Leo V. With these radial velocities
we will investigate whether the outer parts of these remote objects are undergoing
tidal disintegration and we hope to be able to determine the likely orbit of each
dwarf and its velocity dispersion. From these data we can place strong constraints
on the dark matter content and orbital eccentricity of each dwarf.
We have selected a total of 8 fields around these objects and we want to look at
each field twice. Priority should be given to obtaining a first run of each field
before repeating the fields.
We do not need standard stars or special calibrations - standard daytime calibrations
with sky-line checks will be adequate.
We have not specified any guide stars; however we have checked the GSC2 catalog
and there are plenty of candidate guide stars around each field.
Waiver Requests
Critical Observing Condition Constraints
Time-Critical Aspects
Special Execution Requirements
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 ?
If you have prepared your finding charts with tools other than FIMS,
do they comply with the specifications on the FORS1 Phase 2 web page ?
Last creation of page: Tue Oct 6 15:40:29 2009
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