README web version of /home/usg/OPS/MTS/readme_xml/readme_84081802
Principal Investigator Email Address
Estimated Total Execution Time (hours, including overheads)
General Description
UVES spectroscopic observations of nuclear star clusters in six dwarf
galaies.
The observations should be performed with 1.2" slit width with the red arm at central
wavelength 580 nm with 2x2 CCD binning. The derotation mode is "SKY" with ADC on
for ESO 059-01, ESO 223-09, IC 1959, NGC 1311 and "ELEV" for KK 197 and NGC 5237.
The target's coordinates are based on the HST/ACS images WCS, whose typical astrometric
error is 0.3", thus precise enough to directly position even the faintest target
(V_app = 20.2) in NGC 1311. The images used to create the finding charts are from
the same HST/ACS V-band (F606W) images. The resoluoin is 0.05 arcsec / pixel. The
targets are marked with a rectangle with dimensions of 10 x 1.2 arcsec for the targets
in "SKY" and with circle in "ELEV" derotation modes, respectively.
We have split in to 1 , 2 , 4 and 5 OBs of 50.083 min integration time each for
the star clusters depending on cluster apparent V-band magnitude. The total execution
time per OB is 1 hour, thus 18 OBs sums up to 18 hours for the entire Run C. The
expected signal-to-noise is in the range S/N > 10 - 20 per resolution element
in the wavelength range around 5200A (Mg triplet).
Waiver Requests
Critical Observing Condition Constraints
Time-Critical Aspects
Special Execution Requirements
Special Calibration Information
ToO Information
ToO Activators List
Do all your OBs comply with the instrument-specific requirements listed
on the instrument-specific Phase 2 web page ?
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 specified the S/N ratio at given wavelength in the User Comments
field of each OB?
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 15:40:32 2009
If you have comments, please contact usd-help@eso.org