README web version of /home/usg/OPS/MTS/readme_xml/readme_83025201
Principal Investigator Email Address
Estimated Total Execution Time (hours, including overheads)
General Description
These OBs refer to 2 calibrating stellar clusters (NGC104 and NGC7078)
and the Phoenix dI/dSph. This submission completes the allocated observing time.
The OBs do not need to be done in the same night.
Please carefully check the centering of the targets on the slits, expecially for
pointing 02.
The constrain on airmass has been slightly relaxed for the stellar
clusters (can be less than 1.7), while for the science target Phoenix should be
less than 1.5.
The moon illumination constraint has been relaxed for fields 02, 03, 14 (it is now
0.6)
The goal is to acquire spectra of red giant branch stars in both the 2 globular
clusters and Phoenix,
using FORS in MXU mode. The line-of-sight velocities and CaII triplet EW derived
from the stellar clusters spectra will be used to calibrate the science observations
of the Phoenix dI/dSph.
Waiver Requests
Critical Observing Condition Constraints
Seeing <= 1" , airmass < 1.7 , clear sky for NGC7078 and NGC104.
Seeing <= 1", airmass < 1.5, clear sky for the Phoenix dI/dSph.
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
If you have comments, please contact usd-help@eso.org