README web version of /home/usg/OPS/MTS/readme_xml/readme_80063101
Principal Investigator Email Address
Estimated Total Execution Time (hours, including overheads)
General Description
This is a straightforward imaging run consisting of 10 photometric observations
of ~ 3*242s exposure time each with the b_high filter. The goal is to study the
variability of the optical counterpart of the ultraluminous X-ray source NGC1313
X-2. This star has B~23.4 mag and is variable by at least 0.2 mag on a timescale
of days. For scientific reasons, we ask preferentially that each of the photometric
observation should be carried out directly before or after the spectroscopic observation
(program 080.D-0631(A)). As we know that this kind of link decreases the scheduling
possibilities of the VLT, it is however not a strict constraint.
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 15:40:22 2009
If you have comments, please contact usd-help@eso.org