README web version of /home/usg/OPS/MTS/readme_xml/readme_82002900
Principal Investigator Email Address
Estimated Total Execution Time (hours, including overheads)
General Description
This is a simple run in order to measure linear polarimetry of some quasars
in the V-band (i.e. with the V-high filter). The exposure time computed with the
ESO ETC are such that there should be no saturation even if the seeing = 1.0 arcsec.
If the seeing is better than 1.0 arcsec, please reduce the exposure time for the
brightest objects in order to not saturate the images:
-if the seeing is around 0.8", reduce the exposure time given in the OB of targets
with a magnitude Mv < 20 by a factor 0.7 (the faintest objects (Mv>20) will
not saturate, so no correction have to be applied).
-if the seeing is around 0.6", reduce the exposure time given in the OB of targets
with magnitude Mv < 20 by a factor 0.4 (once again the faintest objects (mag>20)
will not saturate)
We give in each OB the magnitude Mv of the target in the 'User comment' line.
Waiver Requests
Critical Observing Condition Constraints
Time-Critical Aspects
Special Execution Requirements
We give a "User Priority" (1,2 or 3) in each OBs in order to execute some
OBs in priority.
Objects with user priority 1 are part of another program ranked in the B class (Prog082.B-0029(B));
obtaining polarimetry for those objects is mandatory in order to complete the scientific
goals of this second program. In addition to these objects, there is another object
with a user 1 priority : COMBO_52963 (=Target name). Obtaining polarimetry for this
object would be much appreciated since it is one of our best candidates to fulfill
one of the principal goal of the current program (obtaining linear polarimetry for
Type1 quasars with a resolved HST image). Please pay attention that we divided the
total exposure time requested for this object into two OBs (COMBO_52963-1 and COMBO_52963-2)
in order to allow a better schedulability (the overheads may be decreased if you
observe the two OBs consecutively).
We do not need more calibrations than those indicated in the FORS1 calibration plan
(i.e. observation of a polarized standard at the end of the night and imaging sky
flat without polarizers).
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 15:40:26 2009
If you have comments, please contact usd-help@eso.org