README web version of /home/usg/OPS/MTS/readme_xml/readme_82038400
Principal Investigator Email Address
Estimated Total Execution Time (hours, including overheads)
General Description
The knowledge of blazar redshifts allows to constraint the physics of
central engine, relativistic jets, high-
energy emission models and bolometric power. The absorption of ? -rays emitted by
blazar-probes at different
z, provide us also crucial information on the cosmic EBL. The quasi-featureless
spectra of blazars hinders the
determination of z and, often, radio/X-ray blazar counterpart associations to close
pairs of optical ob jects are
doubtful. We propose an easy and successful filler program (high S/N spectroscopy
at VLT in SM during bad
seeing/sky conditions), maximizing scientific results in an exciting twofold way.
1) using the new z values for
modelling in the frame of ? -ray space missions like AGILE (flying) and GLAST (launch
May2008). 2) disentan-
gling/investigating spectral features of blazars with an intriguing close environment
(companions, intervening
or more complex systems). Feasibility and success rate is confirmed by our previous
runs in P71-P73, P77, P81.
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 15:40:27 2009
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