README web version of /home/usg/OPS/MTS/readme_xml/readme_83018700
Principal Investigator Email Address
Estimated Total Execution Time (hours, including overheads)
General Description
The knowledge of blazar redshifts is mandatory to constrain the physics
of the central engine, relativistic jets,
emission models and bolometric power. Moreover, the study of gamma-ray absorption
from blazars at di?erent
redshifts is mandatory to obtain informations on the Extragalactic Background Light.
The quasi featureless
spectrum of BL Lacs often hinders the redshift determination. Here we propose an
easy and successful ?ller pro-
gram, aimed at obtaining high S/N BL Lac spectra using VLT in SM under non-optimal
seeing/sky conditions.
The science result will be maximized by: 1) using the new redshift to model blazar
emission in the frame of
the new Fermi gamma-ray missions, 2) studying spectral features of blazar with an
intriguing close environment (i.e.:
close companions, intervening halos, small galaxy groups).
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 15:40:29 2009
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