README web version of /home/usg/OPS/MTS/readme_xml/readme_76050702
Principal Investigator Email Address
Estimated Total Execution Time (hours, including overheads)
General Description
This is a Target of Opportunity/Rapid Response Mode programme to follow
up as rapidly as possible candidate high-redshift gamma-ray bursts (GRBs). The requested
OBs must therefore be executed as soon as possible after we have triggered the override.
Note: to cover all the possibilities, we have made one (and only one) OB for each
configuration we may conceivably wish to use. However we may need to repeat a given
OB once or twice to achieve long (>1hr total execution time) exposures. We understand
this is only possible for ToOs, not RRMs. Therefore we have made as many copies
of each RRM as we may wish to use.
Waiver Requests
Critical Observing Condition Constraints
Time-Critical Aspects
Special Execution Requirements
Special Calibration Information
ToO Information
This is a Target of Opportunity/Rapid Response Mode programme to follow
up as rapidly as possible candidate high-redshift gamma-ray bursts (GRBs). The requested
OBs must therefore be executed as soon as possible after we have triggered the override.
Note: to cover all the possibilities, we have made one (and only one) OB for each
configuration we may conceivably wish to use. However we may need to repeat a given
OB once or twice to achieve long (>1hr total execution time) exposures. We understand
this is only possible for ToOs, not RRMs. Therefore we have made as many copies
of each RRM as we may wish to use.
ToO Activators List
PI: Nial Tanvir nrt@star.herts.ac.uk, nrt@ast.cam.ac.uk
Enrico Cappellaro cappellaro@na.astro.it, Palle Moller pmoller@eso.org
Ferdinando Patat fpatat@eso.org
Ralph Wijers rwijers@science.uva.nl, Rhaana Starling starling@science.uva.nl
Klaas Wiersema kwrsema@science.uva.nl, Alexander van der Horst avdhorst@science.uva.nl
Paul Vreeswijk pvreeswi@eso.org, Peter Curran pcurran@science.uva.nl
Nicola Masetti masetti@bo.iasf.cnr.it, Eliana Palazzi palazzi@bo.iasf.cnr.it
Elisabetta Maiorano maiorano@bo.iasf.cnr.it, Giulia Stratta gstratta@ast.obs-mip.fr
Elena Pian pian@bo.iasf.cnr.it, pian@ts.astro.it
Jens Hjorth jens@astro.ku.dk, Johan Fynbo jfynbo@phys.au.dk
Andreas Jaunsen ajaunsen@eso.org, Holger Pedersen holger@astro.ku.dk
Brian L. Jensen brian_j@astro.ku.dk, Michael Andersen mandersen@aip.de
Palle Moller pmoller@eso.org, Pall Jakobsson pallja@astro.ku.dk
Darach Watson darach@astro.ku.dk, Jesper Sollerman jesper@astro.su.se
Jochen Greiner jcg@mpe.mpg.de, Aybuke Kupcu Yoldas ayoldas@mpe.mpg.de
Arne Rau arau@mpe.mpg.de, Sylvio Klose klose@tls-tautenburg.de
Alberto Castro-Tirado ajct@iaa.es, Jose Maria Castro Ceron josemari@alumni.nd.edu
Javier Gorosabel jgu@iaa.es, jgu@laeff.esa.es
Antonio de Ugarte deugarte@iaa.es, Andy Fruchter fruchter@stsci.edu, James Rhoads
rhoads@stsci.edu
David Bersier bersier@stsci.edu, Andrew Levan anl@star.le.ac.uk, Evert Rol
er45@star.le.ac.uk
Robert Priddey priddey@star.herts.ac.uk, Bob Chapman bchapman@star.herts.ac.uk
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 15:40:10 2009
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