README web version of /home/usg/OPS/MTS/readme_xml/readme_83055204

Principal Investigator Email Address

• nrt3@star.le.ac.uk

Estimated Total Execution Time (hours, including overheads)

• N/A

General Description

• This programme aims to identify high-redshift gamma-ray burst afterglows,
   and consequently obtain their redshift.
  
  Note, this run:
   083.A-0552(E) 0hours SINFONI (alternative for run(A), ISAAC)
  
  is allocated 0hours, because the time-accounting is done together
  with their "mother run", namely A.  Any time used on this run should
  therefore be charged to run A.

Waiver Requests

• No Waiver Request was submitted

Critical Observing Condition Constraints

• There are no critical observing constraints.

Time-Critical Aspects

• This is a target-of-opportunity program. Observations should be executed
   as soon as feasible, since the target brightness decays rapidly.

Special Execution Requirements

• ---(Empty)---

Special Calibration Information

• ---(Empty)---

ToO Information

• This is a target-of-opportunity program. Observations should be executed
   as soon as feasible, since the target brightness decays rapidly.
  We will communicate with the observer to discuss any complications or particular
   requirements for the given target.

ToO Activators List

• Nial Tanvir	      nrt3@star.le.ac.uk, nrt@ast.cam.ac.uk
  Andrew Levan 		a.j.levan@warwick.ac.uk
  Evert Rol 		evert.astro@gmail.com
  Pall Jakobsson 		pja@raunvis.hi.is
  Rhaana Starling 	rlcs1@star.le.ac.uk
  David Bersier 		dfb@astro.livjm.ac.uk
  Ralph Wijers 		rwijers@science.uva.nl
  Klaas Wiersema 		kw113@star.le.ac.uk
  Nicola Masetti 		masetti@bo.iasf.cnr.it
  Eliana Palazzi 		palazzi@bo.iasf.cnr.it
  Elena Pian 		pian@oats.inaf.it
  Jens Hjorth 		jens@astro.ku.dk
  Johan Fynbo 		jfynbo@phys.au.dk
  Brian Lindgren Jensen 	brian_j@astro.ku.dk
  Michael Andersen 	mandersen@aip.de
  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
  Sylvio Klose 		klose@tls-tautenberg.de
  Alberto Castro-Tirado 	ajct@iaa.es
  Javier Gorosabel 	jgu@iaa.es, jgu@laeff.esa.es
  Antonio de Ugarte 	adeugart@eso.org
  Andy Fruchter 		fruchter@stsci.edu
  Palle Moller 		pmoller@eso.org
  Ferdinando Patat 	fpatat@eso.org
  Paul Vreeswijk 		pmv@astro.ku.dk, pmv@dark-cosmology.dk
  James Duke 		jbd2@star.le.ac.uk
  Karl Svensson 		k.m.svensson@warwick.ac.uk
  Andreas Jaunsen		a.o.jausen@astro.uio.no

Is this a Pre-imaging run ?

• false

Pre-imaging Requirements

• ---(Empty)---

Source(s) of Pre-imaging

• ---(Empty)---

Pre-imaging sources not listed above

• ---(Empty)---

Do all your OBs comply with the instrument-specific requirements listed
 on the instrument-specific Phase 2 web page ?

• YES

If this is a pre-imaging run, did you select PRE-IMAGING for the Observing
 Category for each Observing Template ?

• N/A

Do all your finding charts comply with both the general and instrument-specific
 Phase 2 Web Pages ?

• N/A

If you submitted OBs for standard stars, did you specify the magnitude
 and spectral type of all standard stars in the OBs ?

• N/A

Have you included OBs for any calibrations that you need but which are
 not part of the Calibration Plan ?

• N/A

If you are observing Moving Targets, have you attached suitable ephemeris
 files to your OBs?

• N/A

If you have preferences which OBs should be executed first, did you make
 use of the User Priority field in the OBs ?

• N/A

If this is a run that requires coordinated observations with other facilities,
 did you give proper instructions in the Time-Critical Aspects Section ?

• N/A

Did you indicate the magnitude of the brightest object in the field in
 each SINFONI OB?

• N/A

If you are using the AO: Did you indicate for every OB the magnitude
 of the guide star, and its distance to the target (if any)?

• N/A

If you submitted OBs for standard stars, did you use the provided StandardStar
 templates?

• N/A

If you are using a specific offset pattern or position angle: did you
 check carefully the definition in the manual?

• N/A

Did you make really sure that none of your OBs ever saturates the detector?

• YES

If you are using the AO: did you enter the correct Strehl Ratio (on-axis,
 K-band) AND the seeing value in the constraint set?

• N/A