README web version of /home/usg/OPS/MTS/readme_xml/readme_75077100
Principal Investigator Email Address
Estimated Total Execution Time (hours, including overheads)
General Description
LSS spectroscopy with FORS2 300I and order separation filter OG590+32
of the host galaxies of GRB 980703 (2 hours 30 min) and GRB030329 (2 hours 55 min),
splitted into 3 OBs each. 2 hours LSS spectroscopy with FORS2 300I and order separation
filter OG590+32 of the host galaxy of GRB 020405, splitted into 2 OBs. LSS spectroscopy
with FORS2 300V and order separation filter GG435+81 of the host galaxies of GRB
990712 (2 hours) and GRB 011121 (2 hours), splitted into 2 OBs each. 4 hours LSS
spectroscopy with FORS2 of the host galaxy of GRB 031203, with 300V and order separation
filter GG375+80 (1 hour), and with 600RI and order separation filter GG435+81 (2
hours 55 min splitted into 3 OBs). 7 OBs are additionally dedicated for the LSS
observations of standard stars GD153, LTT7987, LTT3864 and LTT3218.
Goal: recombination time-scale and gas density determination of the GRB environments
by measuring the changes in emission line intensities and comparing with previous
observations.
Waiver Requests
Critical Observing Condition Constraints
Time-Critical Aspects
Special Execution Requirements
If possible, please execute the OBs as grouped below right after each
other:
group1: OBs "LSS GRB 980703","LSS GRB 980703-0", "LSS GRB 980703-1"
group2: OBs "LSS GRB 990712","LSS GRB 990712-0"
group3: OBs "LSS GRB 011121","LSS GRB 011121-0"
group4: OBs "LSS GRB 020405","LSS GRB 020405-0"
group5: OBs "LSS GRB 030329","LSS GRB 030329-0", "LSS GRB 030329-1"
group6: OBs "LSS GRB 031203 600RI","LSS GRB 031203 600RI-0","LSS GRB 031203 600RI-1"
group7: OB "LSS GRB 031203 300V"
The OBs forming a group are identical and running them in direct sequence would
save the repetition of the aquisition and through slit templates.
In addition, it is very important to have the spectroscopic standard star OBs right
after the related group. For each group, it is enough to execute a single standard
star OB right after one of the OBs in the group. The details are specified in the
Calibration Requirements section of each science OB.
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 FORS2 Phase 2 web page ?
Last creation of page: Tue Oct 6 15:40:08 2009
If you have comments, please contact usd-help@eso.org