ESO
2.2m-telescope
Procedure to
implement GROND/ToO observations during MPIA time
Regularly scheduled
observations during MPIA blocks are subject to interrupts from Target
of Opportunity Observations (ToOs) of Gamma Ray Bursts (GRBs) and
X-ray transient afterglows using GROND. Exceptions are
time-critical observations which are flagged as such and which may not
be interrupted by GROND/ToOs. In general, GROND/ToOs are executed
automatically and in Rapid
Response Mode (RRM).
On average, 15% of the available time per year may be used for
GROND/ToOs. Due
to the orbital inclincation of the SWIFT satellite, the GRB trigger
rate is variable in time. During times of
increased trigger rates, up to 25% of the available observing time in a
given month may be used for GROND/ToO observations.
Regularly scheduled programmes that suffer from GROND/ToO interrupts
are compensated in real time via ToO placeholders embedded in the
regular observing schedule. The service observer at the telescope takes
a real-time decision about how to fill those placeholders.
In cases where a full compensation for GROND/ToO interrupts is not
possible,
due to constraints imposed by lunar phase, right ascencion, seeing or
weather, the highest-ranked programmes
should be served first.
The rank of a programme is given in the observing plan.
During periods of lower than average trigger rates, the
placeholders may also be used to compensate for weather losses. Again,
the highest-ranked programmes should be served first, unless this is
not
possible from the various constriants such as lunar phase, seeing, etc.
Time accounting is based on the REMEDY ticket database containing all
respective trigger information for the GROND/ToO observations. A final
balancing reflecting actual losses incurred by GROND/ToO will be made
after each year of operation between MPIA and MPE, based on detailed
time
accounting provided by the REMEDY database.
The use of twilight for GROND, WFI, and FEROS
calibrations follows the
rules outlined above. On average, 15% of the time available for
twilight calibrations will be made available for calibrations
required for the GROND/ToO programme.
| Responsible: |
Roland Gredel
|
| Last
updated: |
March 20,
2009 |
|