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Foreseen changes regarding La Silla, Paranal and APEX instrumentation and facilities
La Silla
No foreseen changes.
Paranal
UT instruments and facilities
- CRIRES:
- The ThAr lamp may be replaced by a UNe lamp in the course of P92.
-
Subject to approval of a major upgrade project, the instrument
may be taken out of operations for one year starting in the
second semester of 2014.
- XSHOOTER
will probably undergo an intervention lasting 3 months in Period 93 or 94, during
which the instrument will not be available for operations. The aim of the intervention
is to fix the ADC systems.
-
VIMOS: A call for public spectroscopic surveys may be issued for
VIMOS in the near future,if the instrument upgrade is successful and
the observation backlog has been resolved.
- SINFONI:
the Pupil Tracking mode may be offered in P93.
- It is expected
that the 2nd generation instruments
MUSE
and SPHERE
will undergo commissioning in P93.
Activities related to the installation of
the Adaptive
Optics Facility on UT4 (Yepun)
- GRAAL, the adaptive optics module for HAWK-I, is expected to be installed on Nasmyth A early in Period 93.
- The installation of the
4 Laser Guide Stars Facility (4LGSF) is expected to take place late in Period 93.
- GALACSI, the adaptive optics module for MUSE, is expected to be installed on Nasmyth
B early in Period 94.
- The installation of the Deformable
Secondary Mirror and re-commissioning of the telescope is
expected to take place late in Period 94; as a consequence, UT4 will
not be available during 2 months.
VLTI instruments and facilites
- MIDI
will likely be decommissioned during P93.
- It is expected that the VLTI Visitor Instrument focus will not be available starting with P93.
APEX
- Artemis : the installation of this PI instrument is foreseen in the first quarter of 2014. After succesful commissioning, it may be offered to the ESO community.
- ZEUS-2: Pending successful commissioning, the redshift (z) and Early Universe Spectrometer (ZEUS-2) may be offered as a PI instrument during Period 93. ZEUS-2 is a broadband spectrograph covering 7 telluric windows covering 200 to 850 µm. For details, see Ferkinho et al. 2010.
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