OPEN CALL FOR
OBSERVING TIME AT THE NORDIC OPTICAL TELESCOPE

Credit: Ruslan Merzlyakov
What is offered
In this call, the Nordic Optical Telescope (NOT) offers access to
observing time in return for a contribution to the operational cost.
The Nordic Optical Telescope is located at the Roque de los Muchachos
Observatory on the Canary island La Palma, Spain, which provides some
of the best observing conditions on the northern hemisphere. The
observing conditions, instrumentation and observing modes offered at
the NOT allow to do state-of-the-art observations, at the forefront of
many areas in modern astronomical research, as is also shown by its
strong publication
record. |

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The call is open to anyone from anywhere, be it projects, research
groups, institutes or larger (national) communities. The scale of any
agreement can range from small observing time allocations in a single
semester, up to more extensive allocations over various years
(possibly as a full member).
User contributions
The baseline cost per night is €5,620. The general rules for the
allocation of observing time and the related user contributions can be
found
here,
in particular see Chapter 7 'External projects' of that document.
Instrumentation and telescope
An overview of the instrumentation at the NOT can be
found here.
The workhorse instruments are an optical imager and low-resolution
spectrograph ALFOSC,
a NIR imager and low-resolution
spectrograph NOTCam,
and a fibre fed echelle
spectrograph FIES
which offers resolutions up to ~67,000, and is located in a separate
building in a controlled environment, and provides a radial-velocity
stability of ~4 m/s. A further upgrade of the spectrograph, with the
aim of improving the radial velocity stability to ~2 m/s, is in
progress.
Over the last several years, we have expanded the capabilities of the
telescope to observe solar-system objects, in particular very fast
moving objects such as (hazardous) near-earth asteroids and comets,
and space debris. We have done multiple observations of GPS
satellites, which move with speeds of 50-100 "/sec relative to
siderial rates, and we believe we can do observations of objects with
speeds in the order of ~1000 "/sec.
Observing modes
Scientific programs
One of the strengths of the NOT is that it provides a wide range of
options for flexible scheduling. Broadly speaking, we provide the
following observing modes:
- Visitor mode: This is the classical observing mode, with
specific observing runs, normally consisting of several
consecutive nights, where visiting observers execute the
observations themselves. Astronomical and support is provided on
the first night, and technical support is provided on the
remaining nights
- Service mode: In principle the same as for regular visitor
mode observations, except that the observations are executed by
the NOT staff
- Monitoring mode: This is in effect a sub-category of
service mode, where the observing time is divided in smaller
chunks (being only a part of a night) that are spread over various
nights, where we do the observations. The naming is more an
indication on the scheduling (a couple of nights in a single
observing run versus various small chunks of time spread over
multiple nights)
- Target-of-Opportunity(ToO)/Queue mode: These are also
observations executed in service mode, but the observations are
executed depending on specific requirements. This can, in the case
of a ToO program, be the requirement of prompt (immediate)
execution of observations triggered by a transient event, or this
can (also) be the requirement for specific observing conditions
(e.g., a seeing limit) under which the observations are to be
executed
For the execution of the observations, we provide a system of
Observing Blocks (OBs), in which observation can be fully
defined. The use of OBs is in principle mandatory, except for
visitor mode observations.
Educational use
Beyond the use for scientific programs, the NOT also provides
dedicated facilities for both on-site and remote observing
courses. For general information,
look here.
Contact
For any questions and/or more detailed information, please contact
director@not.iac.es.