Applicants
should use the new NorthStar proposal tool
for preparation and submission of their observing requests. North Star
is reachable at http://proposal.mpifr-bonn.mpg.de
. From 2010 on only proposals submitted via NorthStar
will be accepted.
Observing proposals are
invited for the Effelsberg 100-meter Radio
Telescope of the Max-Planck-Institute for Radioastronomy (MPIfR).
The Effelsberg telescope is one of the World's largest fully steerable
instruments. This extreme-precision antenna is used exclusively for
research in radio astronomy, both as a stand-alone instrument as well
as for Very Long Baseline Interferometry (VLBI) experiments.
With
the advent of the new subreflector, observations from the secondary
focus (especially at frequencies > 10 GHz) gain from
a much higher sensitivity and flatter gain-elevation curves.
The
new hexapod driving system leads to a faster and more
precise focusing of all receiving systems in the primary and secondary
focus.
Access
to the telescope is open to all qualified astronomers. Use of
the instrument by scientists from outside the MPIfR is strongly
encouraged. The institute can provide support and advice on project
preparation, observation, and data analysis.
The directors of the institute make observing time available to
applicants based on the recommendations of the Program Committee for
Effelsberg (PKE), which judges the scientific merit (and technical
feasibility) of the observing requests.
Information about the
Program Committee can be seen at the
Effelsberg
Program Committee web page.
Observing modes
Possible observing modes include spectral line,
continuum, pulsar, and
VLBI. Available backends are a FFT spectrometer (with 8192 channels),
a digital continuum backend, a pulsar system (coherent and
incoherent dedispersion), and
two VLBI terminals (MK4 and VLBA type). For information look
here or
contact a
local
astronomer.
Receiving
systems cover the frequency range from 0.6 to 96 GHz. The
actual availability of the receivers depends on technical circumstances
and proposal pressure. For a description of the receivers read
this page; calibration
parameters, system temperature, sensitivity, etc. can be
found
here.
How to submit
Applicants
should use the new NorthStar proposal tool
for preparation and submission of their observing requests. North Star
is reachable at http://proposal.mpifr-bonn.mpg.de
. From 2010 on only proposals submitted via NorthStar
will be accepted.
For VLBI proposals
special rules apply: For proposals which
request Effelsberg as part of the European VLBI
Network (EVN) see:
http://www.evlbi.org/proposals/prop.html
Information on
proposals for the Global mm-VLBI network can be found on
http://www.mpifr-bonn.mpg.de/div/vlbi/globalmm/index.html.
Other proposals which
ask for Effelsberg plus (an)other antenna(s)
should be submitted
twice, one to the
MPIfR and a second to the
institute(s) operating the other
telescope(s) (eg. to NRAO for the VLBA).
The VLBI terminals in
Effelsberg are described at
http://www.mpifr-bonn.mpg.de/EVN/index.html