E N I G M A*
A network on Blazar research, funded by the European Commission through
the TMR (Training and Mobility for Researchers) program
European
Network for the
Investigation of
Galactic nuclei through
Multifrequency
Analysis
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*ENIGMA is the acronym of this European Network for the
Investigation of Galactic nuclei through Multifrequency Analysis.
An enigma is
a riddle. In ancient Greece the winged sphinx of Boeotian Thebes posed a riddle
taught her by the muses.
In modern times Blazars pose many riddles to astrophysicists working in all
branches of astronomy.
Sphingen are symbols of enigmatic behaviour, as is
frequently displayed by Blazars.
The sphinx is thus a symbol for the riddles posed by Blazars which are
tackled in our network ENIGMA.
On November 1, 2002 this network which deals with investigations of the
structure and radiation processes of quasars through multifrequency studies
started officially. ENIGMA is funded by the European Commission
through the TMR (Training and Mobility for Researchers) programme, and links
eight European research institutions (referred to as members) and seven
additional teams (referred to as associate members).
Science
The science activities of this network are addressed in six complementary
research themes which are closely connected to each other. While all of the
empirical themes drive the requirements of the hardware/software theme, the
empirical projects are aimed at maximizing efficiency by teaming up
observational resources and
coordinated campaigns.
The two theoretical themes
have many links between themselves, and clear connections to the three
empirical subjects.
Further information on each of those subjects is provided here, or by clicking on the specific topic:
1) Towards automated, fast, and accurate
photometry:
2) Separating intrinsic and extrinsic Intraday
Variability:
3) Radiation processes at high energies:
4) Variations of Source Structure and Flux:
5) Particle acceleration in MHD outflows:
6) The Power of Jets:
The research aims are directed at answering three
fundamental questions:
a) How is the bulk kinetic energy within jets transformed
into radiation?
b) What is the relationship between jet power and
accretion power?
c) What is the origin of the FR-I/FR-II dichotomy?
In addition to the six specific themes, a joint effort towards establishing a
data-bank of densely sampled, long-term, high quality photometric data
will be pursued by all teams. This effort will be closely connected with each
of the six specific themes. It will provide the basis for the exploration of
extended parts of parameter space (short time-scales and long time-scales).
Teams
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Team Coordinator and Young Researchers
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Partners and Members
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In addition to the eight teams, the network is supported by an external
advisor, Prof. Alan
Marscher, Boston University, who,
with his group, works on many
aspects of the blazar phenomenon.
Jobs
Seven postdoctoral positions and three predoctoral positions (for Ph.D.
students) are available within the ENIGMA Network.
They are hosted by one of the eight European research institutions
(members) of this network.
The network has been established to carry out research in the following
areas:
Developing reliable robotic systems for automated ground-based monitoring of
AGN;
Developing high-precision photometric routines in different waveband
regimes;
Developing advanced statistical methods for time-series analysis and
applications to astrophysical models;
Multi-frequency observations of radio-loud AGN to study:
radio/optical Intra-Day variability,
relationships between structural and flux density
variability,
relationships in different high-energy bands (X-ray,
gamma-rays, and VHE radiation with Cerenkov telescopes).
Numerical simulations and analytical modelling to better understand:
particle acceleration and radiation mechanisms,
magnetohydrodynamic flows,
jet physics in Blazars.
Postdocs and Ph.D. students will work in their host team and within this
active and interacting network of empirical and theoretical research.
They will have access to unique observational facilities and will profit from
a strong training program involving hardware-related aspects, observational
strategies in all waveband regimes, and theoretical research.
Postdoctoral researchers are
encouraged to spend part of their time at other institutes during their
appointment.
Ph.D. students may either carry out part of their Ph.D. with one of the
partners, with the remaining part being completed within their
home institution, or they may carry out their entire Ph.D. with their host
team and obtain their Ph.D. degree at the corresponding university. The
ENIGMA network will be very flexible in this regard. The Ph.D. students are
expected to work mostly within their host team, but they will be involved in
network-wide training programs. Short-term visits to home universities and
other network teams will be possible.
Questions regarding the research program can be directed to Prof. S. Wagner,
swagner at lsw.uni-heidelberg.de (network coordinator).
Ten positions have/will become available between March 2003 and March 2004.
The positions are tenable for up to two or three years. Competitive salaries
will be paid, differing according to local regulations. Additional support
will be available for extended visits to other partner institutions within the
network, network meetings and conferences.
According to the rules of the EC, the positions are open to young researchers,
holding a passport of a Member or Associate State of the European Union.
Further details are given by the
regulations of the EC programme .
Applications should include a curriculum vitae, a publication list, a summary
of current research interests as well as a list of topics of interest or
institutes which they would prefer to join. Two letters of reference should
also be arranged for. The review of applications will start at different dates
for different teams. Current openings review
applications until the positions are filled. Material
should be sent to Landessternwarte Heidelberg, S. Wagner, Koenigstuhl 12,
69117 Heidelberg, Germany, swagner at lsw.uni-heidelberg.de
For a more detailed description of the positions available and their
individual profiles follow this link.
The poster advertising the vacancies can be downloaded
here. Further details may also be found in the
Job
advertisement of the AAS job register, or the
EC-RTN announcement of vacancies.
Meetings
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The first
network meeting was held May 11 - 14, 2003 in Mayschoss,
Germany.
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The second network meeting was held October 11-15, 2003 in
Portovenere, Italy.
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The third network meeting was held April 25-28,
2004 in Muonio, Finland.
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The fourth network meeting was held October 6-8,
2004 in Perugia, Italy.
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The ENIGMA Mid Term Review was held March 9,
2005 in Bonn, Germany
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The
fifth network meeting was held June 13-17,
2005 in Hotel Bornmuehle,
Neubrandenburg, Germany.
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The
sixth network meeting was held November 22-25,
2005 in Kinsale, Ireland.
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The
seventh network meeting was held Mai 8-10,
2006 in Hydra, Greece.
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The
eighth (last) network meeting was held September 6-8,
2006 in Espoo, Finland.
Schools