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BOLETIM ELETRÔNICO SAB N. 432 - 23/07/2008
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SEÇÃO: OPORTUNIDADES - INFORMES
Responsável: Vera Ap.F. Martin (vmartin1963@gmail.com)
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1. ESA RESEARCH FELLOWSHIPS IN SPACE SCIENCE
2. RESEARCHER IN SOFTWARE FOR RADIO ASTRONOMY WITHIN ASTROPHYSICS
3. CONCURSO NA UNIVERSIDADE FEDERAL DO ABC - VÁRIAS ÁREAS
4. ESO SPECTRAL ADVANCED DATA PRODUCTS
5. POSTDOCTORAL POSITION - STELLAR MHD AND COMPUTATIONAL ASTROPHYSICS
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1. ESA RESEARCH FELLOWSHIPS IN SPACE SCIENCE
(comunicado por Raimundo Lopes)
ESA Research Fellowships in Space Science
=========================================
The European Space Agency awards several postdoctoral fellowships
each year. The aim of these fellowships is to provide young
scientists, holding a PhD or the equivalent degree, with the means
of performing space science research in fields related to the ESA
Science Programme. Areas of research include astronomy and
astrophysics, planetary science, solar and solar-terrestrial
science, plasma physics and fundamental physics. The fellowships
are tenable at the European Space Astronomy Centre (ESAC) in
Villafranca del Castillo, near Madrid, Spain, or at the European
Space Research and Technology Centre (ESTEC) in Noordwijk,
Netherlands.
Astronomy and Astrophysics research opportunities with XMM-Newton
science staff at ESAC include: Research on high energy emission of
(massive) stars, X-ray binaries, galaxies, AGNs and high
resolution X-ray spectroscopy using XMM-Newton data [contact
Norbert Schartel (Norbert.Schartel@sciops.esa.int) for details].
Preference will be given to applications submitted by candidates
within five years of receiving their PhD. Candidates not holding
a PhD yet are encouraged to apply, but they must provide evidence
of receiving their degree before starting the fellowship.
The deadline for the 2009 call for applications is 1 October 2008.
More information on the ESA Research Fellowship programme in Space
Science, on the conditions and eligibility, as well as the
application form can be found on the internet at:
http://www.rssd.esa.int/fellowship
Yours sincerely,
XMM-Newton SOC
=============================================================
2. RESEARCHER IN SOFTWARE FOR RADIO ASTRONOMY WITHIN ASTROPHYSICS
(comunicado por Marcelos Borges)
Physics Department at the University Of Oxford
Vacancy Title: Researcher in Software for Radio Astronomy within
Astrophysics
Reference Number: DB08004
Job Description: We are seeking to appoint a physicist or software
developer to work on designing and developing novel algorithms for the
analysis of radio astronomical data. The Square Kilometre Array (SKA) is
an ambitious global project to design and build the largest radio
telescope in the world, with of order a million square metres of
collecting area, covering frequencies from 100 MHz to 25 GHz. The SKA
will make fundamental advances in cosmology, pulsars and gravitational
astrophysics, cosmic magnetism, and planet formation, as well as opening
up a huge new parameter space for unpredictable discoveries.
Anyone who thinks they may be interested in the job is encouraged to talk
to Dr Steff Salvini (email: stef.salvini@oerc.ox.ac.uk) about it.
Additional details can be found on the web at:
http://www.physics.ox.ac.uk/astro/jobs/
The application deadline is 01/09/2008
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3. CONCURSO NA UNIVERSIDADE FEDERAL DO ABC - VÁRIAS ÁREAS
(comunicado por Adriana Válio)
Caro(a) Senhor(a),
Gostaríamos de lhe informar que a UFABC (Universidade Federal do ABC)
está com concursos abertos para 84 vagas para docentes com título de
doutor em várias áreas do conhecimento. As inscrições encerram em 26
de agosto/2008. A UFABC possui atualmente vários cursos de graduação e
pós-graduação e seu primeiro campus está localizado em Santo
André-SP, com o segundo campus em fase de construção em São Bernardo
do Campo. Maiores informações sobre o concurso podem ser obtidas no
site www.ufabc.edu.br .
Atenciosamente,
UFABC
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4. ESO SPECTRAL ADVANCED DATA PRODUCTS
(comunicado por Rodolfo Smiljanic)
ESO Spectral Advanced Data Products
Como parte do projeto de disponibilizar para a comunidade dados reduzidos de
alto nível prontos para o uso científico, o ESO disponibilizou em novembro do
ano passado o chamado "UVES reprocessed data set".
Esse conjunto de dados consiste em todos os espectros públicos de fontes
pontuais obtidos com o UVES, desde o início de sua operação, reprocessados de
maneira homogênea com o pipeline UVES desenvolvido pelo ESO.
O UVES é um espectrógrafo echelle acoplado ao UT2 do VLT capaz de obter dados
a partir do corte atmosférico em 300 nm até ~ 1100 nm. O poder resolutor
máximo do UVES pode chegar a 80000 no azul e 110000 no vermelho.
O acesso aos dados reduzidos é uma grande oportunidade para utilizar dados
obtidos com um dos melhores espectrógrafos da atualidade.
Outros conjuntos de dados como "HARPS reprocessing", "GOODS FORS2
spectroscopy" e "zCOSMOS", também estão disponíveis.
A consulta à base de dados pode ser feita no endereco:
http://archive.eso.org/wdb/wdb/adp/ssa/form
Mais informações sobre o processamento dos dados UVES podem ser obtidas em:
http://www.eso.org/observing/dfo/quality/reproUVES/processing.html
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5. POSTDOCTORAL POSITION - STELLAR MHD AND COMPUTATIONAL ASTROPHYSICS
(comunicado por Rodolfo Smiljanic)
Postdoctoral Position -- Stellar MHD and Computational Astrophysics
CEA - Saclay, France
We invite applications for a five year post-doctoral position in
magnetohydrodynamics and stellar fluid and plasma dynamics in
support of the European ERC-StG project STARS2 (Simulations
of Turbulent, Active and Rotating Sun and Stars).
The STARS2 project aims at modelling on massively parallel supercomputers
in a self-consistent and three-dimensional way, the complex, time dependent
and nonlinear dynamics operating in the Sun and stars. In particular
we wish to characterize, study, and constrain the dynamical processes,
such as turbulence or dynamo action, acting in stellar convection
and/or radiation zones that are at the origin of the wide variety
of magnetic activity that is observed.
The position will be held in Service d'Astrophysique (SAp), CEA-Saclay,
France. SAp is a world class astrophysical and space science department
with more than 150 faculty and staff members, variously studying stellar
evolution and dynamics, astrophysical fluid dynamics, planets and stars
formation, multi-wavelength astronomy, cosmology, high energy astrophysics.
SAp is located about 15 km south of Paris (near Orsay). The growing
STARS2 team focuses mostly on multi-D stellar/solar MHD and dynamo
action. It is also interested in characterizing the influence of
dynamical processes on the evolution of stars via what is called
secular MHD and in improving 2-D mean field dynamo models by introducing
profiles deduced from 3-D simulations. Further the successful candidate
will also benefit from existing and productive scientific
collaborations with researchers in Paris, in France, in Europe,
and in USA (via the Memorandum of Understanding on Stellar Dynamos
between SAp and JILA, Colorado).
The scientific expertise of the candidate should be among one of
the following fields: convection, turbulence, MHD, dynamos in stars
or planets and computational astrophysics. The successful candidate
will build, compute and analyse sophisticated and realistic high
performance numerical simulations of the Sun and of stars of various
spectral types. To achieve these challenging goals, the candidate
will use and extend the 3-D MHD spectral MPI code ASH (anelastic
spherical harmonics), as well as the 2-D finite element mean field
dynamo code STELEM. The simulations computed within the STARS2
project will be performed on local (linux cluster),
national (CNRS-Idris, CEA-CCRT) and European (DEISA) supercomputer
centres. Additional information can be found at
http://irfu.cea.fr/Projets/STARS2/index.htm
.
Applicants should have a PhD in astrophysics, plasma physics or geophysics.
Prior post doctoral experience would be much appreciated but lack of
it should not prevent potential candidates from applying. The applicants
should have an outstanding record of research and publications,
some experience in managing small scientific projects on their own,
and real interest in computational astrophysics and applied mathematics.
Depending on experience the candidate could be asked to help the
PI co-supervise other less experienced postdocs or PhD students
hired within the STARS2 project.
This position funded for up to 5 years by the European Commission
via the grant ERC-StG STARS2 will be renewed on a yearly basis
depending on scientific progress and achievement. The gross
minimum salary will be 34,000EUR annually (~2,260EUR net per month),
and will be adjusted according to experience and family situation.
A minimum of 5,000 EUR per year of travel money will
also be provided, in addition to the usual funding support of
any French institution. Applications sent before 31 October 2008
will be given top priority, but applications will be considered
until the position is filled. The effective work should
begin as soon as possible and no later than March 2009.
To apply, please send a resume, list of publications,
statement of research interests and experience, and
arrange for at least three letters of reference to be sent to:
Dr Allan Sacha BRUN,
PI of the European (ERC-StG) Project STARS2,
CEA-Saclay,
DSM/IRFU/SAp, Bat 709
91191 Gif-sur-Yvette, Cedex
France \\
Email: sacha.brun@cea.fr;
Tel: +33 1 6908 7660 (Office), +33 1 6908 6577 (Fax)
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