Witam cosmo-pl,
Chyba między nami nie wiemy wiele kandydaci, ale kto wie...
Zobacz na dolu:
4) postdoc @APC 2yr CMB Analysis -> kontakt jest Radek Stompor :)
5) postdoc @Copenhagen CMB 2+1yr
pozdr
boud
> ---------- Forwarded message ----------
> Date: Fri, 9 Jun 2006 23:26:01 +0200 (CEST)
> From: Programme National de Cosmologie <pnc at iap.fr>
> To: Programme National de Cosmologie <pnc at iap.fr>
> Subject: Diffusion PNC
>
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> message # 273 9 juin 2006
>
>
> 1) Atelier PNG , 26 juin 2006 de 9h a 18h Paris-Jussieu
> " L'évolution des galaxies ? l'?re des grands relevés"
> 2) Workshop sur l'inflation , 03-13 juillet 2006 , IAP Paris
> 3) CRAL-Conference Series I , 10-14 July 2006 , Lyon - FRANCE
> CHEMODYNAMICS: from first stars to local galaxies
> 4) Post-doctoral position in CMB data analysis - APC, Paris, France
> 5) Post Doctoral position in CMB science, DNSC , Copenhagen, Denmark
>
>
>
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>
> 1) Atelier PNG , 26 juin 2006 de 9h a 18h Paris-Jussieu
> "L'évolution des galaxies ? l'?re des grands relevés"
>
> Cet atelier sera centré sur les problématiques actuelles concernant
> l'évolution des galaxies sur une echelle de temps cosmologique. L'idée
> est de passer en revue, lors de cette journée, différentes questions
> "clé" qui peuvent etre testées actuellement par l'analyse des grands
> relevés extragalactiques de l'univers proche et lointain ; en relation
> bien sur avec les derniers développements concernant les simulations
> numériques de la formation et de l'évolution des galaxies, ainsi que
> les mod?les de synth?se de populations stellaires.
>
> Le programme préliminaire est accessible ? cette URL:
>
> http://www.ast.obs-mip.fr/users/contini/SF2A/SF2A_PNG_06/prog-PNG_2006.html
>
> Il comprend les exposés de revue suivants:
>
> * Models of galaxy formation and evolution : Julien Devriendt (CRAL - Lyon)
>
> * The local universe as seen by the SDSS : Jarle Brinchmann
> (Université de Porto - Portugal/LA2T - Toulouse)
>
> * Dynamics of galaxies up to z~1 : François Hammer (GEPI - Paris)
>
> * Large spectroscopic surveys : Thierry Contini (LA2T - Toulouse)
>
> * Large infrared surveys : Jean-Loup Puget (IAS - Paris)
>
> * Physical properties of galaxies derived from SED fitting :
> Stéphane Arnouts (LAM - Marseille)
>
> * The next generation of large surveys : Olivier Le F?vre (LAM - Marseille)
>
> Nous invitons les participants intéressés a venir presenter leurs travaux
> sous forme de contributions orales et de posters. Les demandes de presentation
> doivent etre envoyees avant le 10 juin sur le site des Journees de la SF2A:
>
> --> http://aramis.obspm.fr/~sf2a/2006
>
> Notez que les resumes seront references dans ADS. Ils doivent etre ecrits en
> anglais. Il est aussi recommande de présenter des transparents en anglais
> meme pourles presentations en francais, pour faciliter l'acces aux
> non-francophones.
>
> Pour plus de renseignements, contacter:
> Thierry Contini - contini at ast.obs-mip.fr ou
> Guilaine Lagache - guilaine.lagache at ias.u-psud.fr
>
> Le PNG soutiendra les missions des membres du PNG pour se rendre a la
> SF2A s'ils participent a la journee PNG, jusqu'a un montant maximal de 400E
> (dont 50E pour les frais d'inscription). Comme l'an dernier les missions
> seront remboursees globalement, directement par l'INSU sur le budget 2006
> des laboratoires. Il est donc demande a tous les participants PNG
> d'envoyer une copie de leur feuille de remboursement apres la mission,
> indiquant le detail du remboursement payé par le laboratoire. Ces documents
> devront parvenir a Annie Robin (Besancon) des que le remboursement est
> effectué.
>
>
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>
> 2) Workshop sur l'inflation , 03-13 juillet 2006 , IAP Paris
>
> un workshop sur l'inflation suivra le colloque de l'IAP "Inflation+25"
> (http://www.iap.fr/col2006/). Il se tiendra du 03/07/2006 au 13/07/2006
> ? l'IAP. A cette occasion, nous organisons deux ? trois séminaires de
> 45 mn par jour sur ce th?me. Si vous souhaitez participer en tant qu'orateur,
> veuillez nous contacter le plus vite possible (col2006 at iap.fr) car il reste
> un nombre tres limite de places.
>
> Cordialement
> Jerome Martin pour le LOC
>
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>
> 3) CRAL-Conference Series I , 10-14 July 2006 , Lyon - FRANCE
> CHEMODYNAMICS: from first stars to local galaxies
>
> Final ANNOUNCEMENT
> The deadline for abstract submission is May 31
> The deadline for registration is June 9
>
>
> Dear colleague,
>
> we are pleased to announce the first
> international conference in the CRAL Conference Series,
> titled "Chemodynamics: from first stars to local galaxies"
> to be held July 10-14 2006 in the beautiful city of Lyon, France.
>
> There will be five large sessions:
> * First stars and early metal production
> * Galaxy winds and inter galactic medium enrichment at intermediate
> redshifts
> * The intra cluster medium as a laboratory for galaxy chemodynamics
> * Self-regulation processes in the interstellar medium of local and not
> so local galaxies
> * Detailed stellar feedback processes in the Milky Way
>
> Reviewers and invited speakers for these 5 sessions will include :
>
> * Andrea Ferrara, Vanessa Hill, Raffaella Schneider, Raphael Hirschi
> * Anthony Aguirre, Dawn Erb, Philip Richter
> * Sabine Schindler, Stefano Borgani, Brad Gibson
> * Greg Bryan, Adrianne Slyz, Françoise Combes, Fabian Walter
> * Nikos Prantzos, Kim Venn, Keiichi Wada, Julien Devriendt, Hervé Wozniak
> * and Colin Norman for the summary talk.
>
> Registrations are opened, and we *encourage* you to apply *early*.
> See our web site for information and registration:
> http://cralconf.univ-lyon1.fr
>
> Looking forward to seeing you in Lyon!
>
> The Local Organizing Committee
> ====================
> Scientific Rationale:
> ====================
> Chemodynamical evolutionary models were invented to provide a global
> dynamical description of the interplay between the major physical
> components of galaxies: in a gravitational potential essentially dominated
> by dark matter, stars structure the multi-phase ISM through radiation,
> winds and supernovae and enrich it in heavy elements. From a cosmological
> perspective, these models should begin with the formation of the first
> structures. Heavy elements formed by the very first generation of stars
> pollute the early IGM, thus allowing for more efficient radiative cooling
> during the formation of the next astrophysical objects: galaxies are born.
>
> Chemodynamical models yield quantitative predictions for the observable
> consequences of the violent physical mechanisms that occur within galaxies.
> Perhaps the most remarkable one is that the ISM self-regulates which implies
> that the star formation rate in galaxies is ultimately controlled by feedback
> processes. In other words, they argue that observations over a wide range of
> wave-lengths should be linked: X-ray emission of the relatively low density
> supernova heated gas that permeates the entire ISM, impacts on the far
> infrared cooling emission lines present in the densest molecular cores.
>
> Forthcoming instruments such as MUSE, JWST, ALMA and SKA will shed light on
> the high redshift Universe population of proto-galaxies whereas XMM,
> Chandra, GALEX and Spitzer are now probing galaxies panchromatically at
> lower redshifts. On the other hand, current computational power allows
> us to numerically explore the
> first ages of structure formation. It also makes it possible to follow in
> greater detail the chemodynamics of individual objects. As a consequence, we
> now feel that we lie at a crossroad between two epochs, and the time
> has come to review where chemodynamical models stand.
>
> Scientific Organising Committee
> ===============================
> Greg Bryan
> Françoise Combes
> Andrea Ferrara
> Bruno Guiderdoni
> Gerhard Hensler
> Max Pettini
> Eline Tolstoy (chair)
> Keiichi Wada
>
> Local Organising Committee
> ==========================
> Nicolas Champavert, Hél?ne Courtois, Julien Devriendt, Eric Emsellem(chair),
> Jean-François Gonzalez, Gérard Massacrier, Jimmy Paillet, Hervé Wozniak
>
> Practical Issues
> ================
> We encourage you to register as soon as possible as we will limit the total
> number of participants :
> ** the deadline for submitting an abstract is May 31
> ** the deadline for registering is June 9.
>
> We also encourage you to reserve your hotel a.s.a.p.
> since July is certainly a busy time in Lyon
> (and a nice period for sight-seeing).
>
> Fees are 250 euros (including the conference dinner, and proceedings), and
> 300 euros for late payment (after June 9).
> The fees can be paid BEFORE June 9, via bank wiring
> (a procedure to pay via Credit Card will soon be implemented):
> see the registration section on the web site for details.
>
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>
> 4) Post-doctoral position in CMB data analysis - APC, Paris, France
>
> We are seeking a post-doctoral researcher to work in the area of data
> analysis of next generation Cosmic Microwave Background polarization
> data sets.
> The post-holder is expected to share his/her time between a development
> of general, experiment-non-specific methods and software tools, and
> preparations for, and data analysis of, actual experimental data
> sets. These will include the data sets produced by the balloon-borne
> experiment, EBEx and the ground-based observation, PolarBear. The
> possibility will also exist for the selected applicant to get involved
> in other projects currently undertaken by the members of the CMB group
> at APC, including work on Planck-HFI.
> The successful candidate should have a PhD in astronomy or physics,
> thorough knowledge of modern, physical cosmology, background in statistical
> methods, and experience in computer programing. S/he will be associated with
> the ADAMIS (http://www.apc.univ-paris7.fr/APC_CS/Recherche/Adamis/) group at
> APC and is expected to be primarily working with dr. R. Stompor and others
> members of this group. However, interactions with a broader scientific
> community within APC and Paris will be also encouraged.
> APC (http://www.apc.univ-paris7.fr) is a new, dynamic institute associated
> with the Universite Paris-7 and soon to be located on a new campus of the
> University within the city limits of Paris. The members of APC are
> involved in a number of national and international projects, and play a
> significant role in many of them.
> The institute provides a friendly and lively place to work and a
> scientifically exciting and stimulating environment to conduct research
> in.
> The post is for two years with a starting date preferably on or around
> October, 01, 2006. The salary is around 2,200 Euros. A benefit package and
> support for travel and other research expenses will be also provided.
> The application deadline is on May, 31, but late applications will be
> considered until the post is filled. Applications (preferably in electronic
> form) and all
> other correspondence should be sent to:
> R. Stompor
> 11, place M. Berthelot
> 75231 Paris, Cedex 5
> France E-mail: radek at apc.univ-paris7.fr
> In addition applicants should arrange for two letters of reference to be
> sent directly to the above address.
> Requests for any additional information as well as informal inquiries can
> be made to:
> radek at apc.univ-paris7.fr7
> The Laboratory is an Equal Opportunity Employer.
>
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>
> 5) Post Doctoral position in CMB science, DNSC, Copenhagen, Denmark
>
> The Danish National Space Center (DNSC) and the Niels Bohr Institute (NBI)
> announce a joint postdoctoral position in Cosmic Microwave Background (CMB)
> research. Applicants must document a solid theoretical background in
> cosmology, astrophysics or physics and well-developed computer skills.
> The successful applicant is expected to participate in the scientific
> preparation for and exploitation of the upcoming ESA Planck Surveyor Mission
> aimed at measuring the anisotropy and polarization of the CMB, a mission in
> which DNSC and NBI are participating. The main task of the postdoctoral
> fellow will be to conduct and publish research in CMB-related science and to
> participate in the development of methods for extraction of CMB signals from
> the Planck data. The fellow is expected to work closely with people at
> the DNSC (www.spacecenter.dk) and at the NBI (www.nbi.ku.dk).
> Interaction with researchers at the new Dark Cosmology Center
> (www.dark-cosmology.dk) is also foreseen.
>
> The postdoctoral fellowship is for 2 years with the possibility for
> a 3-year extension.
> A Ph.D. degree and relevant research experience are required.
>
> Terms of appointment and salary are set by agreement between the Ministry
> of Finance and AC (the Danish Confederation of Professional
> Associations of Academics in the State).
>
> The applications must be in English and must include:
> - Research Plan
> - Curriculum Vitae
> - A complete list of publications indicating a maximum of 5 papers of
> particular interest
> - 3 copies of each of the selected papers. In case of publications with more
> than one author, a statement regarding the applicant's contribution shall
> be provided
> - Documentation for teaching experience and other qualifications
>
> The applications will be evaluated by an assessment committee. Applicants
> may be summoned for an interview. Any potential applicant is invited to
> apply irrespective of age, sex, race religion or ethnic background. Further
> inquiries about research plans, facilities and staffs should be directed to
> the Principal Investigator of the Planck Reflectors Hans Ulrik
> N?rgaard- Nielsen, DNSC (hunn at spacecenter.dk).
> The application (original plus 3 copies, all with enclosures and selected
> papers) must be send to Director Eigil Friis- Christensen, DNSC, Juliane
> Maries Vej 30, DK- 2100 Copenhagen , Denmark.
> The deadline for application is August 1 2006 at noon. Material received
> after this time will not be considered.
> Applications submitted by email will not be accepted.
>
>
>
