Cosmo-pl

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cosmo-pl@cosmo.torun.pl

June 2006

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CMB postdocs: APC Paris 2yr; Copenhagen 2+1yr
by Boud Roukema 12 Jun '06

12 Jun '06

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 > > --------------------------------------------------------------------------- > PNC PNC PNC http://www.iap.fr/pnc/ PNC PNC PNC PNC > --------------------------------------------------------------------------- > 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 > > > > --------------------------------------------------------------------------- > PNC PNC PNC http://www.iap.fr/pnc/ PNC PNC PNC PNC > --------------------------------------------------------------------------- > > 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. > > > --------------------------------------------------------------------------- > PNC PNC PNC http://www.iap.fr/pnc/ PNC PNC PNC PNC > --------------------------------------------------------------------------- > > 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 > > --------------------------------------------------------------------------- > PNC PNC PNC http://www.iap.fr/pnc/ PNC PNC PNC PNC > --------------------------------------------------------------------------- > > 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. > > --------------------------------------------------------------------------- > PNC PNC PNC http://www.iap.fr/pnc/ PNC PNC PNC PNC > --------------------------------------------------------------------------- > > 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. > > --------------------------------------------------------------------------- > PNC PNC PNC http://www.iap.fr/pnc/ PNC PNC PNC PNC > --------------------------------------------------------------------------- > > 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. > > >

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