From boud w astro.uni.torun.pl  Tue Apr 10 14:14:55 2007
From: boud w astro.uni.torun.pl (Boud Roukema)
Date: Tue, 10 Apr 2007 14:14:55 +0200 (CEST)
Subject: [Cosmo-torun] Diffusion PNC (fwd)
Message-ID: <Pine.LNX.4.64.0704101412550.27404@adjani.astro.uni.torun.pl>

hi cosmo-torun,

Several conferences (most announcements in English) from the PNC:

pozdr
boud



---------- Forwarded message ----------
> Date: Fri, 6 Apr 2007 11:02:23 +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 # 291                                            6 Avril  2007

   1) PostDoc , "Dynamics of Galaxies " , LAM (Marseille)
   2) Postdoc , GRBs with the SVOM satellite , LAM (Marseille)
   3) Postdoc , LAM ( Marseille ) , "Oscillations acoustiques des baryons
        dans le CFH-LS et les prochains sondages grand-champ"
   4) Postdoc, Paticle Astrophysics and String theory, Stockholm (Physics Dept.)
   5) Postdoc in Observational Cosmology , Portsmouth (UK)
   6) Postdoc positions at Instituto de Astrof?­sica de Canarias ( Spain )

   7) Summer School , "Formation and Evolution of cosmic Structure"
      Novicosmo 2007 , Novigrad-Cittanova , Croatia 10-21 September 2007
   8) SIGRAV graduate school in contemporary relativity and
      gravitational physics , VII edition : " The Dark side of the universe"
      Villa Olmo, Como, Italy , May 14-18, 2007
   9) Ecole de Physique des Astroparticules - I
      10 -15 septembre 2007, OHP, Saint Michel l'Observatoire
      ?La Physique des Astroparticules?

  10) Santa Fe Cosmology Summer Workshop, July 2-20
  11) Ecole Internationale d'Astrophysique Daniel Chalonge
      "Dark Matter, Dark Energy, CMB and LSS:
        Understanding the Physics of the Universe"
      16 -17-18 AUGUST 2007, Observatoire de Paris HQ, Paris campus
  12) workshop  : " future wide field weak lensing surveys for cosmology."
        April 24-25, 2007 , CPPM , Marseille.
  13) Conference " Data Analysis in Cosmology 2007 "
     July 9 - 12, 2007 ,  Santander (Spain)
  14) Third Sino-French conference:"Origins". Paris, Sevres 15-20 octobre 2007



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   7) Summer School , "Formation and Evolution of cosmic Structure"
      Novicosmo 2007 , Novigrad-Cittanova , Croatia 10-21 September 2007

   Motivations:
   The goal of understanding the formation and evolution of the cosmic
   structures in the Universe drives current advances in observational
   cosmology. Over the last decade tremendous progress has been made in the
   direct observational study of structures to look back times covering over
   90% of the age of the Universe. In the current paradigm, cosmic structure
   grows through gravitational instability which acts to boost small initial
   fluctuations, seeded from quantum fluctuations during the inflationary phase
   of the Universe. Dark matter haloes are built up which host ordinary baryons.
   These blossom into luminous galaxies. While the evolution of the dark matter
   follows simple physics, namely gravity, our knowledge has significant gaps
   when it comes to describing the luminous, baryonic component of the Universe;
   this ignorance becomes spectacular in the case of the very first "luminous"
   objects which lit up the Universe at the end of the Dark Ages. Complex
   physical processes need to be considered. Through the use of increasingly
   sophisticated computer simulations, the first realistic attempts to model the
   process of galaxy formation over the history of the Universe are now being
   made.

   The purpose of the School is to provide to young scientists with the
   opportunity to widen their knowledge of cosmology and extragalactic
   astrophysics and to become acquainted with key recent theoretical and
   experimental results, as well as to foster an interactive exchange among
   participants. We seek to establish an atmosphere in which observers and
   theorists will review, confront and discuss with young scientists recent
   progress and future directions.
   The School is then aimed at PhD students and young scientists with a Post-doc
   experience of less than 4 years. Outstanding upper level undergraduates may
   also be considered. Each subject will be covered by 3 lectures of 2 hours
   each, delivered by a scientist who has made significant contributions to the
   topic. Everyday there will be a special seminar on a particularly important
   subject in the field of Cosmology.

   http://www.novicosmo.org/

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   8) SIGRAV graduate school in contemporary relativity and
      gravitational physics , VII edition : " The Dark side of the universe"
      Villa Olmo, Como, Italy , May 14-18, 2007

      http://www.centrovolta.it/sigrav/

   The SIGRAV Schools are directed to PH.D. students and young Post-Docs in
   Physics, Astronomy and Mathematics who are interested in widening their
   knowledge in the fields of Physical Cosmology, Relativistic Astrophysics,
   General Relativity, Experimental Gravity and the Modern Quantum Theories of
   Gravitation. The Schools wish to introduce students to current problems,
   highlighting their importance and potential scientific impact. Lecturers
   will report on theoretical, observational and experimental aspects of the
   research, reviewing latest achievements in the field.

   PROGRAM

   Studying the physical and astrophysical properties of the dark matter and
   dark energy components of the Universe is a crucial step towards the
   ultimate goal of unveiling their nature. A large number of  present and
   future experiments and observations is indeed devoted to this goal. The
   school will focus on the theoretical and experimental/observational
   aspects of this problem, as seen from both its cosmological and particle
   physics sides.


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   9) Ecole de Physique des Astroparticules - I
      10 -15 septembre 2007, OHP, Saint Michel l'Observatoire
      Â? La Physique des AstroparticulesÂ?

     Nous avons le plaisir de vous annoncer l'école thématique du CNRS
     intitulée Ecole de Physique des Astroparticules
     elle se tiendra ?  l'OHP (Saint Michel l'Observatoire) du 10 au15 septembre
     2007.
 	hhttp://www.cpt.univ-mrs.fr/~cosmo/WEB_EAP_07/EcoleAP-OHP07.html
     Les organisateurs
     B. Degrange (LLR) - J. Lavalle (CPPM) - R. Triay (CPT)

    Contexte Scientifique
     La physique des astroparticules investit aujourd'hui des problématiques
     aussi diverses que l'origine et la propagation des particules-rayonnements,
     la masse des neutrinos, la proportion d'anti-mati?re dans l'univers,
     l'existence et l'origine de la mati?re noire, l'invariance de Lorentz,
     la physique des processus gravitationnels ?  champs forts, etc. Ces
     derni?res années, les expériences associées ?  cette thématique se   sont
     considérablement développées et leurs résultats suscitent toujours   plus
     d'enthousiasme. Dans la perspective d'assurer une formation
     conséquente dans ce champ explicitement interdisciplinaire, le programme
     a une tendance assez généraliste, il mettra en évidence les point
     forts des th?mes suivants : Neutrino -- Gamma et GRB -- Sources et
     processus d'UHE  -- Mati?re noire -- Rayons cosmiques et
     accél?rateurs cosmiques. Il vise ? couvrir autant les aspects
     d'observation que théoriques de ces problématiques.

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  10) Santa Fe Cosmology Summer Workshop, July 2-20

   The Santa Fe topical workshop for 2007 will concentrate on recent
   developments in cosmology, especially those related to current and expected
   observational advances, including the cosmic microwave background,
   large-scale structure, galaxies and clusters, and dark matter and
   energy/early universe. The format will emphasize discussion with some formal
   pedagogical review and related talks as appropriate. Generally speaking we
   would like to reserve the largest fraction of the day for discussion and
   informal meeting. To encourage this informality and discussion, attendance
   will be limited to about 80 participants.


    There will be no registration fee and highly subsidized housing will
   be provided (the precise cost estimates will be available soon, but
   are typically $150/room/week, $50/week for students). Travel support
   will not be available.

   To register for the meeting and to make suggestions for the scientific
   program, go to the Workshop website at

    http://t8web.lanl.gov/people/salman/sf07/

   We will be filling spaces on a rolling basis, so you are strongly
   advised to register as soon as possible, and preference will be given
   to those who register before April 05, 2007.


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  11) Ecole Internationale d'Astrophysique Daniel Chalonge
      "Dark Matter, Dark Energy, CMB and LSS:
        Understanding the Physics of the Universe"
      16 -17-18 AUGUST 2007, Observatoire de Paris HQ, Paris campus

      The Colloquium is within the astrofundamental physics spirit of the
     Chalonge School, this time focalized on recent observational and
     theoretical progress on dark matter, dark energy, including neutrinos
     and sterile neutrinos, CMB data and the theory of the early universe
     with predictive power.
     The Topics are: Observational and theoretical progress in deciphering
     the nature of dark matter and dark energy . CMB and Large scale structure
     formation. Inflation after WMAP (in connection with the CMB and LSS data),
     quadrupole suppression and initial conditions; quantum effects.
     CMB polarization, primordial magnetic fields effects. Neutrinos in
     cosmology.

     In summary, the aim of the meeting is to put together real cosmological
     data and hard theory predictive approach connected to them.

     An exhibition will retrace the 15 years of activity of the Chalonge School
     and of George Smoot participation to the School along these 15 years.

     All informations about the Meeting, including the general timing and  the
     Programme and Lecturers of the Colloquium  and registration information
     are displayed at the chalonge school web site

      http://chalonge.obspm.fr/colloque2007.html

      Early Registration is strongly encouraged
      Chalonge.Ecole at obspm.fr


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  12) workshop  : " future wide field weak lensing surveys for cosmology."
        April 24-25, 2007 , CPPM , Marseille.

    The idea is to allow discussion between scientists working on current or
    future (either approved or still in development) wide field weak lensing
    surveys.
    Although a good understanding on the statistical limits of weak lensing
    exist, systematics are still to be explored in details and need to be fully
    understood (shape measurements, understanding and modeling the PSF
    correction, but also photometric redshifts and its requirements for
    calibration) in order to optimize the survey and ultimately give
    the best cosmology constraints.
    Furthermore, with the current and future lensing surveys there will be
    other lensing interests than measuring cosmic shear to probe cosmology, so
    it would also be very useful to discuss these science cases
    and understand their requirements.

    I wish you can come and participate to this workshop. So please let me know
    if you are able to attend and give me the title of your oral contribution
    ideally before March 23, 2007.

    The venue of the meeting will be at CPPM on the  Marseille-Luminy campus
    http://marwww.in2p3.fr/
    More details on the meeting, venue, list of participants can be found at
    http://www.oamp.fr/cosmology/weaklensing2007/

    Jean-Paul Kneib on behalf of the SOC: Gary Bernstein, Anne Ealet ,
    Yannick Mellier, Bruno Milliard, Alexandre Refregier,  Jason Rhodes,
    Ludovic van Waerbeke,

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  13) Conference " Data Analysis in Cosmology 2007 "
     July 9 - 12, 2007 ,  Santander (Spain)

   The goal of the conference is to bring together
   experts on techniques and methodologies for data
   analysis which could be applied to cosmological studies.
   In particular the meeting will focus on:
   * Statistical analysis (Bayesian statistics, PCA,ICA, etc)
   * Neural networks
   * Multi-scale analysis
   * Inverse problem
   * Morphological analysis
   * Data fusion

   Registration is now open through the meeting's web page:
     http://max.ifca.unican.es/webcmb/dac07/
   There will be a limited number of contributed talks
   and posters.More details on the meeting can be found
   in the previous web page.
   Please, circulate this announcement to anyone who
   might be interested.
   Contact:
   For practical questions about hotel reservation and
   travel information, please write to:
     congresossantander at viajeseci.es
   For general questions, please write to:
       dac007 at ifca.unican.es
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  14) Third Sino-French conference:"Origins". Paris, Sevres 15-20 octobre 2007

   La troisieme conference franco-chinoise aura lieu a Paris (Sevres),
   du 15 au 20 octobre 2007, sur les themes: origines.

   La thematique "Origines" (de la matiere: cosmologie ; de la vie : planetes
   extra-solaires) est une des fortes priorites des agences europennes et
   chinoises en astronomie/astrophysique. C'est une des grandes questions du
   21me siecle pour laquelle d'etonnants progres ont ete realises ces
   dernieres annees: decouvertes des planetes extrasolaires, de
   l'acceleration de l'Univers et de l'energie noire, des anisotropies du
   fond de rayonnement cosmologique, et des processus de formation des galaxies,
   pour lesquelles de tres forts investissements en instrumentation sol et espace
   ont ete engages.
                   voir le site: http://origins.obspm.fr

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From boud w astro.uni.torun.pl  Wed Apr 11 16:40:22 2007
From: boud w astro.uni.torun.pl (Boud Roukema)
Date: Wed, 11 Apr 2007 16:40:22 +0200 (CEST)
Subject: [Cosmo-torun] Re:
	=?iso-8859-2?q?Szko=B3a_fizyki_teoretycznej_dla_doktorant=F3w?=
In-Reply-To: <004701c760f1$4c4602f0$a50a0a0a@IBMFEB5001D7D6>
References: <004701c760f1$4c4602f0$a50a0a0a@IBMFEB5001D7D6>
Message-ID: <Pine.LNX.4.64.0704111635170.26475@adjani.astro.uni.torun.pl>

Witam Marek,

Średnie oczekiwamy na około 1.55 doktorantów toruńskie na rocznym
szkołu - na założenie 3 szkoły w następnych 3 latach, mamy 
[2.5 + 2.0 + (0.05*3) ] /3 = 1.55  według interpretację czestotliwościową,
lub inaczej, może poprostu to traktować jako P( ) bayesowska.

pozdr
boud



On Wed, 7 Mar 2007, zralek wrote:

> Szanowni Panstwo,
>

> Jak wiekszosc z Panstwa wie na ostatnim spotkaniu naszego
> porozumienia 19 lutego w Warszawie zdecydowalismy, iz bedziemy
> organizowac Szkoly fizyki teoretycznej dla doktorantow z fizyki
> czastek, astrofizyki i kosmologii. Na takiej tygodniowej Szkole,
> organizowanej cyklicznie przez wszystkie grupy naszego porozumienia,
> odbywalyby sie serie wykladow specjalistycznych, ktore trudno
> przeprowadzic w poszczegolnych osrodkach albo ze wzgledu na mala
> liczbe sluchaczy albo brak kadry.  Po pierwsze, prosze o komentarz w
> tej sprawie wszystkich, ktorzy nie byli obecni w Warszawie. I sprawa
> druga, zgodnie z naszymi ustaleniami urzejmie prosze o podanie ilu
> doktorantow mogloby brac udzial w takiej Szkole z kazdego Osrodka.

> Lacze serdeczne pozdrowienia,
> Marek Zralek
>