---------- Forwarded message ----------
> Date: Thu, 22 Feb 2007 13:04:36 +0100 (CET)
> 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 # 289 22 Fev. 2007
5) Public release of the VVDS-DEEP first epoch spectra
6) ESO Workshop on "Science with the VLT in the ELT era"
Garching near Munich, Germany, 8-12 October 2007
7) Workshop, From Quantum to Cosmos II,Bremen, Germany, June 10-13, 2007.
" Space-based Research in Fundamental Physics and Quantum Technologies"
8) XXIIIrd IAP Colloque, in Honour of Bernard Fort
"From giant arcs to CMB lensing: 20 years of gravitational distortion"
July 2 to Friday July 6, 2007 , IAP Paris
9) Conference ,Château de Blois, France, May 20-May 26 2007
"Matter and Energy in the Universe: from nucleosynthesis to cosmology"
10) Conference : "Frontiers of Nonlinear Physics" (FNP 2007) w
Nizhny Novgorod July 3 to July 9, 2007.
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5) Public release of the VVDS-DEEP first epoch spectra
The VIMOS VLT Deep Survey team (http://www.oamp.fr/virmos/) is pleased
to annonce the public release of a catalogue of 8981 spectra of
galaxies, stars and QSOs, selected to have 17.5 < I(AB) < 24.0 in the
VVDS 0226-04 field. The spectroscopic redshifts are measured in the
range 0 < z < 5, with a median redshift of about 0.76. The sample covers
0.5 deg2 of sky area. The on-line database gives access to the redshifts
and quality flags, to the multi-wavelength photometric information, as
well as to the images and VIMOS spectra. The data can be accessed via
http://cencosw.oamp.fr
Reference papers for the data are about: (a) the spectroscopy: Le Fevre
et al., 2005, AA, 439, 845, and Le Fevre et al., 2004, AA, 428, 1023,
(b) the imaging and photometry: Le Fevre et al., AA, 417, 839, McCracken
et al., 2003 , AA, 410, 17, Radovich et al., 2004, AA, 417, 51 and
Iovino et al., 2005, 442, 423, (c) the information system: Le Brun et
al., 2007, AA, in preparation.
For further information please contact: vincent.lebrun at oamp.fr,
laurence.tresse at oamp.fr.
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6) ESO Workshop on "Science with the VLT in the ELT era"
Garching near Munich, Germany, 8-12 October 2007
RATIONALE:
The first of the ELTs (Extremely Large Telescopes) now under study could see
first light in around 10 years when the ESO VLT will still be fully operational
and receiving new 2nd generation instrumentation and upgrades. Even before then
we will also have entered the ALMA (and JWST) era. This Workshop will provide a
forum for the ESO community to debate and provide valuable feedback on how it
expects the scientific use and required instrumentation of the VLT and VLTI to
evolve over this period. It is expected that the results will have a major
impact on the priorities to be set in the next ESO Call for VLT Instrument
Proposals planned to be issued in 2008.
Amongst the topics envisaged are:
-Science highlights illustrating unique VLT and VLTI capabilities
-Future research priorities recommended by Astronet,ESA/ESO Working Groups etc.
- New science capabilities offered by instruments to be installed in 2008-2012
(HAWK-I, X-Shooter, KMOS, SPHERE, MUSE, PRIMA, 2nd gen. VLTI)
- ELT science priorities and possible first light instruments
- VLT and VLTI synergies with ELT, ALMA, JWST...
- VLT and VLTI science priorities beyond 2014 and consequences for possible
specialization of telescopes, operational modes etc.
- Available resources and concepts for new 2nd generation VLT instruments
to be installed beyond 2014
FORMAT:
- Invited review/overview talks
- Contributed papers and posters
- Discussion sessions following each major topic
More details and registration at http://www.eso.org/vlt07
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7) Workshop, From Quantum to Cosmos II,Bremen, Germany, June 10-13, 2007.
" Space-based Research in Fundamental Physics and Quantum Technologies"
The purpose of this workshop is to highlight the emerging discipline of
space-based research in fundamental physics and demonstrate how this area of
modern science can provide the knowledge needed to address outstanding
questions at the intersection of physics, astronomy, and cosmology, thereby
leading to major advances in these fields.
More details at http://www.zarm.uni-bremen.de/Q2C2/.
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8) XXIIIrd IAP Colloque, in Honour of Bernard Fort
"From giant arcs to CMB lensing: 20 years of gravitational distortion"
July 2 to Friday July 6, 2007 , IAP Paris
We are please to announce the XXIIIrd IAP colloquium that will held at IAP
between July 2 and 6.
Each year, The Institut d'Astrophysique de Paris organizes a colloquium on a
different topic in cosmology and astrophysics
2007 will be the 65th anniversary of Prof. Bernard Fort and the 20th
anniversary of the first papers on the discovery of giant arcs.
To celebrate ths event, the XXIIIrd IAP colloquium will focus on gravitational
distortion: rings, giant arcs, weak lensing and cosmic shear, distortion of
CMB anisotropy maps.
More details on the meeting will be published soon. But we invite you
to register already at the following registration page
http://www.iap.fr/scripts/colloques/iap2007/regmenu.asp
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9) Conference ,Château de Blois, France, May 20-May 26 2007
"Matter and Energy in the Universe: from nucleosynthesis to cosmology"
http://confs.obspm.fr/Blois2007/index.htm
This is an announcement and call for papers for an international
conference which will be held in the Château of Blois, in
France's Loire Valley.
Matter and Energy in the Universe: from nucleosynthesis to
cosmology is articulated around our increasingly detailed
understanding of the processes involved in the creation of the
elements and about our increasingly confused picture of the
content of the Universe. The year 2007 fmarks the fiftieth
anniversary of two groundbreaking papers (the famous B2FH paper,
and also a slightly less well known paper by A. Cameron) which
finally put stellar nucleosynthesis on the map, and almost the
sixtieth anniversary of the first quantitative calculations of
big bang nucleosynthesis; although this latter paper turned out
to be fundamentally flawed insofar as nucleosynthesis is
concerned, it did lead directly to Alpher and Hermann's
prediction of the ubiquitous cosmic microwave background
radiation, whose detailed study using instruments on the COBE
satellite earned this year's Nobel prize for physics.
It thus seems appropriate to "stand back" and survey what has
been achieved, and (especially) to highlight the puzzles which
remain to be solved.
Matter and energy in the Universe? will be organised around a
number of basic themes, including:
- the contents of the Universe
- abundance determinations
- primordial nucleosynthesis
- stellar thermonuclear nucleosynthesis
- the nucleidic evolution of galaxies
- cosmological cosmic rays, galactic cosmic rays and stellar
energetic particles
- dark matter, dark energy: what do we really know, and what
can we surmise
- the future.
The conference will consist of plenary sessions for invited
indepth oral presentations (review talks and talks on specific
specialised topics), and contributed papers, in the form of
relatively short oral papers or posters. We will aim to
achieve a balance between review talks, provocative talks given
by recognized specialists, and shorter contributions, special
emphasis being placed on participation by younger researchers and
post-docs. If the need arises (i.e. if so many short papers are
proposed that plenary sessions are insufficient), parallel
sessions will be organised - please do not hesitate to contribute
your work - time can always be found!
This conference will be the 19th in a series of
international mulitidisciplinary meetings which have in the past
covered many topics in physics, astronomy and biology. All
sessions take place in the Château of Blois, a beautiful
renaissance castle which has housed many French kings, and
notably François 1st. Meals are served in the castle to all
participants, in order to encourage interaction between
scientists at all levels. Participation is limited to about
150 persons.
The detailed scientific programme is currently under
development; on the web site
http://confs.obspm.fr/Blois2007/index.htm you will find the
latest information, and if you urgently need information which is
currently not available on this site, you may contact L. M.
Celnikier, at the email address:
blois.confs at obspm.fr
The web site will be updated regularly, as new information
becomes available. Please login regularly.
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10) Conference : "Frontiers of Nonlinear Physics" (FNP 2007) w
Nizhny Novgorod July 3 to July 9, 2007.
The Conference is focused on recent progress in the interrelated fields of
nonlinear dynamics with applications to physical systems of different
origins. Conference scope covers the following subjects, including both
basic aspects and advanced applications:
* Nonlinear dynamics: Coherent and stochastic processes
* General problems of nonlinear waves: Solitons, collapses, and turbulence
* Nonlinear processes in plasmas and laser-plasma interactions
* Nonlinear and high-field optics
* Nonlinear acoustics
* Nonlinear processes and turbulence in fluid dynamics
* Nonlinear problems in geophysics
* Nonlinear problems in astrophysics and cosmology
* Nonlinearities and coherent phenomena in quantum systems
The conference program will include topical oral and poster sessions, and
a set of plenary lectures on interrelated topics.
The list of proposed MINI-SYMPOSIA includes:
* Physics of Cold Gases and Bose-Einstein Condensates
* Large Nonlinear Water Waves, with a Special Focus on Rogue Waves,
Wave Breaking and Remote Sensing
* Physics of Extreme Light: Novel Particle and Radiation Sources
* Turbulence in Fluids and Plasmas
* Nonlinear Processes in Photonic Crystals and Periodic Structures
* Quantum, Coherent, and Nonlinear Optics
* Laser Dynamics
* Supernovae and Shocks
* Semiconductor Optoelectronics and Teraherts Physics
The Conference will be held on board a comfortable boat cruising along
the Volga river from Nizhny Novgorod to Saratov and back from July 3 to
July 9, 2007.
All the relevant information concerned with our meeting,
the form for on-line pre-registration included, is also available
at the FNP 2007 Web-site: htt://www.fnp.sci-nnov.ru
witam cosmo-torun
http://cosmo.torun.pl/Cosmo/ToK070215RoughNotes
The arguments for the Light Dark Matter hypothesis look
impressive to me. E.g. the link between the LDM particle mass
and the neutrino mass.
If you don't understand the notes, well, probably most of it
is already in astro-ph, hep-ph, etc.
pozdr
boud
