Results 91 to 100 of about 77,561 (213)
Observatoires du développement, observatoires pour le développement
L'ouvrage porte sur l'analyse des problèmes conceptuels (théoriques ou méthodologiques) et politiques posés par la création et le fonctionnement d'observatoires du développement dans les pays du Sud. Il s'agit d'abord d'identifier les diverses fonctions des retours sur le terrain ; puis de distinguer différents types d'observatoires, par exemple ceux ...
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The Chalonge 14th Paris Cosmology Colloquium was held on 22-24 July 2010 in Paris Observatory on the Standard Model of the Universe: News from WMAP7, BICEP, QUAD, SPT, AMI, ACT, Planck, QUIJOTE and Herschel; dark matter (DM) searches and galactic ...
de Vega, H. J. +2 more
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LWDM (Warm Dark Matter) is progressing impressively.The galactic scale crisis and decline of LCDM+baryons are staggering. The 16th Paris Chalonge Colloquium 2012 combined real cosmological/astrophysical data and hard theory predictive approach in the ...
de Vega, H. J. +2 more
core
Systèmes d'information et observatoires [PDF]
Contact: Jean Christophe Desconnets, jean-christophe.desconnets@teledetection.fr & Thérèse Libourel, libourel@lirmm.fr ; National ...
Libourel, T. +2 more
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Observatoire économique du Vercors
Blanchet Anne. Observatoire économique du Vercors. In: Revue de géographie alpine, tome 78, n°4, 1990. pp. 96-99.
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We have developed a machine learning algorithm capable of detecting ‘out-of-domain data’ for trustworthy cosmological inference. By using data from two separate suites of cosmological simulations, we show that our algorithm is able to determine whether ...
Tregidga Ethan +3 more
doaj +1 more source
DO MARKET LISTING AND SIZE ENTAIL BEHAVIOURAL DIFFERENCES? [PDF]
It is possible to study companies according to their methods of gaining access to finance, and in particular the stock market. Two approaches are possible.
Bernard BELLETANTE, Bernard PARANQUE
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Numerical simulations of oscillating and differentially rotating neutron stars
Context. The remnants of binary neutron star mergers are expected to be massive, rapidly rotating stars whose oscillations produce gravitational waves in the kilohertz band. The degree of differential rotation and the rotation profiles strongly influence
Jaraba Santiago +2 more
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DENIS-P J104814.7-395606.1: An M9 dwarfs at about 4 pc
We present the discovery of a previously unknown member of the immediate solar neighbourhood, DENIS-P J104814.7-395606.1 (hereafter DENIS 1048-39), identified while mining the DENIS database for new nearby stars.
Alard, C. +10 more
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