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LWDM (Warm Dark Matter) is progressing impressively.The galactic scale crisisand decline of LCDM+baryons are staggering. The 16th Paris Chalonge Colloquium2012 combined real cosmological/astrophysical data and hard theory predictiveapproach in the LWDM Standard Model. News and reviews fromACT,WMAP,SPT,QUIET,Planck,Herschel,JWST,UFFO,KATRIN and MARE experiments;astrophysics, particle and nuclear physics WDM searches, galactic observations,related theory and simulations, with the aim of synthesis and clarification.Here highlights by P Biermann, C Burigana, C Conselice, A Cooray, H de Vega, CGiunti & M Laveder, J Kormendi & K Freeman, E Ma, J Mather, L Page, G Smoot, NSanchez. Summary and conclusions by de Vega, Falvella and Sanchez. Data confirmprimordial CMB gaussianity. Effective (Ginsburg-Landau) Inflation theorypredicts r about 0.04-0.05, negligeable running of ns, the inflation energyscale (GUT scale) and the set of CMB observables in agreement with the data.WMAP9 and Planck measurements are compatible with one or two Majorana sterileneutrinos in the eV mass scale. Cored (non cusped) DM halos and keV WDM arestrongly favored by theory and observations, Wimps are strongly disfavoured.LambdaCDM with baryons do not work at small scales. Inside galaxy cores,quantum WDM effects are important. Quantum WDM calculations (Thomas-Fermi)provide galaxy masses, velocity dispersions and cored profiles and their sizesin agreement with observations. A WDM fermion of about 2 keV naturallyreproduces galaxy, large scale and cosmological observations. WDM keV particlesdeserve dedicated astronomical and laboratory searches, theoretical work andnumerical simulations. KATRIN can be adapted to look to keV scale sterileneutrinos. It will be a fantastic discovery to detect dark matter in betadecay. Photos of the Colloquium are included

Towards the Chalonge 17th Paris Cosmology Colloquium 2013: highlights and conclusions of the Chalonge 16th Paris Cosmology Colloquium 2012