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1. PI3K Mutation Profiles on Exons 9 (E545K and E542K) and 20 (H1047R) in Mexican Patients With HER‐2 Overexpressed Breast Cancer and Its Relevance on Clinical–Pathological and Survival Biological Effects.

2. A White Paper on keV Sterile Neutrino Dark Matter

3. Congenital heart disease in the ESC EORP Registry of Pregnancy and Cardiac disease (ROPAC)

5. The Dark Matter distribution function and Halo Thermalization from the Eddington equation in Galaxies

7. Ameyali: Evaluacion de la usabilidad de la plataforma Integral para el control y monitoreo del servicio de agua potable en comunidades rurales bajo la escala de Sus/Ameyali: Evaluation of the usability of the Integral platform for the control and monitoring of the drinking water service in rural communities under the scale of Sus

8. Equation of state, universal profiles, scaling and macroscopic quantum effects in Warm Dark Matter galaxies

9. The Future of Neutrino Mass Measurements: Terrestrial, Astrophysical, and Cosmological Measurements in the Next Decade. Highlights of the NuMass 2013 Workshop. Milano, Italy, February 4 - 7, 2013

10. Observational rotation curves and density profiles vs. the Thomas-Fermi galaxy structure theory

11. Warm dark matter primordial spectra and the onset of structure formation at redshift z

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

13. Towards the Chalonge Meudon Workshop 2013. Highlights and Conclusions of the Chalonge Meudon workshop 2012: warm dark matter galaxy formation in agreement with observations

14. Dark matter in galaxies: the dark matter particle mass is about 7 keV

15. Quantum WDM fermions and gravitation determine the observed galaxy structures

16. Fermionic warm dark matter produces galaxy cores in the observed scales because of quantum mechanics

17. Towards the Chalonge 16th Paris Cosmology Colloquium 2012: Highlights and Conclusions of the Chalonge 15th Paris Cosmology Colloquium 2011

18. Cosmological evolution of warm dark matter fluctuations I: Efficient computational framework with Volterra integral equations

19. Cosmological evolution of warm dark matter fluctuations II: Solution from small to large scales and keV sterile neutrinos

20. Role of Sterile Neutrino Warm Dark Matter in Rhenium and Tritium Beta Decays

21. Warm dark matter in the galaxies:theoretical and observational progresses. Highlights and conclusions of the chalonge meudon workshop 2011

22. Highlights and Conclusions of the Chalonge 14th Paris Cosmology Colloquium 2010: `The Standard Model of the Universe: Theory and Observations'

23. Highlights and Conclusions of the Chalonge 13th Paris Cosmology Colloquium

24. Highlights and Conclusions of the Chalonge Meudon Workshop Dark Matter in the Universe

25. The Effective Theory of Inflation and the Dark Matter Status in the Standard Model of the Universe

26. The mass of the dark matter particle from theory and observations

27. Forecast for the Planck precision on the tensor to scalar ratio and other cosmological parameters

28. The pre-inflationary and inflationary fast-roll eras and their signatures in the low CMB multipoles

29. Constant surface gravity and density profile of dark matter

30. Higher order terms in the inflaton potential and the lower bound on the tensor to scalar ratio r

31. Model independent analysis of dark matter points to a particle mass at the keV scale

32. The Effective Theory of Inflation in the Standard Model of the Universe and the CMB+LSS data analysis

33. Quantum slow-roll and quantum fast-roll inflationary initial conditions: CMB quadrupole suppression and further effects on the low CMB multipoles

34. The dark matter transfer function: free streaming, particle statistics and memory of gravitational clustering

35. The CMB Quadrupole depression produced by early fast-roll inflation: MCMC analysis of WMAP and SDSS data

36. Constraints on dark matter particles from theory, galaxy observations and N-body simulations

37. MCMC analysis of WMAP3 and SDSS data points to broken symmetry inflaton potentials and provides a lower bound on the tensor to scalar ratio

38. New Inflation vs. Chaotic Inflation, Higher Degree Potentials and the Reconstruction Program in light of WMAP3

39. CMB quadrupole suppression: I. Initial conditions of inflationary perturbations

40. CMB quadrupole suppression: II. The early fast roll stage

41. Dilute and Collapsed Phases of the Self-Gravitating Gas

42. Single Field Inflation models allowed and ruled out by the three years WMAP data

43. Phase transitions in the early and the present Universe

44. Statistical Mechanics of the Self-Gravitating Gas: Thermodynamic Limit, Unstabilities and Phase Diagrams

45. Clarifying Slow Roll Inflation and the Quantum Corrections to the Observable Power Spectra

47. QCD Pomerons at Non-Zero Temperature

48. Neutrino Oscillations in the Early Universe: A Real Time Formulation

49. Clarifying Inflation Models: Slow-roll as an expansion in 1/N_{efolds}

50. Quantum corrections to the inflaton potential and the power spectra from superhorizon modes and trace anomalies

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