All Stories

  1. Square Kilometre Array Science Data Challenge 3a: foreground removal for an EoR experiment
  2. Unexplained correlation between the Cosmic Microwave Background temperature and the local matter density distribution
  3. The benefits of Shuai Shou Gong (SSG) demonstrated in a Randomised Control Trial (RCT) study of older adults in two communities in Thailand
  4. Measurement of changes in uterine and fibroid volume during treatment of heavy menstrual bleeding (HMB)
  5. Multi‐image flock size estimation with CountEm: A case study with half a million Common Eiders and Greater Snow Geese
  6. Eastern Canada Flocks: images and manually annotated bird positions
  7. Transformation of a Grid of Quadrats to Cope With Perspective Artifacts
  8. The CountEm software: simple, efficient and unbiased population size estimation
  9. VARIANCE PREDICTION FOR POPULATION SIZE ESTIMATION
  10. Evaluating the pharmacological response in fluorescence microscopy images: The Δm algorithm
  11. ON THE PRECISION OF THE ISOTROPIC CAVALIERI DESIGN
  12. Simplified procedure for efficient and unbiased population size estimation
  13. Unbiased Population Size Estimation on Still Gigapixel Images
  14. ON THE PRECISION OF THE NUCLEATOR
  15. Planck2015 results
  16. Planck2015 results
  17. Planck2015 results
  18. ON THE PRECISION OF CURVE LENGTH ESTIMATION IN THE PLANE
  19. Efficient and Unbiased Estimation of Population Size
  20. Quantitative Measurements in the Human Hippocampus and Related Areas: Correspondence between Ex-Vivo MRI and Histological Preparations
  21. Planck2013 results. I. Overview of products and scientific results
  22. Planck2013 results. XXIII. Isotropy and statistics of the CMB
  23. Planck2013 results. II. Low Frequency Instrument data processing
  24. Planck2013 results. III. LFI systematic uncertainties
  25. Planck2013 results. XII. Diffuse component separation
  26. Using CMB polarization to constrain the anomalous nature of the Cold Spot with an incomplete-sky coverage
  27. Planckearly results. III. First assessment of the Low Frequency Instrument in-flight performance
  28. Planckearly results. V. The Low Frequency Instrument data processing
  29. Anomalous variance in the WMAP data and Galactic foreground residuals
  30. Cosmic microwave background polarization as a probe of the anomalous nature of the cold spot
  31. On the linear complexity of the Naor–Reingold sequence with elliptic curves
  32. An anomalousWilkinson Microwave Anisotropy Probesignal in the ecliptic plane
  33. The WMAP Cold Spot
  34. The CMB cold spot: texture, cluster or void?
  35. Bianchi VIIhmodels and the cold spot texture
  36. A Cosmic Microwave Background Feature Consistent with a Cosmic Texture
  37. The Non‐Gaussian Cold Spot in the 3 YearWilkinson Microwave Anisotropy ProbeData
  38. The non-Gaussian cold spot in WMAP
  39. The non-Gaussian cold spot in Wilkinson Microwave Anisotropy Probe: significance, morphology and foreground contribution
  40. Detection of a non-Gaussian spot in WMAP