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K. M. Gorski

Identifiers

  • name variant K. M. Gorski 0.60 · backfill

Papers (64)

  1. Planck 2013 results. XXXI. Consistency of the Planck data astro-ph.CO · 2015 · author #57
  2. Planck 2015 results. XXV. Diffuse low-frequency Galactic foregrounds astro-ph.GA · 2015 · author #83
  3. Planck 2015 results. XX. Constraints on inflation astro-ph.CO · 2015 · author #83
  4. Planck 2015 results. XIII. Cosmological parameters astro-ph.CO · 2015 · author #89
  5. Planck 2015 results. VII. HFI TOI and beam processing astro-ph.IM · 2015 · author #80
  6. Monopole and dipole estimation for multi-frequency sky maps by linear regression astro-ph.CO · 2014 · author #7
  7. Planck intermediate results. XXVIII. Interstellar gas and dust in the Chamaeleon clouds as seen by Fermi LAT and Planck astro-ph.HE · 2014 · author #75
  8. Planck intermediate results. XXIX. All-sky dust modelling with Planck, IRAS, and WISE observations astro-ph.GA · 2014 · author #74
  9. Directional dependence of LCDM cosmological parameters astro-ph.CO · 2013 · author #6
  10. Planck 2013 results. XXII. Constraints on inflation astro-ph.CO · 2013 · author #78
  11. Planck 2013 results. XXI. All-sky Compton parameter power spectrum and high-order statistics astro-ph.CO · 2013 · author #80
  12. Planck 2013 results. XV. CMB power spectra and likelihood astro-ph.CO · 2013 · author #84
  13. Planck 2013 results. XIII. Galactic CO emission astro-ph.GA · 2013 · author #80
  14. Constraints on the topology of the Universe derived from the 7-year WMAP CMB data and prospects of constraining the topology using CMB polarisation maps astro-ph.CO · 2013 · author #3
  15. Planck Intermediate Results. V. Pressure profiles of galaxy clusters from the Sunyaev-Zeldovich effect astro-ph.CO · 2012 · author #82
  16. Probing non-Gaussianities in the CMB on an incomplete sky using surrogates astro-ph.CO · 2012 · author #5
  17. Constraining the topology of the Universe using the polarised CMB maps astro-ph.CO · 2011 · author #3
  18. Search for non-Gaussianities in the WMAP data with the Scaling Index Method astro-ph.CO · 2011 · author #5
  19. Planck Early Results XXIV: Dust in the diffuse interstellar medium and the Galactic halo astro-ph.GA · 2011 · author #72
  20. Planck early results. XXI. Properties of the interstellar medium in the Galactic plane astro-ph.GA · 2011 · author #69
  21. Planck Early Results. II. The thermal performance of Planck astro-ph.IM · 2011 · author #86
  22. Scale-dependent non-Gaussianities in the WMAP data as identified by using surrogates and scaling indices astro-ph.CO · 2010 · author #6
  23. Performance of XFaster likelihood in real CMB experiments astro-ph.CO · 2010 · author #5
  24. Probing non-Gaussianities on Large Scales in WMAP5 and WMAP7 Data using Surrogates astro-ph.CO · 2010 · author #5
  25. Application of XFaster power spectrum and likelihood estimator to Planck astro-ph.CO · 2009 · author #4
  26. Increasing evidence for hemispherical power asymmetry in the five-year WMAP data astro-ph.CO · 2009 · author #4
  27. Power Asymmetry in Cosmic Microwave Background Fluctuations from Full Sky to Sub-degree Scales: Is the Universe Isotropic? astro-ph · 2008 · author #3
  28. The scalar perturbation spectral index n_s: WMAP sensitivity to unresolved point sources astro-ph · 2007 · author #5
  29. Applications of Fast Convolution on the Sphere astro-ph · 2007 · author #3
  30. The joint large-scale foreground-CMB posteriors of the 3-year WMAP data astro-ph · 2007 · author #5
  31. Joint Bayesian component separation and CMB power spectrum estimation astro-ph · 2007 · author #5
  32. Bayesian analysis of the low-resolution polarized 3-year WMAP sky maps astro-ph · 2007 · author #4
  33. Hemispherical power asymmetry in the three-year Wilkinson Microwave Anisotropy Probe sky maps astro-ph · 2007 · author #3
  34. Estimation of Polarized Power Spectra by Gibbs sampling astro-ph · 2006 · author #4
  35. Making sky maps from Planck data astro-ph · 2006 · author #8
  36. A re-analysis of the three-year WMAP temperature power spectrum and likelihood astro-ph · 2006 · author #7
  37. Bianchi Type VII_h Models and the WMAP 3-year Data astro-ph · 2006 · author #4
  38. Bayesian foreground analysis with CMB data astro-ph · 2006 · author #6
  39. Fast and Efficient Template Fitting of Deterministic Anisotropic Cosmological Models Applied to WMAP Data astro-ph · 2006 · author #4
  40. Foreground Subtraction of Cosmic Microwave Background Maps using WI-FIT (Wavelet based hIgh resolution Fitting of Internal Templates) astro-ph · 2006 · author #4
  41. On the Viability of Bianchi Type VIIh Models with Dark Energy astro-ph · 2005 · author #4
  42. CMB component separation by parameter estimation astro-ph · 2005 · author #6
  43. Astro-ph communication: Simulations of the WMAP Internal Linear Combination sky map astro-ph · 2005 · author #3
  44. Multipole vector anomalies in the first-year WMAP data: a cut-sky analysis astro-ph · 2005 · author #4
  45. Evidence of vorticity and shear at large angular scales in the WMAP data: a violation of cosmological isotropy? astro-ph · 2005 · author #4
  46. Cosmological Parameter Constraints as Derived from the Wilkinson Microwave Anisotropy Probe Data via Gibbs Sampling and the Blackwell-Rao Estimator astro-ph · 2004 · author #4
  47. HEALPix -- a Framework for High Resolution Discretization, and Fast Analysis of Data Distributed on the Sphere astro-ph · 2004 · author #1
  48. The N-point correlation functions of the first-year Wilkinson Microwave Anisotropy Probe sky maps astro-ph · 2004 · author #3
  49. Power spectrum estimation from high-resolution maps by Gibbs sampling astro-ph · 2004 · author #6
  50. Bayesian Power Spectrum Analysis of the First-Year WMAP data astro-ph · 2004 · author #6
  51. Cosmological parameters and the WMAP data revisited astro-ph · 2004 · author #4
  52. Low-order multipole maps of CMB anisotropy derived from WMAP astro-ph · 2004 · author #2
  53. Testing the cosmological principle of isotropy: local power spectrum estimates of the WMAP data astro-ph · 2004 · author #3
  54. On Foreground Removal from the Wilkinson Microwave Anisotropy Probe Data by an Internal Linear Combination Method: Limitations and Implications astro-ph · 2004 · author #3
  55. Testing for Non-Gaussianity in the Wilkinson Microwave Anisotropy Probe Data: Minkowski Functionals and the Length of the Skeleton astro-ph · 2004 · author #5
  56. Estimating N-Point Correlation Functions from Pixelized Sky Maps astro-ph · 2003 · author #4
  57. Asymmetries in the CMB anisotropy field astro-ph · 2003 · author #4
  58. The N-point correlation functions of the COBE-DMR maps revisited astro-ph · 2002 · author #3
  59. The Trispectrum of the 4 Year COBE-DMR data astro-ph · 2001 · author #5
  60. Spherical Mexican Hat wavelet: an application to detect non-Gaussianity in the COBE-DMR maps astro-ph · 2001 · author #7
  61. A Bayesian estimate of the skewness of the Cosmic Microwave Background astro-ph · 1999 · author #4
  62. Constraining the Power Spectrum using Clusters astro-ph · 1996 · author #4
  63. 4-Year COBE DMR Cosmic Microwave Background Observations: Maps and Basic Results astro-ph · 1996 · author #3
  64. Three-Point Correlations in the COBE-DMR Two-Year Anisotropy Maps astro-ph · 1995 · author #4

Mentions

  • 1508.03375 #57 · backfill · confidence 0.70 K. M. Gorski
  • 1506.06660 #83 · backfill · confidence 0.70 K. M. Gorski
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  • 1502.01589 #89 · backfill · confidence 0.70 K. M. Gorski
  • 1502.01586 #80 · backfill · confidence 0.70 K. M. Gorski
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Frequent Coauthors