2023 - Research.com Physics in Norway Leader Award
2022 - Research.com Physics in Norway Leader Award
His primary scientific interests are in Astrophysics, Planck, Cosmic microwave background, Planck temperature and Sky. His Astrophysics research is multidisciplinary, incorporating perspectives in Cosmic background radiation, Spectral density and CMB cold spot. His Planck research is multidisciplinary, relying on both Polarization, Dark energy and Galaxy, Redshift.
H. K. Eriksen has included themes like Hubble's law, Amplitude, Reionization, Bispectrum and Gravitational lens in his Cosmic microwave background study. His study in Sky is interdisciplinary in nature, drawing from both Radio spectrum, Magnetic field, Spinning dust and Molecular cloud. H. K. Eriksen works mostly in the field of Cosmology, limiting it down to topics relating to Neutrino and, in certain cases, Residual.
H. K. Eriksen focuses on Astrophysics, Planck, Cosmic microwave background, Sky and CMB cold spot. His work deals with themes such as Polarization, Astronomy, Spectral density and Spectral index, which intersect with Astrophysics. The concepts of his Polarization study are interwoven with issues in Telescope and Magnetic field.
With his scientific publications, his incorporates both Planck and Planck temperature. His biological study spans a wide range of topics, including Cosmology, Gravitational wave, Gibbs sampling and Amplitude. His CMB cold spot study combines topics from a wide range of disciplines, such as Isotropy, Dipole, Multipole expansion and Asymmetry.
His main research concerns Astrophysics, Cosmic microwave background, Planck, Polarization and Sky. His work carried out in the field of Astrophysics brings together such families of science as Amplitude and Spectral density. H. K. Eriksen studies Cosmic microwave background, namely Cosmic background radiation.
H. K. Eriksen interconnects Dipole, Cosmology, Dark energy, Bispectrum and Particle physics in the investigation of issues within Planck. His study focuses on the intersection of Polarization and fields such as Spectral index with connections in the field of Synchrotron and Faraday effect. His study in Sky is interdisciplinary in nature, drawing from both CMB cold spot, Molecular cloud, Inverse, Spider and Dust emission.
Cosmic microwave background, Astrophysics, Planck, Polarization and Sky are his primary areas of study. H. K. Eriksen combines subjects such as Astronomy, Gravitational wave, Radio spectrum, Telescope and Reionization with his study of Cosmic microwave background. His research on Astrophysics frequently links to adjacent areas such as Cosmic background radiation.
His biological study spans a wide range of topics, including Redshift, Omega, Spectral density, Spectral index and Particle physics. His research investigates the connection between Polarization and topics such as Lagrangian point that intersect with issues in Satellite and Superconducting detectors. The various areas that H. K. Eriksen examines in his Sky study include Inverse, Magnetic field and Molecular cloud.
This overview was generated by a machine learning system which analysed the scientist’s body of work. If you have any feedback, you can contact us here.
Planck 2015 results. XIII. Cosmological parameters
P. A. R. Ade;N. Aghanim;M. Arnaud.
arXiv: Cosmology and Nongalactic Astrophysics (2015)
Planck 2015 results - XIII. Cosmological parameters
Peter A. R. Ade;N. Aghanim;M. Arnaud;M. Ashdown.
Astronomy and Astrophysics (2016)
Planck 2013 results. XVI. Cosmological parameters
P. A. R. Ade;N. Aghanim;C. Armitage-Caplan.
Astronomy and Astrophysics (2014)
Planck 2013 results. XVI. Cosmological parameters
P. A. R. Ade;N. Aghanim;C. Armitage-Caplan.
arXiv: Cosmology and Nongalactic Astrophysics (2013)
Planck 2015 results. XX. Constraints on inflation
P. A. R. Ade;N. Aghanim;M. Arnaud.
arXiv: Cosmology and Nongalactic Astrophysics (2015)
Planck 2018 results. VI. Cosmological parameters
N. Aghanim;Y. Akrami;M. Ashdown.
arXiv: Cosmology and Nongalactic Astrophysics (2018)
Planck 2018 results. VI. Cosmological parameters
N. Aghanim;Y. Akrami;Y. Akrami;Y. Akrami;M. Ashdown.
Astronomy and Astrophysics (2020)
Planck 2013 results. XXII. Constraints on inflation
P.A.R. Ade;N. Aghanim;M. Arnaud;F. Arroja;F. Arroja.
Astronomy and Astrophysics (2014)
Planck 2013 results. I. Overview of products and scientific results
P. A. R. Ade;N. Aghanim;M. I. R. Alves.
Astronomy and Astrophysics (2014)
Planck 2015. XX. Constraints on inflation
P.A.R. Ade;F.X. Desert;J. Knoche;M. Giard.
Astronomy and Astrophysics (2015)
If you think any of the details on this page are incorrect, let us know.
We appreciate your kind effort to assist us to improve this page, it would be helpful providing us with as much detail as possible in the text box below:
National Institute for Astrophysics
Jet Propulsion Lab
Lawrence Berkeley National Laboratory
University of La Laguna
California Institute of Technology
National Institute for Astrophysics
Sapienza University of Rome
University of Padua
University of Toronto
Institut d'Astrophysique de Paris
University of Natural Resources and Life Sciences
University of Siena
FX Palo Alto Laboratory
University of Michigan–Ann Arbor
Fuji Xerox (Japan)
University of California, Los Angeles
King's College London
Nanjing University of Aeronautics and Astronautics
Bill & Melinda Gates Foundation
University at Buffalo, State University of New York
University of Pittsburgh
University of California, Davis
University of Pittsburgh
University of California, San Diego
National Institute for Astrophysics