2008 - Fellow of Alfred P. Sloan Foundation
N. W. Halverson spends much of his time researching Astrophysics, Cosmic microwave background, South Pole Telescope, Astronomy and Redshift. His Astrophysics research focuses on subjects like Cosmic Background Imager, which are linked to Very Small Array. N. W. Halverson has included themes like Neutrino and Spectral density in his Cosmic microwave background study.
His study on South Pole Telescope also encompasses disciplines like
His primary areas of study are Cosmic microwave background, Astrophysics, South Pole Telescope, Astronomy and Optics. N. W. Halverson does research in Cosmic microwave background, focusing on Cosmic background radiation specifically. His Astrophysics research includes elements of Spectral density and Cluster.
The Spectral density study combines topics in areas such as Amplitude, Spectral line, Cold dark matter and Anisotropy. His study in South Pole Telescope is interdisciplinary in nature, drawing from both Sky, Cosmic infrared background, Planck, Neutrino and Multiplexing. His Galaxy cluster research is multidisciplinary, relying on both Cosmology, Dark energy and Weak gravitational lensing.
N. W. Halverson mainly investigates Cosmic microwave background, Astrophysics, South Pole Telescope, Optics and Polarization. His work deals with themes such as Gravitational wave, Astronomy, Sky and Telescope, which intersect with Cosmic microwave background. His study in the field of Satellite, Lagrangian point and Inflation also crosses realms of Project plan.
His research links Spectral density with Astrophysics. N. W. Halverson works mostly in the field of South Pole Telescope, limiting it down to concerns involving Radio spectrum and, occasionally, Antenna array. His Polarization research incorporates themes from COSMIC cancer database, Angular resolution and Neutrino.
The scientist’s investigation covers issues in Cosmic microwave background, Astrophysics, South Pole Telescope, Polarization and Planck. His Cosmic microwave background study incorporates themes from Astronomy, Spectral line, Telescope, Gravitational wave and Detector. His Astrophysics study frequently draws connections to adjacent fields such as Cosmic background radiation.
His research in South Pole Telescope tackles topics such as Gravitational lens which are related to areas like Polarimetry and Multiplexing. N. W. Halverson focuses mostly in the field of Polarization, narrowing it down to topics relating to Lagrangian point and, in certain cases, Passive cooling, Noise, Satellite and Superconducting detectors. His Planck research includes themes of Spectral density and CMB cold spot.
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.
First M87 Event Horizon Telescope Results. I. The Shadow of the Supermassive Black Hole
Kazunori Akiyama;Antxon Alberdi;Walter Alef.
The Astrophysical Journal (2019)
Degree Angular Scale Interferometer First Results: A Measurement of the Cosmic Microwave Background Angular Power Spectrum
N. W. Halverson;E. M. Leitch;C. Pryke;J. Kovac.
The Astrophysical Journal (2002)
Detection of polarization in the cosmic microwave background using DASI
J. M. Kovac;E. M. Leitch;Clement L Pryke;J. E. Carlstrom.
Nature (2002)
DASI First Results: A Measurement of the Cosmic Microwave Background Angular Power Spectrum
N. W. Halverson;E. M. Leitch;C. Pryke;J. Kovac.
arXiv: Astrophysics (2001)
Cosmological Parameter Extraction from the First Season of Observations with the Degree Angular Scale Interferometer
C. Pryke;N. W. Halverson;E. M. Leitch;J. Kovac.
The Astrophysical Journal (2002)
The 10 Meter South Pole Telescope
J. E. Carlstrom;Peter A. R. Ade;K. A. Aird;B. A. Benson.
Publications of the Astronomical Society of the Pacific (2011)
Galaxy clusters discovered via the Sunyaev-Zel'dovich effect in the 2500-square-degree SPT-SZ survey
L. E. Bleem;L. E. Bleem;Brian A Stalder;T. de Haan;K. A. Aird.
Astrophysical Journal Supplement Series (2015)
A MEASUREMENT OF THE DAMPING TAIL OF THE COSMIC MICROWAVE BACKGROUND POWER SPECTRUM WITH THE SOUTH POLE TELESCOPE
R. Keisler;C. L. Reichardt;K. A. Aird;B. A. Benson.
The Astrophysical Journal (2011)
The Anisotropy of the Microwave Background to l = 3500: Mosaic Observations with the Cosmic Background Imager
B. S. Mason;B. S. Mason;T. J. Pearson;A. C. S. Readhead;M. C. Shepherd.
The Astrophysical Journal (2003)
First M87 Event Horizon Telescope Results. II. Array and Instrumentation
Kazunori Akiyama;Antxon Alberdi;Walter Alef.
The Astrophysical Journal (2019)
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