K. Vanderlinde mainly focuses on Astrophysics, South Pole Telescope, Cosmic microwave background, Astronomy and Redshift. The Galaxy and Cosmology research K. Vanderlinde does as part of his general Astrophysics study is frequently linked to other disciplines of science, such as Neutrino oscillation, therefore creating a link between diverse domains of science. His study with South Pole Telescope involves better knowledge in Galaxy cluster.
His research in Cosmic microwave background intersects with topics in Dark energy, Hubble's law and Reionization. In the subject of general Astronomy, his work in Sunyaev–Zel'dovich effect is often linked to Research council, Excellence and Library science, thereby combining diverse domains of study. His Redshift study deals with Dark matter intersecting with Extragalactic astronomy.
His primary scientific interests are in Astrophysics, South Pole Telescope, Cosmic microwave background, Astronomy and Redshift. His Astrophysics study incorporates themes from Cosmic infrared background and Cluster. His South Pole Telescope study combines topics from a wide range of disciplines, such as Sunyaev–Zel'dovich effect, Sky, Bolometer, Dark energy and Gravitational lens.
His work on Cosmic background radiation as part of general Cosmic microwave background study is frequently connected to Multipole expansion, therefore bridging the gap between diverse disciplines of science and establishing a new relationship between them. K. Vanderlinde combines subjects such as Luminosity, Dark matter and Galaxy formation and evolution with his study of Redshift. His Galaxy cluster research incorporates elements of Cosmology, Amplitude, ROSAT and Velocity dispersion.
His primary areas of investigation include Astrophysics, South Pole Telescope, Cosmic microwave background, Planck and Galaxy. His work on Dark energy, Redshift and Sky as part of his general Astrophysics study is frequently connected to Planck temperature, thereby bridging the divide between different branches of science. The various areas that he examines in his Dark energy study include Weak gravitational lensing and Galaxy cluster.
K. Vanderlinde studied South Pole Telescope and Detector that intersect with Multiplexing. His study in Cosmic microwave background is interdisciplinary in nature, drawing from both Amplitude, Polarization, Gravitational lens and Cluster. His biological study spans a wide range of topics, including Lambda and Baryon.
The scientist’s investigation covers issues in Astrophysics, Cosmic microwave background, South Pole Telescope, Galaxy and Canadian Hydrogen Intensity Mapping Experiment. His research related to Redshift and Dark energy might be considered part of Astrophysics. His Dark energy research integrates issues from Weak gravitational lensing and Galaxy cluster.
In general Cosmic microwave background study, his work on Cosmic background radiation often relates to the realm of Multipole expansion, thereby connecting several areas of interest. His South Pole Telescope study is concerned with the larger field of Astronomy. K. Vanderlinde interconnects Spiral galaxy, Sky and Dwarf galaxy in the investigation of issues within Canadian Hydrogen Intensity Mapping Experiment.
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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)
SPT-3G: A Next-Generation Cosmic Microwave Background Polarization Experiment on the South Pole Telescope
B. A. Benson;P. A. R. Ade;Z. Ahmed;S. W. Allen.
arXiv: Instrumentation and Methods for Astrophysics (2014)
Constraints on Cosmology from the Cosmic Microwave Background Power Spectrum of the 2500 ${ m deg}^2$ SPT-SZ Survey
Z. Hou;C. L. Reichardt;K. T. Story;B. Follin.
arXiv: Cosmology and Nongalactic Astrophysics (2012)
Detection of B-Mode Polarization in the Cosmic Microwave Background with Data from the South Pole Telescope
D. Hanson;S. Hoover;A. Crites;P. A.R. Ade.
Physical Review Letters (2013)
GALAXY CLUSTERS SELECTED WITH THE SUNYAEV-ZEL'DOVICH EFFECT FROM 2008 SOUTH POLE TELESCOPE OBSERVATIONS
K. Vanderlinde;T. M. Crawford;T. De Haan;J. P. Dudley.
The Astrophysical Journal (2010)
Cosmological Constraints from Sunyaev-Zel'dovich-Selected Clusters with X-ray Observations in the First 178 Square Degrees of the South Pole Telescope Survey
B. A. Benson;T. de Haan;J. P. Dudley;C. L. Reichardt.
arXiv: Cosmology and Nongalactic Astrophysics (2011)
ALMA redshifts of millimeter-selected galaxies from the SPT survey: The redshift distribution of dusty star-forming galaxies
A. Weiss;C. De Breuck;D. P. Marrone;J. D. Vieira.
arXiv: Cosmology and Nongalactic Astrophysics (2013)
An SZ-selected sample of the most massive galaxy clusters in the 2500-square-degree South Pole Telescope survey
R. Williamson;B. A. Benson;F. W. High;K. Vanderlinde.
arXiv: Cosmology and Nongalactic Astrophysics (2011)
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