Oak Ridge National Laboratory
United States
His primary areas of investigation include Astrophysics, Galaxy, Astronomy, Dark energy and Redshift. While the research belongs to areas of Astrophysics, E. Suchyta spends his time largely on the problem of Cosmic microwave background, intersecting his research to questions surrounding Neutrino. As a part of the same scientific family, E. Suchyta mostly works in the field of Galaxy, focusing on Data set and, on occasion, Limiting magnitude and Astronomical Objects.
His research in the fields of Redshift survey, Sky and Photometry overlaps with other disciplines such as European research. His Dark energy study combines topics in areas such as South Pole Telescope, COSMIC cancer database, Weak gravitational lensing and Planck. His work deals with themes such as Luminosity, Quasar, LIGO and Sigma, which intersect with Redshift.
His primary scientific interests are in Astrophysics, Dark energy, Galaxy, Redshift and Astronomy. Supernova, Milky Way, Light curve, Galaxy cluster and Quasar are the core of his Astrophysics study. His Milky Way research is multidisciplinary, incorporating elements of Globular cluster, Dwarf galaxy and Large Magellanic Cloud.
His Dark energy study combines topics from a wide range of disciplines, such as COSMIC cancer database, Weak gravitational lensing, Cosmic microwave background and Planck. His Galaxy research incorporates elements of Cluster analysis, Dark matter and Photometry. His studies deal with areas such as Luminosity, Stellar mass, Sky and Telescope as well as Redshift.
E. Suchyta focuses on Astrophysics, Dark energy, Galaxy, Redshift and Supernova. His Light curve, Luminosity, Quasar, Dark matter and Dwarf galaxy study are his primary interests in Astrophysics. His Dark energy research is multidisciplinary, relying on both Weak gravitational lensing, Cosmic microwave background and Planck.
He interconnects Sky, Sigma and Photometry in the investigation of issues within Galaxy. The study incorporates disciplines such as Galaxy cluster and Diffuse reflection in addition to Redshift. His research in Supernova focuses on subjects like Neutron star, which are connected to LIGO.
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.
Dark Energy Survey year 1 results: Cosmological constraints from galaxy clustering and weak lensing
T. M. C. Abbott;F. B. Abdalla;A. Alarcon;J. Aleksić.
Physical Review D (2018)
The Dark Energy Camera
B. Flaugher;H. T. Diehl;K. Honscheid;T. M. C. Abbott.
arXiv: Instrumentation and Methods for Astrophysics (2015)
THE DARK ENERGY CAMERA
B. Flaugher;H. T. Diehl;K. Honscheid;T. M. C. Abbott.
The Astronomical Journal (2015)
Eight New Milky Way Companions Discovered in First-Year Dark Energy Survey Data
K. Bechtol;A. Drlica-Wagner;E. Balbinot.
arXiv: Astrophysics of Galaxies (2015)
The Electromagnetic Counterpart of the Binary Neutron Star Merger LIGO/Virgo GW170817. II. UV, Optical, and Near-infrared Light Curves and Comparison to Kilonova Models
P. S. Cowperthwaite;E. Berger;V. A. Villar;B. D. Metzger.
The Astrophysical Journal (2017)
A gravitational-wave standard siren measurement of the Hubble constant
B. P. Abbott;R. Abbott;T. D. Abbott;F. Acernese;F. Acernese.
Nature (2017)
The Dark Energy Survey: more than dark energy - an overview
T. Abbott;F. B. Abdalla;J. Aleksić.
Monthly Notices of the Royal Astronomical Society (2016)
Eight Ultra-faint Galaxy Candidates Discovered in Year Two of the Dark Energy Survey
A. Drlica-Wagner;K. Bechtol;E. S. Rykoff.
arXiv: Astrophysics of Galaxies (2015)
Eight new Milky Way companions discovered in first-year Dark Energy Survey data
K. Bechtol;A. Drlica-Wagner;E. Balbinot;A. Pieres.
The Astrophysical Journal (2015)
The Electromagnetic Counterpart of the Binary Neutron Star Merger LIGO/Virgo GW170817. I. Dark Energy Camera Discovery of the Optical Counterpart
M. Soares-Santos;D. E. Holz;J. Annis;R. Chornock.
arXiv: High Energy Astrophysical Phenomena (2017)
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