D-Index & Metrics Best Publications
E. J. Sanchez

E. J. Sanchez

California Institute of Technology
United States

Overview

What is he best known for?

The fields of study he is best known for:

  • Quantum mechanics
  • Astronomy
  • Astrophysics

His scientific interests lie mostly in Astrophysics, LIGO, Astronomy, Gravitational wave and Galaxy. His research in Redshift, Binary black hole, Dark energy, Neutron star and Black hole are components of Astrophysics. His research in Binary black hole intersects with topics in General relativity and Gravitational wave background.

His study in LIGO is interdisciplinary in nature, drawing from both Stars, Mass distribution and Mass ratio. His biological study spans a wide range of topics, including Gamma-ray burst, Observatory and Detector. His work on Milky Way as part of general Galaxy study is frequently linked to Spins, bridging the gap between disciplines.

His most cited work include:

  • Observation of Gravitational Waves from a Binary Black Hole Merger (7103 citations)
  • GW170817: observation of gravitational waves from a binary neutron star inspiral (4913 citations)
  • GW151226: observation of gravitational waves from a 22-solar-mass binary black hole coalescence (2671 citations)

What are the main themes of his work throughout his whole career to date?

E. J. Sanchez focuses on Astrophysics, Galaxy, Dark energy, Redshift and Astronomy. LIGO, Gravitational wave, Supernova, Neutron star and Sky are the subjects of his Astrophysics studies. His LIGO research includes themes of Gamma-ray burst and Binary black hole, Black hole.

E. J. Sanchez focuses mostly in the field of Gravitational wave, narrowing it down to topics relating to Detector and, in certain cases, Nuclear physics and Particle physics. His work carried out in the field of Galaxy brings together such families of science as Cluster analysis and Photometry. E. J. Sanchez interconnects Luminosity and Quasar in the investigation of issues within Redshift.

He most often published in these fields:

  • Astrophysics (55.47%)
  • Galaxy (29.76%)
  • Dark energy (29.65%)

What were the highlights of his more recent work (between 2019-2021)?

  • Astrophysics (55.47%)
  • Dark energy (29.65%)
  • Galaxy (29.76%)

In recent papers he was focusing on the following fields of study:

E. J. Sanchez spends much of his time researching Astrophysics, Dark energy, Galaxy, Redshift and LIGO. His research investigates the connection between Dark energy and topics such as Weak gravitational lensing that intersect with problems in Dark matter. His Galaxy research focuses on Sigma and how it connects with COSMIC cancer database.

His Redshift study integrates concerns from other disciplines, such as Spectral density, Galaxy cluster and Flux. His LIGO research includes themes of Gamma-ray burst and Black hole. His Neutron star research is multidisciplinary, incorporating perspectives in Mass distribution and Kilonova.

Between 2019 and 2021, his most popular works were:

  • GW190425: Observation of a Compact Binary Coalescence with Total Mass ∼ 3.4 M ⊙ (463 citations)
  • GW190425: Observation of a Compact Binary Coalescence with Total Mass $\sim 3.4 M_{\odot}$ (389 citations)
  • GW190814: Gravitational Waves from the Coalescence of a 23 Solar Mass Black Hole with a 2.6 Solar Mass Compact Object (356 citations)

In his most recent research, the most cited papers focused on:

  • Quantum mechanics
  • Astronomy
  • Statistics

E. J. Sanchez mainly focuses on Astrophysics, LIGO, Gravitational wave, Dark energy and Redshift. His work is connected to Galaxy, Supernova, Galaxy cluster, Mass distribution and Sky, as a part of Astrophysics. His LIGO research incorporates themes from Computational physics, Stars, Gamma-ray burst, Black hole and Neutron star.

In his work, Compact star, Multipole expansion and Theory of relativity is strongly intertwined with Mass ratio, which is a subfield of Gravitational wave. His Dark energy research incorporates elements of Stellar mass, Weak gravitational lensing and Telescope. The Redshift study combines topics in areas such as Amplitude, Quasar and Omega.

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.

Best Publications

Observation of Gravitational Waves from a Binary Black Hole Merger

B. Abbott;R. Abbott;T. D. Abbott;M. R. Abernathy.
Physical Review Letters (2016)

11699 Citations

GW170817: observation of gravitational waves from a binary neutron star inspiral

B. P. Abbott;R. Abbott;T. D. Abbott;F. Acernese.
Physical Review Letters (2017)

6436 Citations

GW151226: observation of gravitational waves from a 22-solar-mass binary black hole coalescence

B. P. Abbott;R. Abbott.
Physical Review Letters (2016)

3544 Citations

GW170104: Observation of a 50-Solar-Mass Binary Black Hole Coalescence at Redshift 0.2

B. P. Abbott;R. Abbott;T. D. Abbott;F. Acernese.
Physical Review Letters (2017)

2511 Citations

Gravitational Waves and Gamma-Rays from a Binary Neutron Star Merger: GW170817 and GRB 170817A

B. P. Abbott;R. Abbott;T. D. Abbott;F. Acernese.
The Astrophysical Journal (2017)

2285 Citations

GW170814: A three-detector observation of gravitational waves from a binary black hole coalescence

B. P. Abbott;R. Abbott;T. D. Abbott;F. Acernese.
Physical Review Letters (2017)

1991 Citations

GWTC-1: A Gravitational-Wave Transient Catalog of Compact Binary Mergers Observed by LIGO and Virgo during the First and Second Observing Runs

B. P. Abbott;R. Abbott.
Physical Review X (2019)

1821 Citations

The DELPHI detector at LEP.

P.A. Aarnio;W. Kucewicz;J. Wikne;J.A. Lidbury.
Nuclear Instruments & Methods in Physics Research Section A-accelerators Spectrometers Detectors and Associated Equipment (1991)

1791 Citations

Prospects for Observing and Localizing Gravitational-Wave Transients with Advanced LIGO, Advanced Virgo and KAGRA

B. P. Abbott;R. Abbott;T. D. Abbott;M. R. Abernathy.
Living Reviews in Relativity (2018)

1586 Citations

Binary Black Hole Mergers in the First Advanced LIGO Observing Run

B. P. Abbott;R. Abbott.
Physical Review X (2016)

1521 Citations

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