What is he best known for?
The fields of study he is best known for:
- Astronomy
- Astrophysics
- Electron
The scientist’s investigation covers issues in Astrophysics, Astronomy, Neutron star, Pulsar and Magnetar.
His work deals with themes such as Spectral line and Photon, which intersect with Astrophysics.
His research in Neutron star intersects with topics in Accretion, Millisecond, Oscillation, Supermassive black hole and Transient.
His Pulsar research is multidisciplinary, relying on both Stars and Black-body radiation.
His Magnetar course of study focuses on ROSAT and Static timing analysis, Spectral component and Green Bank Telescope.
Sandro Mereghetti usually deals with Observatory and limits it to topics linked to Cherenkov Telescope Array and Astroparticle physics, Telescope and LIGO.
His most cited work include:
- Gravitational Waves and Gamma-Rays from a Binary Neutron Star Merger: GW170817 and GRB 170817A (1739 citations)
- The strongest cosmic magnets: soft gamma-ray repeaters and anomalous X-ray pulsars (625 citations)
- Introducing the CTA concept (533 citations)
What are the main themes of his work throughout his whole career to date?
His primary areas of investigation include Astrophysics, Astronomy, Gamma ray, Neutron star and Pulsar.
His work on Gamma-ray burst and Blazar is typically connected to Flux and Agile software development as part of general Astrophysics study, connecting several disciplines of science.
His Luminosity, X-ray binary, Telescope, Satellite and Sky study are his primary interests in Astronomy.
His biological study spans a wide range of topics, including Flare and Transient.
His Neutron star study incorporates themes from Accretion, Stars and Supernova remnant.
His studies deal with areas such as Radius and Black-body radiation as well as Pulsar.
He most often published in these fields:
- Astrophysics (86.80%)
- Astronomy (32.62%)
- Gamma ray (24.75%)
What were the highlights of his more recent work (between 2016-2021)?
- Astrophysics (86.80%)
- Gamma ray (24.75%)
- LIGO (4.51%)
In recent papers he was focusing on the following fields of study:
His primary scientific interests are in Astrophysics, Gamma ray, LIGO, Astronomy and Transient.
His work on Neutron star, Gamma-ray burst, Pulsar and Magnetar as part of general Astrophysics study is frequently linked to Ibis, bridging the gap between disciplines.
His Neutron star study integrates concerns from other disciplines, such as Accretion, Luminosity and White dwarf.
His research investigates the connection between Pulsar and topics such as Black-body radiation that intersect with problems in Radius.
Many of his research projects under Gamma ray are closely connected to Agile software development with Agile software development, tying the diverse disciplines of science together.
His research is interdisciplinary, bridging the disciplines of Cherenkov Telescope Array and Astronomy.
Between 2016 and 2021, his most popular works were:
- Gravitational Waves and Gamma-Rays from a Binary Neutron Star Merger: GW170817 and GRB 170817A (1739 citations)
- The e-ASTROGAM mission: Exploring the extreme Universe with gamma rays in the MeV – GeV range (122 citations)
- Science with e-ASTROGAM (A space mission for MeV-GeV gamma-ray astrophysics) (117 citations)
In his most recent research, the most cited papers focused on:
- Astrophysics
- Astronomy
- Electron
His primary areas of study are Astrophysics, Astronomy, Magnetar, Neutron star and Gamma ray.
Sandro Mereghetti interconnects Spectral line and X-ray in the investigation of issues within Astrophysics.
His Astronomy study often links to related topics such as Cherenkov Telescope Array.
His Magnetar research incorporates elements of Scattering and Supernova.
His Neutron star research focuses on White dwarf and how it connects with Magnetosphere and Young stellar object.
His Gamma ray study incorporates themes from COSMIC cancer database and Sky.
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.
