What is she best known for?
The fields of study she is best known for:
- Quantum mechanics
- Galaxy
- Astrophysics
Andrea V. Macciò mainly investigates Astrophysics, Astronomy, Galaxy, Dark matter and Galaxy formation and evolution.
Her work is connected to Halo, Cold dark matter, Dark matter halo, Galaxy rotation curve and Star formation, as a part of Astrophysics.
Her studies in Halo integrate themes in fields like Cosmology, Scale, Surface brightness and Virial theorem.
Her work in Galaxy addresses subjects such as Stars, which are connected to disciplines such as Supernova.
Her Dark matter study incorporates themes from Dark energy, Baryon, Galaxy cluster and Dwarf galaxy.
The concepts of her Galaxy formation and evolution study are interwoven with issues in Galactic halo and Luminosity function.
Her most cited work include:
- Constraints on the relationship between stellar mass and halo mass at low and high redshift (991 citations)
- Concentration, spin and shape of dark matter haloes as a function of the cosmological model: WMAP1, WMAP3 and WMAP5 results (633 citations)
- Cold dark matter haloes in the Planck era: evolution of structural parameters for Einasto and NFW profiles (574 citations)
What are the main themes of her work throughout her whole career to date?
Andrea V. Macciò mainly focuses on Astrophysics, Galaxy, Dark matter, Halo and Galaxy formation and evolution.
Her work on Astrophysics is being expanded to include thematically relevant topics such as Astronomy.
Her study brings together the fields of Stars and Galaxy.
Andrea V. Macciò has researched Dark matter in several fields, including Radius, Baryon, Cosmology, Dark energy and Galaxy cluster.
Her Halo study combines topics from a wide range of disciplines, such as Surface brightness, Redshift, Virial theorem and Angular momentum.
Her Galaxy formation and evolution study integrates concerns from other disciplines, such as Accretion and Reionization.
She most often published in these fields:
- Astrophysics (132.32%)
- Galaxy (103.05%)
- Dark matter (65.85%)
What were the highlights of her more recent work (between 2018-2021)?
- Astrophysics (132.32%)
- Galaxy (103.05%)
- Dark matter (65.85%)
In recent papers she was focusing on the following fields of study:
Her scientific interests lie mostly in Astrophysics, Galaxy, Dark matter, Halo and Galaxy formation and evolution.
In her work, Radiation is strongly intertwined with Photoionization, which is a subfield of Astrophysics.
Her Galaxy study frequently draws parallels with other fields, such as Radius.
Andrea V. Macciò interconnects Galaxy rotation curve and Kinetic energy in the investigation of issues within Dark matter.
Her studies deal with areas such as Range, Redshift and Relaxation as well as Halo.
Her research in Galaxy formation and evolution intersects with topics in Correlation function and Spatial distribution.
Between 2018 and 2021, her most popular works were:
- NIHAO XV: the environmental impact of the host galaxy on galactic satellite and field dwarf galaxies (56 citations)
- NIHAO XV: the environmental impact of the host galaxy on galactic satellite and field dwarf galaxies (56 citations)
- Formation of ultra-diffuse galaxies in the field and in galaxy groups (49 citations)
In her most recent research, the most cited papers focused on:
- Quantum mechanics
- Galaxy
- Milky Way
Andrea V. Macciò spends much of her time researching Astrophysics, Galaxy, Halo, Star formation and Dark matter.
Astrophysics is represented through her Stellar mass, Galaxy formation and evolution, Redshift, Supernova and Stars research.
While the research belongs to areas of Stellar mass, Andrea V. Macciò spends her time largely on the problem of Milky Way, intersecting her research to questions surrounding Virial mass, Scale height and Computational astrophysics.
Her Galaxy research includes themes of Baryon and Angular momentum.
Her research in Star formation focuses on subjects like Cold dark matter, which are connected to Surface brightness and Accretion.
In her study, which falls under the umbrella issue of Dark matter, Newtonian dynamics is strongly linked to Galaxy rotation curve.
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.
