What is she best known for?
The fields of study she is best known for:
- Galaxy
- Astronomy
- Milky Way
Her scientific interests lie mostly in Astrophysics, Astronomy, Galaxy, Galaxy cluster and Elliptical galaxy.
Her Redshift, Galaxy group, Brightest cluster galaxy, Luminous infrared galaxy and Lenticular galaxy investigations are all subjects of Astrophysics research.
Bianca M. Poggianti studied Brightest cluster galaxy and Peculiar galaxy that intersect with Luminosity function and Coma Cluster.
The various areas that she examines in her Galaxy study include Universe and Sky.
Bianca M. Poggianti combines subjects such as Galaxy formation and evolution and Radius with her study of Galaxy cluster.
Her Star formation research incorporates themes from Infrared and Photometric system.
Her most cited work include:
- Evolution since Z = 0.5 of the morphology-density relation for clusters of galaxies (911 citations)
- The Star Formation Histories of Galaxies in Distant Clusters (642 citations)
- A Spectroscopic catalog of 10 distant rich clusters of galaxies (504 citations)
What are the main themes of her work throughout her whole career to date?
Bianca M. Poggianti mostly deals with Astrophysics, Galaxy, Galaxy cluster, Redshift and Astronomy.
Her works in Star formation, Elliptical galaxy, Brightest cluster galaxy, Galaxy group and Luminous infrared galaxy are all subjects of inquiry into Astrophysics.
The study incorporates disciplines such as Lenticular galaxy, Open cluster and Interacting galaxy in addition to Brightest cluster galaxy.
Her biological study spans a wide range of topics, including Stars and Spectral line.
Her research in Galaxy cluster intersects with topics in Luminosity function, Radio galaxy and Photometry.
Her Redshift research is multidisciplinary, incorporating perspectives in Spectroscopy, Luminosity, Spiral galaxy, Sigma and Velocity dispersion.
She most often published in these fields:
- Astrophysics (95.50%)
- Galaxy (71.62%)
- Galaxy cluster (44.59%)
What were the highlights of her more recent work (between 2017-2021)?
- Astrophysics (95.50%)
- Galaxy (71.62%)
- Star formation (30.63%)
In recent papers she was focusing on the following fields of study:
The scientist’s investigation covers issues in Astrophysics, Galaxy, Star formation, Redshift and Ram pressure.
Her work on Galaxy cluster, Brightest cluster galaxy and Dark matter as part of general Astrophysics study is frequently linked to Center and Projection, therefore connecting diverse disciplines of science.
Her work in Galaxy cluster addresses subjects such as Field galaxy, which are connected to disciplines such as Galaxy group and Anisotropy.
Her Galaxy study contributes to a more complete understanding of Astronomy.
The concepts of her Star formation study are interwoven with issues in Spectral line, Universe and Milky Way.
Her work deals with themes such as Galaxy formation and evolution, Radius, Velocity dispersion and Point source, which intersect with Redshift.
Between 2017 and 2021, her most popular works were:
- The XXL Survey: XXVII. The 3XLSS point source catalogue (31 citations)
- GASP. XXII. The Molecular Gas Content of the JW100 Jellyfish Galaxy at z ∼ 0.05: Does Ram Pressure Promote Molecular Gas Formation? (20 citations)
- The GOGREEN survey: the environmental dependence of the star-forming galaxy main sequence at 1.0 < z < 1.5 (20 citations)
In her most recent research, the most cited papers focused on:
- Galaxy
- Astronomy
- Milky Way
Her primary scientific interests are in Astrophysics, Galaxy, Redshift, Star formation and Ram pressure.
Her work in the fields of Galaxy cluster, Photometric redshift and Universe overlaps with other areas such as Context.
Her Galaxy cluster research is multidisciplinary, incorporating elements of Cosmology and Field galaxy.
Her research links Line with Galaxy.
Her Redshift study combines topics from a wide range of disciplines, such as Radio galaxy, Giant Metrewave Radio Telescope, Supercluster and Point source.
She interconnects Virial theorem and Sky in the investigation of issues within Star formation.
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