Pascale Jablonka

What is she best known for?

The fields of study she is best known for:

• Galaxy
• Milky Way
• Astronomy

Her scientific interests lie mostly in Astrophysics, Astronomy, Galaxy, Dwarf galaxy and Dwarf spheroidal galaxy. Her work is connected to Milky Way, Galaxy formation and evolution, Metallicity, Galaxy cluster and Globular cluster, as a part of Astrophysics. Stellar population, Elliptical galaxy, Velocity dispersion, Stars and Galaxy group are the subjects of her Astronomy studies.

Her study looks at the relationship between Elliptical galaxy and fields such as Luminous infrared galaxy, as well as how they intersect with chemical problems. Her research in Galaxy is mostly focused on Star formation. In Dwarf galaxy, she works on issues like Spiral galaxy, which are connected to Blue straggler and Galactic halo.

Her most cited work include:

• Two distinct ancient components in the Sculptor dwarf spheroidal galaxy: First results from the dwarf abundances and radial velocities team (325 citations)
• The DART Imaging And CaT Survey of the Fornax Dwarf Spheroidal Galaxy (297 citations)
• The evolution of the star formation activity in galaxies and its dependence on environment (277 citations)

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

Pascale Jablonka mainly focuses on Astrophysics, Galaxy, Astronomy, Metallicity and Stars. Her study in Astrophysics concentrates on Dwarf galaxy, Milky Way, Galaxy cluster, Star formation and Redshift. Her study in Elliptical galaxy, Globular cluster, Lenticular galaxy, Brightest cluster galaxy and Galaxy group is done as part of Astronomy.

While the research belongs to areas of Elliptical galaxy, Pascale Jablonka spends her time largely on the problem of Luminous infrared galaxy, intersecting her research to questions surrounding Radio galaxy. Her Metallicity research is multidisciplinary, incorporating elements of Interstellar medium, Supernova and Dwarf spheroidal galaxy. Her Stars research is multidisciplinary, incorporating perspectives in Spectral line and Galactic halo.

She most often published in these fields:

• Astrophysics (147.63%)
• Galaxy (106.31%)
• Astronomy (76.66%)

What were the highlights of her more recent work (between 2018-2021)?

• Galaxy (106.31%)
• Astrophysics (147.63%)
• Dwarf galaxy (46.69%)

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

Her primary areas of investigation include Galaxy, Astrophysics, Dwarf galaxy, Star formation and Stars. The Galaxy study combines topics in areas such as Spectroscopy and Spectral line. Metallicity, Stellar mass, Milky Way, Local Group and Halo are the primary areas of interest in her Astrophysics study.

Her study in Metallicity is interdisciplinary in nature, drawing from both Stellar population and Dwarf spheroidal galaxy. Her study explores the link between Milky Way and topics such as Accretion that cross with problems in Elliptic orbit. Astronomy covers Pascale Jablonka research in Galaxy formation and evolution.

Between 2018 and 2021, her most popular works were:

• 4MOST: Project overview and information for the First Call for Proposals (74 citations)
• The Pristine Dwarf-Galaxy survey – II. In-depth observational study of the faint Milky Way satellite Sagittarius II (25 citations)
• The Pristine Dwarf-Galaxy survey – II. In-depth observational study of the faint Milky Way satellite Sagittarius II (25 citations)

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

• Galaxy
• Milky Way
• Astronomy

Pascale Jablonka mainly investigates Galaxy, Astrophysics, Redshift, Star formation and Galaxy cluster. Her Galaxy study is focused on Astronomy in general. Astrophysics is a component of her Stellar mass, Dwarf galaxy and Velocity dispersion studies.

Her work deals with themes such as Metallicity and Milky Way, which intersect with Dwarf galaxy. Her Metallicity research integrates issues from Dwarf spheroidal galaxy and White dwarf. The various areas that Pascale Jablonka examines in her Redshift study include Universe and Dark matter.