What is he best known for?
The fields of study he is best known for:
- Galaxy
- Astronomy
- Astrophysics
Mark Seibert focuses on Astrophysics, Galaxy, Astronomy, Star formation and Stellar mass.
His study in Astrophysics focuses on Elliptical galaxy, Stars, Metallicity, Luminosity function and Surface brightness.
His work deals with themes such as Sky and Photometry, which intersect with Galaxy.
As a part of the same scientific family, he mostly works in the field of Star formation, focusing on Radius and, on occasion, Extinction.
Mark Seibert works mostly in the field of Stellar mass, limiting it down to topics relating to Stellar mass loss and, in certain cases, Young stellar object and Globular cluster, as a part of the same area of interest.
In his study, Baryon, Initial mass function and Star cluster is inextricably linked to Dwarf galaxy, which falls within the broad field of Luminosity.
His most cited work include:
- The Origin of the Mass-Metallicity Relation: Insights from 53,000 Star-forming Galaxies in the Sloan Digital Sky Survey (2961 citations)
- The Origin of the Mass-Metallicity Relation: Insights from 53,000 Star-forming Galaxies in the Sloan Digital Sky Survey (2961 citations)
- The Origin of the Mass--Metallicity Relation: Insights from 53,000 Star-Forming Galaxies in the SDSS (2906 citations)
What are the main themes of his work throughout his whole career to date?
His primary scientific interests are in Astrophysics, Galaxy, Astronomy, Star formation and Stars.
His work in Stellar mass, Galaxy formation and evolution, Redshift, Luminous infrared galaxy and Luminosity are all subfields of Astrophysics research.
His Galaxy research includes elements of Stellar structure, Sky and Photometry.
Astronomy is represented through his Elliptical galaxy, Lenticular galaxy, Metallicity, Radio galaxy and Luminosity function research.
In his work, Milky Way is strongly intertwined with Cepheid variable, which is a subfield of Metallicity.
His Star formation research includes themes of Extinction, Surface brightness, Universe and Active galactic nucleus.
He most often published in these fields:
- Astrophysics (91.65%)
- Galaxy (67.47%)
- Astronomy (49.89%)
What were the highlights of his more recent work (between 2013-2021)?
- Astrophysics (91.65%)
- Galaxy (67.47%)
- Astronomy (49.89%)
In recent papers he was focusing on the following fields of study:
The scientist’s investigation covers issues in Astrophysics, Galaxy, Astronomy, Stars and RR Lyrae variable.
His studies in Photometry, Supernova, Elliptical galaxy, Luminosity and Luminous infrared galaxy are all subfields of Astrophysics research.
His work carried out in the field of Luminosity brings together such families of science as Energy and Apparent magnitude.
His research integrates issues of Disc and Galaxy formation and evolution in his study of Luminous infrared galaxy.
His Galaxy research is multidisciplinary, relying on both Stellar structure and Cepheid variable.
Mark Seibert works mostly in the field of Stellar mass, limiting it down to concerns involving Halo and, occasionally, Baryon.
Between 2013 and 2021, his most popular works were:
- Galaxy and mass assembly (GAMA): End of survey report and data release 2 (352 citations)
- The Carnegie-Chicago Hubble Program. VIII. An Independent Determination of the Hubble Constant Based on the Tip of the Red Giant Branch (255 citations)
- Reconstructing the stellar mass distributions of galaxies using S4G IRAC 3.6 and 4.5 micron images: II. The conversion from light to mass (217 citations)
In his most recent research, the most cited papers focused on:
- Galaxy
- Astronomy
- Milky Way
His main research concerns Astrophysics, Galaxy, Astronomy, Stars and Stellar mass.
His study in Photometry, Elliptical galaxy, Luminous infrared galaxy, Distance modulus and RR Lyrae variable is carried out as part of his studies in Astrophysics.
His studies deal with areas such as Stellar structure and Sky as well as Galaxy.
His work in the fields of Stars, such as Brown dwarf, intersects with other areas such as Visible radiation, Near infrared radiation, Delta-v and White light.
His study in Stellar mass is interdisciplinary in nature, drawing from both Basis and Giant star.
In general Star formation study, his work on Stellar population often relates to the realm of Specific relative angular momentum, thereby connecting several areas of interest.
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