Tufts University
United States
His main research concerns Astrophysics, Galaxy, Astronomy, Redshift and Galaxy formation and evolution. His study in Luminous infrared galaxy, Radio galaxy and Quasar are all subfields of Astrophysics. The study incorporates disciplines such as Cosmology and Stars, Spitzer Space Telescope in addition to Galaxy.
His research in Star formation and Emission spectrum are components of Astronomy. His Redshift research is multidisciplinary, incorporating elements of Number density, Spectral line and Photometry. Within one scientific family, Danilo Marchesini focuses on topics pertaining to Elliptical galaxy under Galaxy formation and evolution, and may sometimes address concerns connected to Stellar density and Black hole.
His primary areas of investigation include Astrophysics, Galaxy, Redshift, Astronomy and Stellar mass. All of his Astrophysics and Star formation, Galaxy formation and evolution, Luminous infrared galaxy, Stellar population and Photometry investigations are sub-components of the entire Astrophysics study. His Galaxy formation and evolution research focuses on Spectral resolution and how it connects with Extended Groth Strip.
The concepts of his Galaxy study are interwoven with issues in Stars and Universe. His Redshift study combines topics from a wide range of disciplines, such as Number density, Spectral line, Halo and Effective radius. Danilo Marchesini interconnects Spectral energy distribution, Star, Emission spectrum and Velocity dispersion in the investigation of issues within Stellar mass.
Danilo Marchesini focuses on Astrophysics, Galaxy, Redshift, Stellar mass and Star formation. His work on Luminous infrared galaxy, Galaxy merger, Metallicity and Elliptical galaxy is typically connected to Content as part of general Astrophysics study, connecting several disciplines of science. His Galaxy research is classified as research in Astronomy.
His specific area of interest is Astronomy, where Danilo Marchesini studies Galaxy formation and evolution. His Redshift research is multidisciplinary, incorporating perspectives in Stars, Stellar population, Wide Field Camera 3, Galaxy cluster and Velocity dispersion. His research integrates issues of Spectral line, Starlight and Active galactic nucleus in his study of Star formation.
The scientist’s investigation covers issues in Astrophysics, Galaxy, Redshift, Stellar mass and Star formation. Many of his research projects under Astrophysics are closely connected to Content with Content, tying the diverse disciplines of science together. His Galaxy study is concerned with the field of Astronomy as a whole.
His studies in Redshift integrate themes in fields like Stars, Photometry, Wide Field Camera 3, Galaxy cluster and Universe. He has included themes like Spectroscopy and Weak gravitational lensing in his Photometry study. As part of the same scientific family, he usually focuses on Stellar mass, concentrating on Stellar population and intersecting with Radius, Effective radius, Mass ratio and Luminosity.
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.
An ultra-deep near-infrared spectrum of a compact quiescent galaxy at z=2.2
Mariska Kriek;Pieter G. van Dokkum;Ivo Labbé;Marijn Franx.
The Astrophysical Journal (2009)
THE EVOLUTION OF THE STELLAR MASS FUNCTIONS OF STAR-FORMING AND QUIESCENT GALAXIES TO z = 4 FROM THE COSMOS/UltraVISTA SURVEY*
Adam Muzzin;Danilo Marchesini;Mauro Stefanon;Marijn Franx.
The Astrophysical Journal (2013)
The Growth of Massive Galaxies Since z = 2
Pieter G. van Dokkum;Pieter G. van Dokkum;Katherine E. Whitaker;Katherine E. Whitaker;Gabriel Brammer;Gabriel Brammer;Marijn Franx.
The Astrophysical Journal (2010)
Confirmation of the Remarkable Compactness of Massive Quiescent Galaxies at z ~ 2.3: Early-Type Galaxies Did not Form in a Simple Monolithic Collapse* **
Pieter G. van Dokkum;Marijn Franx;Mariska Kriek;Bradford Holden.
The Astrophysical Journal (2008)
3D-HST WFC3-selected Photometric Catalogs in the Five CANDELS/3D-HST Fields: Photometry, Photometric Redshifts, and Stellar Masses
Rosalind E. Skelton;Katherine E. Whitaker;Ivelina G. Momcheva;Gabriel B. Brammer.
Astrophysical Journal Supplement Series (2014)
The 3D-HST Survey: Hubble Space Telescope WFC3/G141 grism spectra, redshifts, and emission line measurements for $\sim 100,000$ galaxies
Ivelina G. Momcheva;Gabriel B. Brammer;Pieter G. van Dokkum;Rosalind E. Skelton.
arXiv: Astrophysics of Galaxies (2015)
3D-HST: a wide-field grism spectroscopic survey with the Hubble Space Telescope
Gabriel B. Brammer;Pieter G. Van Dokkum;Marijn Franx;Mattia Fumagalli.
Astrophysical Journal Supplement Series (2012)
A PUBLIC K-s-SELECTED CATALOG IN THE COSMOS/ULTRAVISTA FIELD: PHOTOMETRY, PHOTOMETRIC REDSHIFTS, AND STELLAR POPULATION PARAMETERS
Adam Muzzin;Danilo Marchesini;Mauro Stefanon;Marijn Franx.
Astrophysical Journal Supplement Series (2013)
THE EVOLUTION OF THE STELLAR MASS FUNCTION OF GALAXIES FROM z = 4.0 AND THE FIRST COMPREHENSIVE ANALYSIS OF ITS UNCERTAINTIES: EVIDENCE FOR MASS-DEPENDENT EVOLUTION*
Danilo Marchesini;Pieter G. van Dokkum;Natascha M. Förster Schreiber;Marijn Franx.
The Astrophysical Journal (2009)
A Public Ks-selected Catalog in the COSMOS/UltraVISTA Field: Photometry, Photometric Redshifts and Stellar Population Parameters
Adam Muzzin;Danilo Marchesini;Mauro Stefanon;Marijn Franx.
arXiv: Cosmology and Nongalactic Astrophysics (2013)
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