Diego Portales University
Chile
The scientist’s investigation covers issues in Galaxy, Astrophysics, Astronomy, Redshift and Star formation. Manuel Aravena works mostly in the field of Galaxy, limiting it down to concerns involving Millimeter and, occasionally, Telescope. Luminous infrared galaxy, Luminosity, Hubble Ultra-Deep Field, Quasar and Active galactic nucleus are among the areas of Astrophysics where the researcher is concentrating his efforts.
The concepts of his Luminosity study are interwoven with issues in Line and Spectral energy distribution. His work on Hubble Deep Field as part of general Redshift study is frequently connected to Excitation, therefore bridging the gap between diverse disciplines of science and establishing a new relationship between them. Manuel Aravena studied Star formation and Milky Way that intersect with Accretion.
Manuel Aravena mainly focuses on Astrophysics, Galaxy, Redshift, Star formation and Astronomy. His study looks at the relationship between Astrophysics and fields such as Emission spectrum, as well as how they intersect with chemical problems. As part of his studies on Galaxy, Manuel Aravena often connects relevant areas like Millimeter.
Manuel Aravena focuses mostly in the field of Redshift, narrowing it down to topics relating to Spectral energy distribution and, in certain cases, Jansky. He combines subjects such as Accretion, Continuum, Active galactic nucleus, Milky Way and Billion years with his study of Star formation. His work in the fields of Luminosity, such as Luminosity function, intersects with other areas such as Atomic carbon.
Manuel Aravena spends much of his time researching Astrophysics, Galaxy, Redshift, Star formation and Hubble Ultra-Deep Field. In his research, Einstein radius is intimately related to Spectral line, which falls under the overarching field of Astrophysics. His biological study spans a wide range of topics, including Line and Emission spectrum.
Manuel Aravena has researched Redshift in several fields, including COSMIC cancer database, Jansky and Millimeter. His work deals with themes such as Billion years, Quasar, Luminosity function and Infrared excess, which intersect with Star formation. His Hubble Ultra-Deep Field research incorporates elements of Submillimeter Array, Mass ratio and Sigma.
Manuel Aravena mainly investigates Astrophysics, Galaxy, Redshift, Hubble Ultra-Deep Field and Star formation. His Galaxy formation and evolution, Stellar mass, Interstellar medium, Luminosity and Line investigations are all subjects of Astrophysics research. His Galaxy research encompasses a variety of disciplines, including Excitation and Sequence.
The study incorporates disciplines such as Active galactic nucleus and Millimeter in addition to Redshift. His Hubble Ultra-Deep Field research integrates issues from COSMIC cancer database and Submillimeter Array. His research investigates the connection with Star formation and areas like Infrared excess which intersect with concerns in Sigma.
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.
The spitzer survey of stellar structure in galaxies (s^4g)
Kartik Sheth;Kartik Sheth;Michael Regan;Joannah L. Hinz;Armando Gil de Paz.
Publications of the Astronomical Society of the Pacific (2010)
ALMA redshifts of millimeter-selected galaxies from the SPT survey: The redshift distribution of dusty star-forming galaxies
A. Weiss;C. De Breuck;D. P. Marrone;J. D. Vieira.
arXiv: Cosmology and Nongalactic Astrophysics (2013)
Dusty starburst galaxies in the early Universe as revealed by gravitational lensing
J. D. Vieira;D. P. Marrone;S. C. Chapman;S. C. Chapman;C. De Breuck.
Nature (2013)
ALMA redshifts of millimeter-selected galaxies from the SPT survey: The redshift distribution of dusty star-forming galaxies
A. Weiß;C. De Breuck;D. P. Marrone;J. D. Vieira.
The Astrophysical Journal (2013)
ALMA Spectroscopic Survey in the Hubble Ultra Deep Field: The Infrared Excess of UV-selected z=2-10 galaxies as a function of UV-continuum Slope and Stellar Mass
Rychard J Bouwens;Manuel Aravena;Roberto Decarli;Fabian E Walter;Fabian E Walter.
The Astrophysical Journal (2016)
CO excitation of normal star forming galaxies out to z= 1.5 as regulated by the properties of their interstellar medium
Emanuele Daddi;H. Dannerbauer;D. Liu;D. Liu;M. Aravena.
Astronomy and Astrophysics (2015)
Imaging the molecular gas in a submm galaxy at z = 4.05: cold mode accretion or a major merger?
C.L. Carilli;E. Daddi;D. Riechers;F. Walter.
arXiv: Cosmology and Nongalactic Astrophysics (2010)
ALMA Imaging and Gravitational Lens Models of South Pole Telescope-Selected Dusty, Star-Forming Galaxies at High Redshifts
Justin Spilker;Daniel Marrone;Manuel Aravena;Matthieu Bethermin.
arXiv: Astrophysics of Galaxies (2016)
Extragalactic millimeter-wave point source catalog, number counts and statistics from 771 square degrees of the SPT-SZ Survey
L. M. Mocanu;T. M. Crawford;J. D. Vieira;K. A. Aird.
arXiv: Cosmology and Nongalactic Astrophysics (2013)
Imaging the Molecular Gas in a Submillimeter Galaxy at z = 4.05: Cold Mode Accretion or a Major Merger?
C. L. Carilli;E. Daddi;D. Riechers;F. Walter.
The Astrophysical Journal (2010)
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