What is he best known for?
The fields of study he is best known for:
- Galaxy
- Astronomy
- Astrophysics
His primary areas of investigation include Astrophysics, Galaxy, Astronomy, Star formation and Luminous infrared galaxy.
His work in Astrophysics is not limited to one particular discipline; it also encompasses Infrared.
While the research belongs to areas of Galaxy, Dieter Lutz spends his time largely on the problem of Line, intersecting his research to questions surrounding Plateau de Bure Interferometer.
His Star formation research includes elements of Halo, Star and Disc galaxy.
Dieter Lutz works mostly in the field of Luminous infrared galaxy, limiting it down to concerns involving Stellar evolution and, occasionally, Main sequence.
His Redshift research is multidisciplinary, incorporating perspectives in Metallicity and Conjunction.
His most cited work include:
- The Photodetector Array Camera and Spectrometer (PACS) on the Herschel Space Observatory (2260 citations)
- What Powers Ultraluminous IRAS Galaxies (1066 citations)
- What Powers Ultra-luminous IRAS Galaxies? (1034 citations)
What are the main themes of his work throughout his whole career to date?
Astrophysics, Galaxy, Astronomy, Star formation and Luminous infrared galaxy are his primary areas of study.
Dieter Lutz combines subjects such as Spectral line and Infrared with his study of Astrophysics.
His Galaxy research incorporates elements of Line, Emission spectrum and Stars.
His Star formation study combines topics in areas such as Accretion, Metallicity, Halo, Interstellar medium and Bulge.
His work deals with themes such as QSOS and Velocity dispersion, which intersect with Luminous infrared galaxy.
His Redshift study combines topics from a wide range of disciplines, such as Far infrared, Millimeter and Photometry.
He most often published in these fields:
- Astrophysics (90.26%)
- Galaxy (70.16%)
- Astronomy (45.94%)
What were the highlights of his more recent work (between 2014-2021)?
- Astrophysics (90.26%)
- Galaxy (70.16%)
- Star formation (36.95%)
In recent papers he was focusing on the following fields of study:
Dieter Lutz mainly focuses on Astrophysics, Galaxy, Star formation, Astronomy and Redshift.
His works in Active galactic nucleus, Luminous infrared galaxy, Stellar mass, Luminosity and Line are all subjects of inquiry into Astrophysics.
Dieter Lutz combines subjects such as Elliptical galaxy, Stellar evolution, Surface brightness, Far infrared and Emission spectrum with his study of Luminous infrared galaxy.
In his study, Equivalent width is strongly linked to Infrared, which falls under the umbrella field of Galaxy.
His Star formation study integrates concerns from other disciplines, such as Metallicity, Interstellar medium, Photometry and Bulge.
His Redshift research incorporates themes from Galaxy formation and evolution and Halo.
Between 2014 and 2021, his most popular works were:
- COMBINED CO AND DUST SCALING RELATIONS OF DEPLETION TIME AND MOLECULAR GAS FRACTIONS WITH COSMIC TIME, SPECIFIC STAR-FORMATION RATE, AND STELLAR MASS (491 citations)
- The KMOS3D survey: design, first results, and the evolution of galaxy kinematics from 0.7 ≤ z ≤ 2.7 (393 citations)
- PHIBSS: Unified Scaling Relations of Gas Depletion Time and Molecular Gas Fractions (363 citations)
In his most recent research, the most cited papers focused on:
- Galaxy
- Astronomy
- Astrophysics
His main research concerns Astrophysics, Galaxy, Astronomy, Redshift and Luminous infrared galaxy.
As part of the same scientific family, he usually focuses on Astrophysics, concentrating on Emission spectrum and intersecting with Photometric redshift and Velocity dispersion.
His studies deal with areas such as Line, Infrared, Dark matter and Stars as well as Galaxy.
His study on Luminosity and Redshift survey is often connected to Spectral density as part of broader study in Astronomy.
The various areas that he examines in his Luminous infrared galaxy study include Stellar evolution, Radio galaxy, Photometry and Elliptical galaxy.
Dieter Lutz interconnects Surface brightness and Bulge in the investigation of issues within Star formation.
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