What is he best known for?
The fields of study he is best known for:
- Galaxy
- Astronomy
- Astrophysics
His primary areas of study are Astrophysics, Galaxy, Redshift, Astronomy and Star formation.
His Astrophysics study is mostly concerned with Stellar mass, Photometry, Hubble Ultra-Deep Field, Active galactic nucleus and Quasar.
His study on Stellar mass also encompasses disciplines like
- Stellar population and Doubly ionized oxygen most often made with reference to Metallicity,
- Mass growth which intersects with area such as Spectrometer.
Nimish P. Hathi has researched Hubble Ultra-Deep Field in several fields, including Low Mass, Surface brightness, Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey and Advanced Camera for Surveys.
His Redshift research is multidisciplinary, relying on both COSMIC cancer database and Emission spectrum.
Nimish P. Hathi combines subjects such as Spectral line, Stellar evolution and Accretion with his study of Star formation.
His most cited work include:
- CANDELS: The Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey (1588 citations)
- CANDELS: The Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey - The Hubble Space Telescope Observations, Imaging Data Products and Mosaics (1582 citations)
- Candels: The cosmic assembly near-infrared deep extragalactic legacy survey - The hubble space telescope observations, imaging data products, and mosaics (1567 citations)
What are the main themes of his work throughout his whole career to date?
His primary areas of investigation include Astrophysics, Galaxy, Redshift, Astronomy and Star formation.
His Astrophysics research includes themes of Spectral line and Emission spectrum.
Galaxy is often connected to Stars in his work.
His study in Redshift is interdisciplinary in nature, drawing from both Line, Metallicity, Active galactic nucleus and Photometry.
His Star formation research incorporates elements of COSMIC cancer database and Universe.
The various areas that Nimish P. Hathi examines in his Stellar mass study include Extinction, Spectral energy distribution, Accretion and Dwarf galaxy.
He most often published in these fields:
- Astrophysics (97.26%)
- Galaxy (84.54%)
- Redshift (61.25%)
What were the highlights of his more recent work (between 2019-2021)?
- Astrophysics (97.26%)
- Galaxy (84.54%)
- Redshift (61.25%)
In recent papers he was focusing on the following fields of study:
Astrophysics, Galaxy, Redshift, Star formation and Stellar mass are his primary areas of study.
His Astrophysics study frequently draws parallels with other fields, such as Emission spectrum.
His work deals with themes such as Spectral line, Equivalent width and Continuum, which intersect with Galaxy.
The concepts of his Redshift study are interwoven with issues in Atacama Large Millimeter Array, Universe, Infrared and Photometry.
His research integrates issues of COSMIC cancer database and Galaxy formation and evolution in his study of Star formation.
His Stellar mass research incorporates themes from Halo and Far infrared.
Between 2019 and 2021, his most popular works were:
- The ALPINE-ALMA [CII] Survey: Data processing, catalogs, and statistical source properties (46 citations)
- The ALPINE–ALMA [C ii] Survey: Multiwavelength Ancillary Data and Basic Physical Measurements (41 citations)
- The ALPINE-ALMA [CII] survey. Little to no evolution in the [CII]-SFR relation over the last 13 Gyr (40 citations)
In his most recent research, the most cited papers focused on:
- Galaxy
- Astronomy
- Astrophysics
Nimish P. Hathi focuses on Astrophysics, Galaxy, Redshift, Star formation and Stellar mass.
His research combines Equivalent width and Astrophysics.
His Galaxy study combines topics in areas such as Stars, Spectral line and Continuum.
His studies deal with areas such as Atacama Large Millimeter Array and Interstellar medium as well as Redshift.
His Star formation research is multidisciplinary, incorporating elements of Galaxy formation and evolution and Luminosity function.
His Stellar mass research is multidisciplinary, incorporating perspectives in Halo and Metal absorption.
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