D-Index & Metrics Best Publications
Jacqueline Hodge

Jacqueline Hodge

Leiden University
Netherlands

Overview

What is she best known for?

The fields of study she is best known for:

  • Galaxy
  • Astronomy
  • Milky Way

Her main research concerns Galaxy, Astrophysics, Star formation, Astronomy and Redshift. Her Galaxy research focuses on subjects like Stars, which are linked to Radius. Millimeter, Submillimeter Array and Galaxy formation and evolution are the core of her Astrophysics study.

Jacqueline Hodge has included themes like Spectral line, Spectral index, Position angle, Effective radius and Dust emission in her Submillimeter Array study. Her Star formation research includes themes of Line, Luminosity and Stellar evolution. Her research brings together the fields of Stellar mass and Redshift.

Her most cited work include:

  • The 2014 ALMA Long Baseline Campaign: First Results from High Angular Resolution Observations toward the HL TAU Region (901 citations)
  • FIRST RESULTS FROM HIGH ANGULAR RESOLUTION ALMA OBSERVATIO NS TOWARD THE HL TAU REGION (895 citations)
  • AN ALMA SURVEY OF SUB-MILLIMETER GALAXIES IN THE EXTENDED CHANDRA DEEP FIELD SOUTH: PHYSICAL PROPERTIES DERIVED FROM ULTRAVIOLET-TO-RADIO MODELING (293 citations)

What are the main themes of her work throughout her whole career to date?

Jacqueline Hodge mostly deals with Astrophysics, Galaxy, Redshift, Star formation and Astronomy. Her study involves Luminosity, Quasar, Hubble Ultra-Deep Field, Luminous infrared galaxy and Active galactic nucleus, a branch of Astrophysics. The various areas that she examines in her Quasar study include Photometry, Galaxy cluster and Sky.

Her Galaxy research is multidisciplinary, incorporating perspectives in Line and Millimeter. Her studies deal with areas such as COSMIC cancer database, Interstellar medium and Emission spectrum as well as Redshift. Her biological study spans a wide range of topics, including Accretion, Metallicity and Infrared.

She most often published in these fields:

  • Astrophysics (106.25%)
  • Galaxy (98.56%)
  • Redshift (50.00%)

What were the highlights of her more recent work (between 2017-2021)?

  • Galaxy (98.56%)
  • Astrophysics (106.25%)
  • Redshift (50.00%)

In recent papers she was focusing on the following fields of study:

Jacqueline Hodge mainly focuses on Galaxy, Astrophysics, Redshift, Star formation and Luminosity. In her research on the topic of Galaxy, Brightness temperature and Photometric redshift is strongly related with Millimeter. Her research ties Spectral line and Astrophysics together.

Her Redshift research incorporates elements of Billion years, Stellar mass, Luminous infrared galaxy and Emission spectrum. Her Star formation study which covers Spiral galaxy that intersects with Eddington luminosity and Chandra Deep Field South. Her biological study deals with issues like Line, which deal with fields such as Excitation temperature, Mass ratio and Optical depth.

Between 2017 and 2021, her most popular works were:

  • Rotation in [C ii ]-emitting gas in two galaxies at a redshift of 6.8 (96 citations)
  • The Karl G. Jansky Very Large Array Sky Survey (VLASS). Science case and survey design (90 citations)
  • COLDz: Shape of the CO Luminosity Function at High Redshift and the Cold Gas History of the Universe (86 citations)

In her most recent research, the most cited papers focused on:

  • Galaxy
  • Astronomy
  • Milky Way

The scientist’s investigation covers issues in Galaxy, Astrophysics, Redshift, Star formation and Luminosity. Her Galaxy study frequently draws connections to other fields, such as Baryon. Astrophysics and Far ultraviolet are frequently intertwined in her study.

The study incorporates disciplines such as Cosmology and Millimeter in addition to Redshift. Her studies in Star formation integrate themes in fields like COSMIC cancer database and Spiral galaxy. Jacqueline Hodge usually deals with Luminosity and limits it to topics linked to Line and Multi Unit Spectroscopic Explorer, Spectroscopy and Galaxy formation and evolution.

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.

Best Publications

FIRST RESULTS FROM HIGH ANGULAR RESOLUTION ALMA OBSERVATIO NS TOWARD THE HL TAU REGION

Partnership Alma;C. L. Brogan;L. M. Perez;T. R. Hunter.
arXiv: Solar and Stellar Astrophysics (2015)

1542 Citations

The 2014 ALMA Long Baseline Campaign: First Results from High Angular Resolution Observations toward the HL Tau Region

Alma Partnership;C. L. Brogan;L. M. Pérez;T. R. Hunter.
The Astrophysical Journal (2015)

1042 Citations

An ALMA survey of Sub-millimeter Galaxies in the Extended Chandra Deep Field South: Physical properties derived from ultraviolet-to-radio modelling

Elisabete da Cunha;Fabian Walter;Ian Smail;Mark Swinbank.
arXiv: Astrophysics of Galaxies (2015)

483 Citations

AN ALMA SURVEY OF SUB-MILLIMETER GALAXIES IN THE EXTENDED CHANDRA DEEP FIELD SOUTH: PHYSICAL PROPERTIES DERIVED FROM ULTRAVIOLET-TO-RADIO MODELING

E. da Cunha;F. Walter;I. R. Smail;A. M. Swinbank.
The Astrophysical Journal (2015)

357 Citations

AN ALMA SURVEY OF SUBMILLIMETER GALAXIES IN THE EXTENDED CHANDRA DEEP FIELD SOUTH: SOURCE CATALOG AND MULTIPLICITY

J. A. Hodge;A. Karim;I. Smail;A. M. Swinbank.
The Astrophysical Journal (2013)

346 Citations

An ALMA survey of sub-millimetre Galaxies in the Extended Chandra Deep Field South: the far-infrared properties of SMGs

A. M. Swinbank;J. M. Simpson;Ian Smail;C. M. Harrison.
Monthly Notices of the Royal Astronomical Society (2014)

336 Citations

Kiloparsec-scale dust disks in high-redshift luminous submillimeter galaxies

J. A. Hodge;A. M. Swinbank;J. M. Simpson;I. Smail.
arXiv: Astrophysics of Galaxies (2016)

310 Citations

An ALMA survey of submillimetre galaxies in the Extended Chandra Deep Field South: high-resolution 870 μm source counts

A. Karim;A. M. Swinbank;J. A. Hodge;I. R. Smail.
Monthly Notices of the Royal Astronomical Society (2013)

298 Citations

An ALMA survey of submillimeter galaxies in the Extended Chandra Deep Field South : the redshift distribution and evolution of submillimeter galaxies.

J. M. Simpson;A. M. Swinbank;Ian Smail;D. M. Alexander.
The Astrophysical Journal (2014)

297 Citations

Evidence for a Clumpy, Rotating Gas Disk in a Submillimeter Galaxy at z = 4

J. A. Hodge;C. L. Carilli;F. Walter;F. Walter;W. J. G. de Blok;W. J. G. de Blok.
The Astrophysical Journal (2012)

286 Citations

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