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Maud Galametz

Maud Galametz

Université Paris Cité
France

Overview

What is she best known for?

The fields of study she is best known for:

Astronomy
Galaxy
Astrophysics

Her primary areas of investigation include Astrophysics, Galaxy, Astronomy, Metallicity and Star formation. Her Astrophysics study is mostly concerned with Interstellar medium, Luminous infrared galaxy, Dwarf galaxy, Extinction and Cosmic dust. Her Cosmic dust research incorporates elements of Emissivity and Molecular cloud.

Her Galaxy study incorporates themes from Stars and Mass ratio. While the research belongs to areas of Metallicity, Maud Galametz spends her time largely on the problem of Intensity, intersecting her research to questions surrounding Star, Radio galaxy and Hydrogen line. As a part of the same scientific study, Maud Galametz usually deals with the Star formation, concentrating on Redshift and frequently concerns with Initial mass function.

Her most cited work include:

The CO-to-H2 Conversion Factor and Dust-to-gas Ratio on Kiloparsec Scales in Nearby Galaxies (441 citations)
Gas-to-dust mass ratios in local galaxies over a 2 dex metallicity range (392 citations)
KINGFISH—Key Insights on Nearby Galaxies: A Far-Infrared Survey with Herschel: Survey Description and Image Atlas (383 citations)

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

Maud Galametz mainly investigates Astrophysics, Galaxy, Astronomy, Star formation and Interstellar medium. Her Astrophysics research focuses on Metallicity, Luminous infrared galaxy, Stars, Spectral energy distribution and Cosmic dust. Her Metallicity study combines topics in areas such as Wavelength and Mass ratio.

Her Galaxy research is multidisciplinary, incorporating elements of Line and Infrared. The study incorporates disciplines such as Radiative transfer, Luminosity, Surface brightness and Molecular cloud in addition to Star formation. Maud Galametz has included themes like Spectral line, Emission spectrum, Universe and Spire in her Interstellar medium study.

She most often published in these fields:

Astrophysics (97.57%)
Galaxy (81.94%)
Astronomy (43.75%)

What were the highlights of her more recent work (between 2018-2021)?

Astrophysics (97.57%)
Galaxy (81.94%)
Star formation (42.01%)

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

Maud Galametz spends much of her time researching Astrophysics, Galaxy, Star formation, Metallicity and Stars. Many of her studies on Astrophysics apply to Radiative transfer as well. Her work deals with themes such as Cosmic dust and Mass ratio, which intersect with Galaxy.

Her work carried out in the field of Cosmic dust brings together such families of science as Luminous infrared galaxy and Photometry. Her Star formation research is multidisciplinary, incorporating perspectives in Continuum, Wavelength and Molecular cloud. Her studies deal with areas such as Universe and Dwarf galaxy as well as Metallicity.

Between 2018 and 2021, her most popular works were:

A systematic metallicity study of DustPedia galaxies reveals evolution in the dust-to-metal ratios (70 citations)
Comprehensive comparison of models for spectral energy distributions from 0.1 μm to 1 mm of nearby star-forming galaxies (45 citations)
Comprehensive comparison of models for spectral energy distributions from 0.1 μm to 1 mm of nearby star-forming galaxies (45 citations)

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

Gas-to-dust mass ratios in local galaxies over a 2 dex metallicity range

Aurélie Rémy-Ruyer;S. C. Madden;F. Galliano;M. Galametz.
Astronomy and Astrophysics (2014)

510 Citations

The CO-to-H2 Conversion Factor and Dust-to-gas Ratio on Kiloparsec Scales in Nearby Galaxies

K. M. Sandstrom;A. K. Leroy;F. Walter;A. D. Bolatto.
The Astrophysical Journal (2013)

487 Citations

KINGFISH—Key Insights on Nearby Galaxies: A Far-Infrared Survey with Herschel: Survey Description and Image Atlas

R. C. Kennicutt;D. Calzetti;G. Aniano;P. Appleton.
Publications of the Astronomical Society of the Pacific (2011)

451 Citations

The applicability of FIR fine-structure lines as Star Formation Rate tracers over wide ranges of metallicities and galaxy types

Ilse De Looze;Diane Cormier;Vianney Lebouteiller;Suzanne Madden.
arXiv: Astrophysics of Galaxies (2014)

415 Citations

The Herschel Reference Survey

A. Boselli;S. Eales;L. Cortese;G. Bendo.
arXiv: Cosmology and Nongalactic Astrophysics (2010)

399 Citations

Herschel Far-Infrared and Sub-millimeter Photometry for the KINGFISH Sample of Nearby Galaxies

D. A. Dale;G. Aniano;C. W. Engelbracht;J. L. Hinz.
arXiv: Cosmology and Nongalactic Astrophysics (2011)

376 Citations

Evolution of the dust emission of massive galaxies up to z=4 and constraints on their dominant mode of star formation

Matthieu Béthermin;Emanuele Daddi;Georgios Magdis;Claudia Lagos.
arXiv: Astrophysics of Galaxies (2014)

349 Citations

The applicability of far-infrared fine-structure lines as star formation rate tracers over wide ranges of metallicities and galaxy types

Ilse De Looze;Diane Cormier;Vianney Lebouteiller;Suzanne Madden.
Astronomy and Astrophysics (2014)

332 Citations

The Herschel Reference Survey

A. Boselli;Stephen Anthony Eales;Luca Cortese;G. Bendo.
Publications of the Astronomical Society of the Pacific (2010)

314 Citations

Probing the Dust Properties of Galaxies at Submillimetre Wavelengths II. Dust-to-gas mass ratio trends with metallicity and the submm excess in dwarf galaxies

Maud Galametz;Suzanne C. Madden;Frederic Galliano;Sacha Hony.
arXiv: Cosmology and Nongalactic Astrophysics (2011)

277 Citations

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