Maud Galametz
Paris Diderot University
238 Papers
3.8K Citations
Maud Galametz is an academic researcher from Paris Diderot University. The author has contributed to research in topics: Galaxy & Star formation. The author has an hindex of 71, co-authored 238 publications. Previous affiliations of Maud Galametz include Imperial College London & University of Cambridge.
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Papers
The CO-to-H2 Conversion Factor and Dust-to-gas Ratio on Kiloparsec Scales in Nearby Galaxies
Karin Sandstrom,Adam K. Leroy,Frederick M. Walter,Alberto D. Bolatto,Kevin V. Croxall,Kevin V. Croxall,Bruce T. Draine,Christine D. Wilson,Mark G. Wolfire,Daniela Calzetti,Robert C. Kennicutt,G. Aniano,G. Aniano,J. Donovan Meyer,Antonio Usero,Frank Bigiel,Elias Brinks,W. J. G. de Blok,Alison F. Crocker,Alison F. Crocker,Daniel A. Dale,Charles W. Engelbracht,Charles W. Engelbracht,Maud Galametz,Brent Groves,Leslie K. Hunt,Jin Koda,Kathryn Kreckel,Hendrik Linz,Sharon E. Meidt,Eric W. Pellegrini,Hans-Walter Rix,Helene Roussel,Eva Schinnerer,Andreas Schruba,K. F. Schuster,Ramin A. Skibba,Ramin A. Skibba,T. P. R. van der Laan,P. N. Appleton,Lee Armus,Bernhard R. Brandl,Karl D. Gordon,J. Hinz,Oliver Krause,E. Montiel,E. Montiel,Marc Sauvage,Anika Schmiedeke,Anika Schmiedeke,J. D. T. Smith,L. Vigroux +51 more
TL;DR: In this paper, the authors presented a large-scale spatial resolution map of the CO-to-H$2}$ conversion factor and dust-togas ratio (DGR) in 26 nearby, star-forming galaxies.
Gas-to-dust mass ratios in local galaxies over a 2 dex metallicity range
A. Rémy-Ruyer,S. C. Madden,Frédéric Galliano,Maud Galametz,Tsutomu T. Takeuchi,Ryosuke Asano,Svitlana Zhukovska,Svitlana Zhukovska,Vianney Lebouteiller,D. Cormier,Anthony P. Jones,M. Bocchio,Maarten Baes,George J. Bendo,Médéric Boquien,Alessandro Boselli,I. Delooze,V. Doublier-Pritchard,Thomas M. Hughes,O. Ł. Karczewski,L. Spinoglio +20 more
TL;DR: In this article, the authors analyzed the behavior of the gas-to-dust mass ratio (G/D) of local Universe galaxies over a wide metallicity range and investigated several explanations for the observed relation and scatter.
KINGFISH—Key Insights on Nearby Galaxies: A Far-Infrared Survey with Herschel: Survey Description and Image Atlas
Robert C. Kennicutt,Daniela Calzetti,G. Aniano,P. N. Appleton,Lee Armus,P. Beirao,Alberto D. Bolatto,Bernhard R. Brandl,Alison F. Crocker,Kevin V. Croxall,Daniel A. Dale,J. Dononvan Meyer,Bruce T. Draine,Charles W. Engelbracht,Maud Galametz,Karl D. Gordon,Brent Groves,Cai-Na Hao,George Helou,J. L. Hinz,Leslie K. Hunt,Benjamin D. Johnson,Jin Koda,Oliver Krause,Adam K. Leroy,Yongbao Li,Sharon E. Meidt,E. Montiel,Eric J. Murphy,Nurur Rahman,H-W. Rix,Helene Roussel,Karin Sandstrom,Marc Sauvage,Eva Schinnerer,Ramin A. Skibba,J. D. T. Smith,Sundar Srinivasan,L. Vigroux,Frederick M. Walter,C. D. Wilson,Mark G. Wolfire,Stefano Zibetti +42 more
TL;DR: The Kingfish project (Key Insights on Nearby Galaxies: a Far-Infrared Survey with Herschel) as discussed by the authors is an imaging and spectroscopic survey of 61 nearby galaxies, chosen to cover a wide range of galaxy properties and local interstellar medium (ISM) environments found in the nearby universe.
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 C. Madden,Maarten Baes,George J. Bendo,Médéric Boquien,Alessandro Boselli,David L. Clements,Luca Cortese,Luca Cortese,Asantha Cooray,Asantha Cooray,Maud Galametz,Frédéric Galliano,Javier Graciá-Carpio,K. G. Isaak,O. Ł. Karczewski,T. J. Parkin,Eric W. Pellegrini,Aurélie Rémy-Ruyer,Luigi Spinoglio,Matthew Smith,Eckhard Sturm +23 more
TL;DR: In this paper, the authors analyzed the applicability of far-infrared fine-structure lines [Cii] 158μm, [Oi] 63μm and [Oiii] 88μm to reliably trace the star formation rate (SFR) in a sample of low-metallicity dwarf galaxies from the Herschel Dwarf Galaxy Survey and furthermore, extended the analysis to a broad sample of galaxies of various types and metallicities in the literature.
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 E. Magdis,Claudia del P. Lagos,Mark Sargent,M. Albrecht,Herve Aussel,Frank Bertoldi,Veronique Buat,Maud Galametz,Sebastien Heinis,Olivier Ilbert,Alexander Karim,Anton M. Koekemoer,Cedric G. Lacey,Emeric Le Floc'h,F. Navarrete,Maurilio Pannella,Corentin Schreiber,Vernesa Smolčić,M. Symeonidis,M. Symeonidis,Marco P. Viero +22 more
TL;DR: In this article, the authors measured the average spectral energy distributions as a function of redshift using a stacking analysis of Spitzer, Herschel, LABOCA and AzTEC data for two samples of galaxies: normal star-forming objects and strong starbursts, as defined by their distance to the main sequence.
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