Materials Map

Discover the materials research landscape. Find experts, partners, networks.

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The Materials Map is an open tool for improving networking and interdisciplinary exchange within materials research. It enables cross-database search for cooperation and network partners and discovering of the research landscape.

The dashboard provides detailed information about the selected scientist, e.g. publications. The dashboard can be filtered and shows the relationship to co-authors in different diagrams. In addition, a link is provided to find contact information.

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The Materials Map is still under development. In its current state, it is only based on one single data source and, thus, incomplete and contains duplicates. We are working on incorporating new open data sources like ORCID to improve the quality and the timeliness of our data. We will update Materials Map as soon as possible and kindly ask for your patience.

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Naji, M.
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in Cooperation with on an Cooperation-Score of 37%

Topics

Publications (4/4 displayed)

  • 2022Cosmic dust evolution: The challenges for NIKA2citations
  • 2021A nearby galaxy perspective on dust evolution. Scaling relations and constraints on the dust build-up in galaxies with the DustPedia and DGS samples85citations
  • 2020A hierarchical bayesian dust SED model and its application to the nearby universecitations
  • 2019A systematic metallicity study of DustPedia galaxies reveals evolution in the dust-to-metal ratios206citations

Places of action

Chart of shared publication
Mosenkov, Aleksandr
1 / 1 shared
Dobbels, Wouter
1 / 1 shared
Baes, Maarten
1 / 5 shared
Xilouris, Emmanuel M.
1 / 1 shared
Roychowdhury, Sambit
2 / 2 shared
Madden, Suzanne C.
1 / 2 shared
Jones, Anthony P.
1 / 5 shared
Casasola, Viviana
1 / 1 shared
Bianchi, Simone
1 / 6 shared
Cassará, Letizia P.
1 / 1 shared
Fritz, Jacopo
1 / 3 shared
Ysard, Nathalie
1 / 3 shared
De Looze, Ilse
1 / 10 shared
Galametz, Maud
1 / 2 shared
Nersesian, Angelos
1 / 4 shared
De Vis, P.
1 / 5 shared
Cassara, L. P.
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Ysard, N.
1 / 14 shared
Bianchi, S.
1 / 7 shared
Clark, C. J. R.
1 / 5 shared
Galametz, M.
1 / 7 shared
Madden, S.
1 / 6 shared
Baes, M.
1 / 12 shared
Xilouris, E. M.
1 / 5 shared
Viaene, S.
1 / 3 shared
Mosenkov, A. V.
1 / 2 shared
Casasola, V.
1 / 2 shared
De Looze, I.
1 / 13 shared
Jones, A.
1 / 13 shared
Lianou, S.
1 / 2 shared
Davies, J. I.
1 / 3 shared
Nersesian, A.
1 / 4 shared
Manilla-Robles, A.
1 / 2 shared
Chart of publication period
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Co-Authors (by relevance)

  • Mosenkov, Aleksandr
  • Dobbels, Wouter
  • Baes, Maarten
  • Xilouris, Emmanuel M.
  • Roychowdhury, Sambit
  • Madden, Suzanne C.
  • Jones, Anthony P.
  • Casasola, Viviana
  • Bianchi, Simone
  • Cassará, Letizia P.
  • Fritz, Jacopo
  • Ysard, Nathalie
  • De Looze, Ilse
  • Galametz, Maud
  • Nersesian, Angelos
  • De Vis, P.
  • Cassara, L. P.
  • Ysard, N.
  • Bianchi, S.
  • Clark, C. J. R.
  • Galametz, M.
  • Madden, S.
  • Baes, M.
  • Xilouris, E. M.
  • Viaene, S.
  • Mosenkov, A. V.
  • Casasola, V.
  • De Looze, I.
  • Jones, A.
  • Lianou, S.
  • Davies, J. I.
  • Nersesian, A.
  • Manilla-Robles, A.
OrganizationsLocationPeople

document

A hierarchical bayesian dust SED model and its application to the nearby universe

  • Galliano, Frédéric
Abstract

In this paper, I review several dust evolution studies based on the DustPedia nearby galaxy sample. I first present the dust spectral energy distribution model, implementing a hierarchical Bayesian method, that we have developed. I then discuss the dust evolution trends we have derived among (integrated) and within (resolved) galaxies. In particular, we show that the trend of dust-to-gas ratio with metallicity is clearly non-linear, indicating the need for grain growth in the interstellar medium. Our trend is closer to the one derived with damped Lyα systems than what was suggested by previous studies. We finally demonstrate the universal processing of small amorphous carbon grains by stellar photons....

Topics
  • impedance spectroscopy
  • amorphous
  • Carbon
  • grain
  • grain growth