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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Materials Map under construction

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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1.080 Topics available

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977 Locations available

693.932 PEOPLE
693.932 People People

693.932 People

Show results for 693.932 people that are selected by your search filters.

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PeopleLocationsStatistics
Naji, M.
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Mutschke, H.

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in Cooperation with on an Cooperation-Score of 37%

Topics

Publications (9/9 displayed)

  • 2024Interstellar oxygen along the line of sight of Cygnus X-219citations
  • 2023Oxygen and iron in interstellar dust:An X-ray investigation19citations
  • 2018Investigating the interstellar dust through the Fe K-edge27citations
  • 2018Femtosecond laser irradiation of olivine single crystals: Experimental simulation of space weathering31citations
  • 2013The X-ray side of the absorption by interstellar dust in the Milky Waycitations
  • 2012Observational evidence for composite grains in an AGB outflow: MgS in the extreme carbon star LL Pegasi28citations
  • 2011UV irradiation of hydrogenated amorphous carbon (HAC) as a carrier candidate of the interstellar UV bump at 4.6 μm<SUP>-1</SUP>citations
  • 2006Nanodiamond dust and the energy distribution of quasars2citations
  • 2003Spectral properties of carbonaceous and siliceous cosmic dust analogscitations

Places of action

Chart of shared publication
De Groot, F.
4 / 5 shared
Psaradaki, I.
2 / 4 shared
Trasobares Llorente, Susana
1 / 3 shared
Mehdipour, M.
2 / 4 shared
Rogantini, D.
2 / 2 shared
Waters, L. B. F. M.
4 / 14 shared
De Vries, C. P.
3 / 5 shared
Zeegers, S. T.
4 / 5 shared
Costantini, E.
3 / 5 shared
Den Herder, J. W. A.
1 / 2 shared
Trasobares, S.
1 / 3 shared
Corrales, L.
1 / 2 shared
Bras, W.
1 / 13 shared
Nolte, S.
1 / 14 shared
Harries, D.
1 / 1 shared
Langenhorst, F.
1 / 5 shared
Matthäus, G.
1 / 10 shared
Fazio, A.
1 / 3 shared
Waters, L.
1 / 2 shared
De Vries, C.
1 / 3 shared
Costantini, Elisa
1 / 3 shared
Pinto, Ciro
1 / 2 shared
Lombaert, R.
1 / 2 shared
Min, M.
1 / 4 shared
De Vries, B. L.
1 / 1 shared
Decin, L.
1 / 2 shared
Smolders, K.
1 / 3 shared
De Koter, A.
1 / 4 shared
Jager, C.
1 / 2 shared
Andersen, Anja Cetti
2 / 5 shared
Haro-Corzo, S.
1 / 1 shared
Binette, L.
1 / 1 shared
Posch, Th.
1 / 1 shared
Dorschner, J.
1 / 1 shared
Jäger, C.
1 / 6 shared
Chart of publication period
2024
2023
2018
2013
2012
2011
2006
2003

Co-Authors (by relevance)

  • De Groot, F.
  • Psaradaki, I.
  • Trasobares Llorente, Susana
  • Mehdipour, M.
  • Rogantini, D.
  • Waters, L. B. F. M.
  • De Vries, C. P.
  • Zeegers, S. T.
  • Costantini, E.
  • Den Herder, J. W. A.
  • Trasobares, S.
  • Corrales, L.
  • Bras, W.
  • Nolte, S.
  • Harries, D.
  • Langenhorst, F.
  • Matthäus, G.
  • Fazio, A.
  • Waters, L.
  • De Vries, C.
  • Costantini, Elisa
  • Pinto, Ciro
  • Lombaert, R.
  • Min, M.
  • De Vries, B. L.
  • Decin, L.
  • Smolders, K.
  • De Koter, A.
  • Jager, C.
  • Andersen, Anja Cetti
  • Haro-Corzo, S.
  • Binette, L.
  • Posch, Th.
  • Dorschner, J.
  • Jäger, C.
OrganizationsLocationPeople

article

Nanodiamond dust and the energy distribution of quasars

  • Mutschke, H.
  • Andersen, Anja Cetti
  • Haro-Corzo, S.
  • Binette, L.
Abstract

<p>The spectral energy distribution of quasars shows a sharp steepening of the continuum shortward of ≃ 1100 Å. The steepening could be a result of dust absorption. We present a dust extinction model which considers crystalline carbon grains and compare it with SMC-like dust extinction consisting of a mixture of silicate grains with graphite or amorphous carbon grains. We show that the sharp break seen in individual quasar spectra of intermediate redshift ∼1-2 can be reproduced by dust absorption provided the extinction curve consists of nanodiamonds, composed of terrestial cubic diamonds or of diamonds similar to the presolar nanodiamonds found in primitive meteorites.</p>

Topics
  • amorphous
  • Carbon
  • grain