Materials Map

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

  • About
  • Privacy Policy
  • Legal Notice
  • Contact

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.

×

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.

To Graph

1.080 Topics available

To Map

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.

←

Page 1 of 27758

→
←

Page 1 of 0

→
PeopleLocationsStatistics
Naji, M.
  • 2
  • 13
  • 3
  • 2025
Motta, Antonella
  • 8
  • 52
  • 159
  • 2025
Aletan, Dirar
  • 1
  • 1
  • 0
  • 2025
Mohamed, Tarek
  • 1
  • 7
  • 2
  • 2025
Ertürk, Emre
  • 2
  • 3
  • 0
  • 2025
Taccardi, Nicola
  • 9
  • 81
  • 75
  • 2025
Kononenko, Denys
  • 1
  • 8
  • 2
  • 2025
Petrov, R. H.Madrid
  • 46
  • 125
  • 1k
  • 2025
Alshaaer, MazenBrussels
  • 17
  • 31
  • 172
  • 2025
Bih, L.
  • 15
  • 44
  • 145
  • 2025
Casati, R.
  • 31
  • 86
  • 661
  • 2025
Muller, Hermance
  • 1
  • 11
  • 0
  • 2025
Kočí, JanPrague
  • 28
  • 34
  • 209
  • 2025
Šuljagić, Marija
  • 10
  • 33
  • 43
  • 2025
Kalteremidou, Kalliopi-ArtemiBrussels
  • 14
  • 22
  • 158
  • 2025
Azam, Siraj
  • 1
  • 3
  • 2
  • 2025
Ospanova, Alyiya
  • 1
  • 6
  • 0
  • 2025
Blanpain, Bart
  • 568
  • 653
  • 13k
  • 2025
Ali, M. A.
  • 7
  • 75
  • 187
  • 2025
Popa, V.
  • 5
  • 12
  • 45
  • 2025
Rančić, M.
  • 2
  • 13
  • 0
  • 2025
Ollier, Nadège
  • 28
  • 75
  • 239
  • 2025
Azevedo, Nuno Monteiro
  • 4
  • 8
  • 25
  • 2025
Landes, Michael
  • 1
  • 9
  • 2
  • 2025
Rignanese, Gian-Marco
  • 15
  • 98
  • 805
  • 2025

Gordon, Karl

  • Google
  • 8
  • 79
  • 166

in Cooperation with on an Cooperation-Score of 37%

Topics

Publications (8/8 displayed)

  • 2024JWST Calibration Pipelinecitations
  • 2009Dust Around Red Supergiants in the Magellanic Cloudscitations
  • 2006Spitzer MIPS Infrared Imaging of M31: Further Evidence for a Spiral-Ring Composite Structure166citations
  • 2006Modelling Evolved Stars Detected by the Spitzer LMC Survey (SAGE)citations
  • 2003The Exciting Wavelength of Extended Red Emissioncitations
  • 2003Spectropolarimetric study of circumstellar dust around AGB stars and proto-planetary nebulae.citations
  • 2003Search for Blue Photoluminescence by Interstellar Dustcitations
  • 2000Interpretation of Extragalactic Extinction Measurements Using the Maximum Entropy Methodcitations

Places of action

Chart of shared publication
Freeman, W.
1 / 4 shared
Silva, D.
1 / 9 shared
Levesque, E.
1 / 4 shared
Massey, P.
1 / 3 shared
Olsen, K.
1 / 4 shared
Plez, B.
1 / 4 shared
Nordhaus, J.
1 / 6 shared
Clayton, G.
1 / 5 shared
Chatelain, J.
1 / 4 shared
Bright, Stacey N.
1 / 4 shared
Young, E. T.
1 / 1 shared
Engelbracht, C. W.
1 / 3 shared
Gibson, B. K.
1 / 1 shared
Rieke, G. H.
1 / 4 shared
Barmby, P.
1 / 1 shared
Misselt, K. A.
3 / 5 shared
Levine, D. A.
1 / 1 shared
Marleau, F. R.
1 / 1 shared
Hinz, J.
1 / 3 shared
Bailin, J.
1 / 1 shared
Krause, O.
1 / 2 shared
Latter, W. B.
1 / 2 shared
Hines, D. C.
1 / 1 shared
Werner, M. W.
1 / 2 shared
Ashby, M. L. N.
1 / 3 shared
Thilker, D. A.
1 / 1 shared
Noriega-Crespo, A.
1 / 1 shared
Stolovy, S.
1 / 1 shared
Hora, Joseph
1 / 1 shared
Indebetouw, R.
1 / 5 shared
Meade, M.
1 / 2 shared
Blum, R. D.
1 / 1 shared
Whitney, B.
1 / 2 shared
Vijh, U.
1 / 2 shared
Markwick-Kemper, F.
1 / 1 shared
Misselt, K.
1 / 3 shared
Block, M.
1 / 3 shared
For, B.
1 / 2 shared
Engelbracht, C.
1 / 3 shared
Volk, Kevin
1 / 1 shared
Srinivasan, Sundar
1 / 4 shared
Meixner, Margaret
1 / 12 shared
Team, Sage
1 / 1 shared
Leitherer, C.
1 / 3 shared
Babler, B.
1 / 4 shared
Schmidt, G. D.
1 / 1 shared
Bieging, J. H.
1 / 1 shared
Oppenheimer, B. D.
1 / 1 shared
Witt, Adolf
1 / 1 shared
Vijh, Uma
1 / 1 shared
Clayton, G. C.
1 / 3 shared
Wolff, M. J.
1 / 2 shared
Chart of publication period
2024
2009
2006
2003
2000

Co-Authors (by relevance)

  • Freeman, W.
  • Silva, D.
  • Levesque, E.
  • Massey, P.
  • Olsen, K.
  • Plez, B.
  • Nordhaus, J.
  • Clayton, G.
  • Chatelain, J.
  • Bright, Stacey N.
  • Young, E. T.
  • Engelbracht, C. W.
  • Gibson, B. K.
  • Rieke, G. H.
  • Barmby, P.
  • Misselt, K. A.
  • Levine, D. A.
  • Marleau, F. R.
  • Hinz, J.
  • Bailin, J.
  • Krause, O.
  • Latter, W. B.
  • Hines, D. C.
  • Werner, M. W.
  • Ashby, M. L. N.
  • Thilker, D. A.
  • Noriega-Crespo, A.
  • Stolovy, S.
  • Hora, Joseph
  • Indebetouw, R.
  • Meade, M.
  • Blum, R. D.
  • Whitney, B.
  • Vijh, U.
  • Markwick-Kemper, F.
  • Misselt, K.
  • Block, M.
  • For, B.
  • Engelbracht, C.
  • Volk, Kevin
  • Srinivasan, Sundar
  • Meixner, Margaret
  • Team, Sage
  • Leitherer, C.
  • Babler, B.
  • Schmidt, G. D.
  • Bieging, J. H.
  • Oppenheimer, B. D.
  • Witt, Adolf
  • Vijh, Uma
  • Clayton, G. C.
  • Wolff, M. J.
OrganizationsLocationPeople

article

Interpretation of Extragalactic Extinction Measurements Using the Maximum Entropy Method

  • Clayton, G. C.
  • Wolff, M. J.
  • Misselt, K. A.
  • Gordon, Karl
Abstract

We present size distributions of interstellar dust grains derived from several sightlines in the Small and Large Magellanic Clouds. Employing the Maximum Entropy Method algorithm, as developed by Kim and collaborators, we fit interstellar extinction measurements which span the wavelength range 0.125-3 micron. In order to facilitate comparison, our sample includes several Galactic sightlines whose extinction curves share some similarities with the extragalactic targets. Our work has greatly benefited from recent reanalyses of IUE observations. The grain models employed for this presentation are the simplistic homogeneous spheres models (i.e., Mathis, Rumpl, & Nordsieck 1977) with two (graphite, silicate) or three (graphite, silicate, amorphous carbon) components. Though such usage is only a first step, the results do provide interesting insight into the use of grain size as a diagnostic of extragalactic environment.

Topics
  • impedance spectroscopy
  • amorphous
  • Carbon
  • grain
  • grain size