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

Wright, Edward L.

  • Google
  • 2
  • 33
  • 165

in Cooperation with on an Cooperation-Score of 37%

Topics

Publications (2/2 displayed)

  • 2016The AllWISE Motion Survey, Part 295citations
  • 2010Infrared Luminosities and Aromatic Features in the 24 μm Flux-limited Sample of 5MUSES70citations

Places of action

Chart of shared publication
Logsdon, Sarah E.
1 / 1 shared
Kirkpatrick, J. Davy
1 / 1 shared
Martin, Emily C.
1 / 1 shared
Sheppard, Scott S.
1 / 1 shared
Lansbury, George B.
1 / 1 shared
Fajardo-Acosta, Sergio
1 / 1 shared
Faherty, Jacqueline K.
1 / 1 shared
Cushing, Michael C.
1 / 1 shared
Kellogg, Kendra
1 / 1 shared
Schneider, Adam C.
1 / 1 shared
Gelino, Christopher R.
1 / 1 shared
Stern, Daniel
1 / 4 shared
Greco, Jennifer
1 / 1 shared
Mace, Gregory N.
1 / 1 shared
Eisenhardt, Peter R. M.
1 / 1 shared
Cutri, Roc M.
1 / 1 shared
Conrow, Tim
1 / 1 shared
Mclean, Ian S.
1 / 1 shared
Schurr, Steven D.
1 / 1 shared
Dasyra, Kalliopi
1 / 1 shared
Shi, Yong
1 / 1 shared
Draine, Bruce
1 / 2 shared
Smith, J. D.
1 / 6 shared
Papovich, Casey
1 / 5 shared
Cormier, Diane
1 / 2 shared
Fadda, Dario
1 / 2 shared
Rahman, Nurur
1 / 1 shared
Stierwalt, Sabrina
1 / 1 shared
Lagache, G.
1 / 4 shared
Armus, Lee
1 / 6 shared
Dale, Daniel A.
1 / 5 shared
Helou, George
1 / 1 shared
Wu, Yanling
1 / 1 shared
Chart of publication period
2016
2010

Co-Authors (by relevance)

  • Logsdon, Sarah E.
  • Kirkpatrick, J. Davy
  • Martin, Emily C.
  • Sheppard, Scott S.
  • Lansbury, George B.
  • Fajardo-Acosta, Sergio
  • Faherty, Jacqueline K.
  • Cushing, Michael C.
  • Kellogg, Kendra
  • Schneider, Adam C.
  • Gelino, Christopher R.
  • Stern, Daniel
  • Greco, Jennifer
  • Mace, Gregory N.
  • Eisenhardt, Peter R. M.
  • Cutri, Roc M.
  • Conrow, Tim
  • Mclean, Ian S.
  • Schurr, Steven D.
  • Dasyra, Kalliopi
  • Shi, Yong
  • Draine, Bruce
  • Smith, J. D.
  • Papovich, Casey
  • Cormier, Diane
  • Fadda, Dario
  • Rahman, Nurur
  • Stierwalt, Sabrina
  • Lagache, G.
  • Armus, Lee
  • Dale, Daniel A.
  • Helou, George
  • Wu, Yanling
OrganizationsLocationPeople

article

The AllWISE Motion Survey, Part 2

  • Logsdon, Sarah E.
  • Kirkpatrick, J. Davy
  • Martin, Emily C.
  • Sheppard, Scott S.
  • Lansbury, George B.
  • Fajardo-Acosta, Sergio
  • Faherty, Jacqueline K.
  • Cushing, Michael C.
  • Kellogg, Kendra
  • Schneider, Adam C.
  • Gelino, Christopher R.
  • Stern, Daniel
  • Wright, Edward L.
  • Greco, Jennifer
  • Mace, Gregory N.
  • Eisenhardt, Peter R. M.
  • Cutri, Roc M.
  • Conrow, Tim
  • Mclean, Ian S.
  • Schurr, Steven D.
Abstract

We use the AllWISE Data Release to continue our search for Wide-field Infrared Survey Explorer (WISE)-detected motions. In this paper, we publish another 27,846 motion objects, bringing the total number to 48,000 when objects found during our original AllWISE motion survey are included. We use this list, along with the lists of confirmed WISE-based motion objects from the recent papers by Luhman and by Schneider et al., and candidate motion objects from the recent paper by Gagné et al., to search for widely separated, common-proper-motion systems. We identify 1039 such candidate systems. All 48,000 objects are further analyzed using color-color and color-mag plots to provide possible characterizations prior to spectroscopic follow-up. We present spectra of 172 of these, supplemented with new spectra of 23 comparison objects from the literature, and provide classifications and physical interpretations of interesting sources. Highlights include: (1) the identification of three G/K dwarfs that can be used as standard candles to study clumpiness and grain size in nearby molecular clouds because these objects are currently moving behind the clouds, (2) the confirmation/discovery of several M, L, and T dwarfs and one white dwarf whose spectrophotometric distance estimates place them 5-20 pc from the Sun, (3) the suggestion that the Na I “D” line be used as a diagnostic tool for interpreting and classifying metal-poor late-M and L dwarfs, (4) the recognition of a triple system including a carbon dwarf and late-M subdwarf, for which model fits of the late-M subdwarf (giving [Fe/H] ≈ -1.0) provide a measured metallicity for the carbon star, and (5) a possible 24 pc distant K5 dwarf + peculiar red L5 system with an apparent physical separation of 0.1 pc....

Topics
  • Carbon
  • grain
  • grain size