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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in Cooperation with on an Cooperation-Score of 37%

Topics

Publications (3/3 displayed)

  • 2020Design and production of segment mirrors for the Large-Sized Telescopes of the Cherenkov Telescope Array4citations
  • 2015The Optical system for the Large Size Telescope of the Cherenkov Telescope Arraycitations
  • 2008Oxygen line mapping of SN 1006 with Suzaku3citations

Places of action

Chart of shared publication
Yamamoto, Tokonatsu
1 / 1 shared
Yoshida, Tatsuo
1 / 1 shared
Teshima, Masahiro
1 / 1 shared
Saito, Takayuki
1 / 1 shared
Okumura, Akira
1 / 1 shared
Obara, Koutaro
1 / 1 shared
Mazin, Daniel
1 / 1 shared
Vovk, Ievgen
1 / 1 shared
Kagaya, Mika
1 / 1 shared
Chikawa, Michiyuki
1 / 1 shared
Noda, Koji
1 / 2 shared
Fukami, Satoshi
1 / 1 shared
Inada, Tomohiro
1 / 1 shared
Jablonski, C.
1 / 2 shared
Horns, Dieter
1 / 1 shared
Okumura, A.
1 / 1 shared
Yoshida, T.
1 / 3 shared
Kagaya, M.
1 / 2 shared
Ogino, M.
1 / 2 shared
Fukami, S.
1 / 3 shared
Wetteskind, H.
1 / 2 shared
Barres De Almeida, U.
1 / 2 shared
Straumann, U.
1 / 3 shared
Vollhardt, A.
1 / 2 shared
Chikawa, M.
1 / 2 shared
Saito, T.
1 / 5 shared
Cho, N.
1 / 2 shared
Hayashida, M.
1 / 2 shared
Stadler, R.
1 / 2 shared
Noda, K.
1 / 2 shared
Steiner, S.
1 / 7 shared
Teshima, M.
1 / 2 shared
Yamamoto, T.
1 / 7 shared
Gadola, A.
1 / 2 shared
Hanabata, Y.
1 / 2 shared
Chart of publication period
2020
2015
2008

Co-Authors (by relevance)

  • Yamamoto, Tokonatsu
  • Yoshida, Tatsuo
  • Teshima, Masahiro
  • Saito, Takayuki
  • Okumura, Akira
  • Obara, Koutaro
  • Mazin, Daniel
  • Vovk, Ievgen
  • Kagaya, Mika
  • Chikawa, Michiyuki
  • Noda, Koji
  • Fukami, Satoshi
  • Inada, Tomohiro
  • Jablonski, C.
  • Horns, Dieter
  • Okumura, A.
  • Yoshida, T.
  • Kagaya, M.
  • Ogino, M.
  • Fukami, S.
  • Wetteskind, H.
  • Barres De Almeida, U.
  • Straumann, U.
  • Vollhardt, A.
  • Chikawa, M.
  • Saito, T.
  • Cho, N.
  • Hayashida, M.
  • Stadler, R.
  • Noda, K.
  • Steiner, S.
  • Teshima, M.
  • Yamamoto, T.
  • Gadola, A.
  • Hanabata, Y.
OrganizationsLocationPeople

article

Oxygen line mapping of SN 1006 with Suzaku

  • Takahashi, Tadayuki
  • Koyama, Katsuji
  • Kitamoto, Shunji
  • Holt, Steve
  • Tsuboi, Yohko
  • Miyata, Emi
  • Tsunemi, Hiroshi
  • Nakajima, Hiroshi
  • Ueno, Masaru
  • Katagiri, Hideaki
  • Kokubun, Motohide
  • Katsuda, Satoru
  • Petre, Rob
  • Bamba, Aya
  • Hughes, John P.
  • Yamaguchi, Hiroya
  • Hiraga, Junko S.
  • Tomida, Hiroshi
  • Matsumoto, Hironori
  • Tsujimoto, Masahiro
  • Kataoka, Jun
  • Mori, Koji
  • Uchiyama, Yasunobu
  • Ozaki, Masanobu
  • Watanabe, Shin
  • Sekiguchi, Akiko
  • Tanaka, Takaaki
  • Terada, Yukikatsu
Abstract

SN 1006 is one of the supernova remnants (SNRs) with relatively low-temperature electrons, considering the young age of just 1000 years. We carried out SN 1006 mapping observations with the X-ray Imaging Spectrometers (XIS) and the Hard X-ray Detector (HXD) onboard Suzaku, the fifth Japanese X-ray satellite. Thanks to the excellent spectral resolution of XIS in the soft X-ray band, H-like and He-like oxygen emission lines were clearly detected, and we could make a map of the line intensity, and as well as a flux and the photon index of nonthermal component. We found that these parameters have spatial dependences from region to region in the SNR; the north region is bright in nonthermal, while dim in thermal; the east region is bright in both nonthermal and thermal; the inner region shows dim nonthermal and bright thermal emission. The photon index is the smallest in the north region....

Topics
  • impedance spectroscopy
  • Oxygen