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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in Cooperation with on an Cooperation-Score of 37%

Topics

Publications (1/1 displayed)

  • 2004Supernova 2004dj in NGC 2403citations

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Chart of shared publication
Filippenko, A. V.
1 / 5 shared
Li, W.
1 / 48 shared
Chart of publication period
2004

Co-Authors (by relevance)

  • Filippenko, A. V.
  • Li, W.
OrganizationsLocationPeople

article

Supernova 2004dj in NGC 2403

  • Filippenko, A. V.
  • Challis, P.
  • Li, W.
Abstract

A. V. Filippenko and W. Li, University of California, Berkeley; P. Challis, Harvard-Smithsonian Center for Astrophysics; and S. D. Van Dyk, Infrared Processing and Analysis Center, California Institute of Technology, report:"We have examined optical images of SN 2004dj obtained on Aug. 17 UT with the Wide Field Camera of the Advanced Camera for Surveys aboard the Hubble Space Telescope. Although the supernova is very saturated in these images, it is clearly located within the compact star cluster Sandage 96, confirming the suggestion made on IAUC 8385 and justified in detail by Maiz-Apellaniz et al. (http://xxx.lanl.gov/abs/astro-ph/?0408265). The tentative identification of a different progenitor star made by Li et al. (IAUC 8388) was based on the radio position reported on IAUC 8379 by Stockdale et al., which is possibly affected by inclusion of extended radio emission in the host galaxy (observed in the VLA-D configuration at 8.46 GHz)."

Topics
  • impedance spectroscopy
  • cluster
  • inclusion