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)

  • 2019DSA-10: a prototype array for localizing fast radio bursts57citations

Places of action

Chart of shared publication
Woody, D.
1 / 1 shared
Daddario, L.
1 / 1 shared
Shi, Jun
1 / 2 shared
Catha, M.
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Kulkarni, S.
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Hallinan, Gregg
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Ravi, V.
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Vedantham, Harish
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Chart of publication period
2019

Co-Authors (by relevance)

  • Woody, D.
  • Daddario, L.
  • Shi, Jun
  • Catha, M.
  • Kulkarni, S.
  • Hallinan, Gregg
  • Ravi, V.
  • Vedantham, Harish
  • Weinreb, S.
  • Hobbs, R.
OrganizationsLocationPeople

article

DSA-10: a prototype array for localizing fast radio bursts

  • Woody, D.
  • Daddario, L.
  • Shi, Jun
  • Catha, M.
  • Kulkarni, S.
  • Kocz, J.
  • Hallinan, Gregg
  • Ravi, V.
  • Vedantham, Harish
  • Weinreb, S.
  • Hobbs, R.
Abstract

<jats:title>ABSTRACT</jats:title><jats:p>The Deep Synoptic Array 10-dish prototype (DSA-10) is an instrument designed to detect and localize fast radio bursts with arcsecond accuracy in real time. Deployed at Owens Valley Radio Observatory, it consists of ten 4.5-m diameter dishes, equipped with a 250-MHz bandwidth dual polarization receiver, centred at 1.4 GHz. The 20 input signals are digitized and field programmable gate arrays are used to transform the data to the frequency domain and transmit it over ethernet. A series of computer servers buffer both raw data samples and perform a real time search for fast radio bursts on the incoherent sum of all inputs. If a pulse is detected, the raw data surrounding the pulse are written to disc for coherent processing and imaging. The prototype system was operational from 2017 June to 2018 February conducting a drift scan search. Giant pulses from the Crab Pulsar were used to test the detection and imaging pipelines. The 10-dish prototype system was brought online again in 2019 March, and will gradually be replaced with the new DSA-110, a 110-dish system, over the next 2 yr to improve sensitivity and localization accuracy.</jats:p>

Topics
  • impedance spectroscopy