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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Naji, M.
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Ord, Stephen

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in Cooperation with on an Cooperation-Score of 37%

Topics

Publications (24/24 displayed)

  • 2023The Southern-sky MWA Rapid Two-metre (SMART) pulsar survey—I. Survey design and processing pipeline16citations
  • 2023The Southern-sky MWA Rapid Two-metre (SMART) pulsar survey—II. Survey status, pulsar census, and first pulsar discoveries14citations
  • 2019ASKAP Science Data Processor software - ASKAPsoft Version 0.22.0citations
  • 2019ASKAP Science Data Processor software - ASKAPsoft Version 0.23.3citations
  • 2019ASKAP Science Data Processor software - ASKAPsoft Version 0.22.2citations
  • 2019ASKAP Science Data Processor software - ASKAPsoft Version 0.23.1citations
  • 2019ASKAP Science Data Processor software - ASKAPsoft Version 0.23.0citations
  • 2019ASKAP Science Data Processor software - ASKAPsoft Version 0.23.2citations
  • 2018ASKAP Science Data Processor software - ASKAPsoft Version 0.19.6citations
  • 2018ASKAP Science Data Processor software - ASKAPsoft Version 0.20.1citations
  • 2018ASKAP Science Data Processor software - ASKAPsoft Version 0.20.0citations
  • 2018ASKAP Science Data Processor software - ASKAPsoft Version 0.20.3citations
  • 2018ASKAP Science Data Processor software - ASKAPsoft Version 0.21.0citations
  • 2018ASKAP Science Data Processor software - ASKAPsoft Version 0.20.2citations
  • 2017ASKAP Science Data Processor software - ASKAPsoft Version 0.19.2citations
  • 2017ASKAP Science Data Processor software - ASKAPsoft Version 0.19.0citations
  • 2017ASKAP Science Data Processor software - ASKAPsoft Version 0.18.2citations
  • 2017ASKAP Science Data Processor software - ASKAPsoft Version 0.18.0citations
  • 2017ASKAP Science Data Processor software - ASKAPsoft Version 0.19.5citations
  • 2017ASKAP Science Data Processor software - ASKAPsoft Version 0.19.3citations
  • 2017ASKAP Science Data Processor software - ASKAPsoft Version 0.17.0citations
  • 2017ASKAP Science Data Processor software - ASKAPsoft Version 0.18.1citations
  • 2017ASKAP Science Data Processor software - ASKAPsoft Version 0.18.3citations
  • 2017ASKAP Science Data Processor software - ASKAPsoft Version 0.19.4citations

Places of action

Chart of shared publication
Tremblay, S. E.
2 / 2 shared
Straten, W. Van
2 / 2 shared
Smith, K. R.
2 / 2 shared
Kudale, Sanjay
2 / 2 shared
Swainston, Nicholas
2 / 2 shared
Mcsweeney, S. J.
2 / 2 shared
Bhat, Ramesh
2 / 3 shared
Williams, A.
2 / 15 shared
Walker, M.
2 / 7 shared
Meyers, B. W.
2 / 2 shared
Kaplan, D. L.
2 / 19 shared
Johnston-Hollitt, M.
2 / 2 shared
Tocknell, J.
2 / 2 shared
Lange, R.
2 / 2 shared
Dai, S.
2 / 3 shared
Mitchell, Daniel
22 / 24 shared
Bastholm, Eric
22 / 22 shared
Lenc, Emil
22 / 23 shared
Van Diepen, Ger
22 / 22 shared
Whiting, Matthew
22 / 23 shared
Khoo, Jonathan
22 / 22 shared
Collins, Daniel
22 / 22 shared
Wu, Xinyu
22 / 22 shared
Marquarding, Malte
22 / 22 shared
Bannister, Keith
22 / 22 shared
Lahur, Paulus
22 / 22 shared
Maher, Tony
22 / 22 shared
Voronkov, Max
22 / 22 shared
Guzman, Juan
22 / 22 shared
Chart of publication period
2023
2019
2018
2017

Co-Authors (by relevance)

  • Tremblay, S. E.
  • Straten, W. Van
  • Smith, K. R.
  • Kudale, Sanjay
  • Swainston, Nicholas
  • Mcsweeney, S. J.
  • Bhat, Ramesh
  • Williams, A.
  • Walker, M.
  • Meyers, B. W.
  • Kaplan, D. L.
  • Johnston-Hollitt, M.
  • Tocknell, J.
  • Lange, R.
  • Dai, S.
  • Mitchell, Daniel
  • Bastholm, Eric
  • Lenc, Emil
  • Van Diepen, Ger
  • Whiting, Matthew
  • Khoo, Jonathan
  • Collins, Daniel
  • Wu, Xinyu
  • Marquarding, Malte
  • Bannister, Keith
  • Lahur, Paulus
  • Maher, Tony
  • Voronkov, Max
  • Guzman, Juan
OrganizationsLocationPeople

document

ASKAP Science Data Processor software - ASKAPsoft Version 0.20.0

  • Mitchell, Daniel
  • Bastholm, Eric
  • Ord, Stephen
  • Lenc, Emil
  • Van Diepen, Ger
  • Whiting, Matthew
  • Khoo, Jonathan
  • Collins, Daniel
  • Wu, Xinyu
  • Marquarding, Malte
  • Bannister, Keith
  • Lahur, Paulus
  • Maher, Tony
  • Voronkov, Max
  • Guzman, Juan
Abstract

ASKAPsoft, the ASKAP Science Data Processor, provides data processing functionality, including:* Calibration * Spectral line imaging * Continuum imaging * Source detection and generation of source catalogs * Transient detectionASKAPsoft is developed as a part of the CSIRO Australian Square Kilometre Array Pathfinder (ASKAP) Science Data Processor component. ASKAPsoft is a key component in the ASKAP system. It is the primary software for storing and processing raw data, and initiating the archiving of resulting science data products into the data archive (CASDA).The processing pipelines within ASKAPsoft are largely written in C++ built on top of casacore and other third party libraries. The software is designed to be parallelised, where possible, for performance.ASKAPsoft is designed to be built and executed in a standard Unix/Linux environment and core dependencies must be fulfilled by the platform. These include, but are not limited to, a C/C++/Fortran compiler, Make, Python 2.7, Java 7 and MPI. More specific dependencies are downloaded by the ASKAPsoft build system and are installed within the ASKAPsoft development tree. Specific to the Debian platform, after a standard installation of Debian Wheezy (7.x) the following packages will need to be installed with apt-get:* g++ * gfortran * openjdk-7-jdk * python-dev * flex * bison * openmpi-bin * libopenmpi-dev * libfreetype6-dev * libpng12-devMore information regarding the building, installation and running of the software can be found in the README file in the root of the file structure that forms this collection.Source code can be accessed via the links in Related Materials section.----- Pipelines: * Corrected the use of the $ACES environment variable when running thecontinuum validation script, so that pecularities of the localenvironment are appropriately dealt with. * Some corrections in pipeline scripts regarding FITS mode processing:- Ensures the continuum linmos image is copied at the field-levelmosaicking job.- Ensures the spectral-line selavy job uses the correct fileextensions.- Ensures the imcontsub job converts the contsub cube to fits at theend if we are working in FITS mode.- Updates the naming of the contsub cube to ensure consistency(removing .fits from the middle of it).* Improve copying of spectral weights images when running linmos to avoidambiguities and prevent unnecessary files. * Added a parameter, DO_SOURCE_FINDING_FIELD_MOSAICS, to turn off sourcefinding for individual fields and rely on the source finding for thefinal mosaic instead. This prevents unnecessary source finding jobsbeing launched. * Selavy source finding jobs now have scheduling block ID (SBID) passedin parsets. * The casdaupload utility can now handle cubelets (as well as spectra& moment-maps). These are included by the casda script in thepipeline.* TIME selection options in flagging are now exposed in pipelinescripts via TIME_FLAG_SCIENCE, TIME_FLAG_SCIENCE_AV andTIME_FLAG_1934. It is up to the user to provide suitable values.* Pipelines allow processing of scheduling blocks (SB) where the numberof measurement sets (MS) is different to the number of beams. Thisaddresses an issue where the SB have recorded 36 MSs but only asubset of them are valid. * The use of dcp for copying MSs from the archive is turned off bydefault to minimise the load on the hpc-data nodes (the method fordoing this is not ideal).Processing Software: * Modifications to Selavy to include additional information in theheaders of the spectra & related images (Object name, date-obsand duration, Project ID and SBID, history comments). * Fixed a problem where mslist output was corrupted by long fieldnames. * Shortened objectID strings are now used in catalogues. No longeruses image name, but instead SBID + catalogue/data product type +sequence ID.

Topics
  • impedance spectroscopy
  • mass spectrometry
  • atom probe tomography