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)

  • 2010Southern Cosmology Survey II: Massive Optically-Selected Clusters from 70 square degrees of the SZE Common Survey Area35citations

Places of action

Chart of shared publication
Infante, Leopoldo
1 / 1 shared
Kosowsky, Arthur
1 / 1 shared
Spergel, David
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Verde, Licia
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Deshpande, Amruta J.
1 / 1 shared
Barrientos, L. Felipe
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Menanteau, Felipe
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Hughes, John P.
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Hilton, Matt
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2010

Co-Authors (by relevance)

  • Infante, Leopoldo
  • Kosowsky, Arthur
  • Spergel, David
  • Verde, Licia
  • Deshpande, Amruta J.
  • Barrientos, L. Felipe
  • Menanteau, Felipe
  • Hughes, John P.
  • Hilton, Matt
OrganizationsLocationPeople

article

Southern Cosmology Survey II: Massive Optically-Selected Clusters from 70 square degrees of the SZE Common Survey Area

  • Infante, Leopoldo
  • Kosowsky, Arthur
  • Spergel, David
  • Verde, Licia
  • Moodley, Kavilan
  • Deshpande, Amruta J.
  • Barrientos, L. Felipe
  • Menanteau, Felipe
  • Hughes, John P.
  • Hilton, Matt
Abstract

We present a catalog of 105 rich and massive ($M>3^{14}M_$) optically-selected clusters of galaxies extracted from 70 square-degrees of public archival griz imaging from the Blanco 4-m telescope acquired over 45 nights between 2005 and 2007. We use the clusters' optically-derived properties to estimate photometric redshifts, optical luminosities, richness, and masses. We complement the optical measurements with archival XMM-Newton and ROSAT X-ray data which provide additional luminosity and mass constraints on a modest fraction of the cluster sample. Two of our clusters show clear evidence for central lensing arcs; one of these has a spectacular large-diameter, nearly-complete Einstein Ring surrounding the brightest cluster galaxy. A strong motivation for this study is to identify the massive clusters that are expected to display prominent signals from the Sunyaev-Zeldovich Effect (SZE) and therefore be detected in the wide-area mm-band surveys being conducted by both the Atacama Cosmology Telescope and the South Pole Telescope. The optical sample presented here will be useful for verifying new SZE cluster candidates from these surveys, for testing the cluster selection function, and for stacking analyzes of the SZE

Topics
  • impedance spectroscopy
  • cluster