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arxiv: astro-ph/0401473 · v1 · submitted 2004-01-22 · 🌌 astro-ph

X-Ray Observations of the Most Massive DLS Shear-Selected Galaxy Clusters

John P. Hughes (1) , Ian Dell'Antonio (2) , Joseph Hennawi (3) Vera Margoniner (4) , Sandor Molnar (1) , Dara Norman (5) , David Spergel (3) J. Anthony Tyson (4) , Gillian Wilson (6) , David Wittman (4) ((1) Rutgers University
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(2) Brown University (3) Princeton University (4) Bell Labs Lucent Technologies (5) CTIO/NSF AAPF (6) SIRTF Science Center)
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keywords clustersx-rayclustermassivesampleshear-selectedsurveyarticle
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We report on preliminary results of our X-ray survey of the most massive clusters currently identified from the Deep Lens Survey (DLS). The DLS cluster sample is selected based on weak lensing shear, which makes it possible for the first time to study clusters in a baryon-independent way. In this article we present X-ray properties of a subset of the shear-selected cluster sample.

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