Hostname: page-component-586b7cd67f-r5fsc Total loading time: 0 Render date: 2024-11-25T17:40:19.864Z Has data issue: false hasContentIssue false

Which way to the next frontier? Finding the most powerful cluster lenses

Published online by Cambridge University Press:  27 October 2016

Harald Ebeling
Affiliation:
Institute for Astronomy, University of Hawaii, Honolulu, HI 96822 email: [email protected]
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

While the identification of a worthy topic or challenge is fundamental to the goal of conducting cutting-edge research, another ingredient is indispensable in the field of observational astronomy: the best possible target. Indeed, the ability to choose from a significant number of extremely powerful gravitational lenses was central to the success of the Frontier Fields project. We here briefly review the surveys that provided this crucial pool of targets, before focusing on the results of ongoing work to identify similarly extreme (if not more extreme) systems at higher redshift for the exploration of a yet more distant extragalactic frontier – with JWST and other, evermore ambitious missions.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2016 

References

Andersson, et al. 2011, ApJ, 738, 48 CrossRefGoogle Scholar
Ebeling, et al. 2001, ApJ, 553, 668 CrossRefGoogle Scholar
Ebeling, et al. 2007, ApJ, 661, L33 CrossRefGoogle Scholar
Ebeling, et al. 2010, MNRAS, 407, 83 CrossRefGoogle Scholar
Mann, & Ebeling, 2012, MNRAS, 420, 2120 CrossRefGoogle Scholar
Ebeling, et al. 2013, MNRAS, 432, 62 CrossRefGoogle Scholar
Kaiser, et al. 2007, AAS, #211, #142.05Google Scholar
Reichardt, et al. 2013, ApJ, 763, 127 CrossRefGoogle Scholar
Planck Collaboration 2013, A&A, 550, 130 Google Scholar
Voges, et al. 1999, A&A, 505, 991 Google Scholar