2010
DOI: 10.3726/978-3-0352-0036-2
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Pratiques imaginées et images des pratiques plurilingues

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Cited by 37 publications
(2 citation statements)
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“…The current large sample of z > 1 clusters comes from X-ray surveys (e.g., Mullis et al 2005;Stanford et al 2006;Bremer et al 2006;Pacaud et al 2007;Henry et al 2010;Fassbender et al 2011a,b;Nastasi et al 2011;Santos et al 2011), spacebased MIR surveys (e.g., Stanford et al 2005;Eisenhardt et al 2008;Muzzin et al 2009;Wilson et al 2009;Papovich et al 2010;Demarco et al 2010;Brodwin et al 2011;Stanford et al 2012;Zeimann et al 2012), ground-based NIR surveys (e.g., Gobat et al 2011;Spitler et al 2012), millimeter SZE surveys (e.g., Brodwin et al 2010;Foley et al 2011;Stalder et al 2012), as well as narrow-band and MIR searches around high-redshift radio galaxies (e.g., Venemans et al 2007;Galametz et al 2010Galametz et al , 2012.…”
Section: Introductionmentioning
confidence: 99%
“…The current large sample of z > 1 clusters comes from X-ray surveys (e.g., Mullis et al 2005;Stanford et al 2006;Bremer et al 2006;Pacaud et al 2007;Henry et al 2010;Fassbender et al 2011a,b;Nastasi et al 2011;Santos et al 2011), spacebased MIR surveys (e.g., Stanford et al 2005;Eisenhardt et al 2008;Muzzin et al 2009;Wilson et al 2009;Papovich et al 2010;Demarco et al 2010;Brodwin et al 2011;Stanford et al 2012;Zeimann et al 2012), ground-based NIR surveys (e.g., Gobat et al 2011;Spitler et al 2012), millimeter SZE surveys (e.g., Brodwin et al 2010;Foley et al 2011;Stalder et al 2012), as well as narrow-band and MIR searches around high-redshift radio galaxies (e.g., Venemans et al 2007;Galametz et al 2010Galametz et al , 2012.…”
Section: Introductionmentioning
confidence: 99%
“…Therefore, the consistency of the cusp energetic hypothesis introduced here should be verified by existing theories as well as by those in development. In this sense, the second part of this article will aim to provide a comprehensive approach that can select the best candidates for describe the energetic cusp (+.-) in a complete cosmological approach pointing out possible observational constraints [11,12].…”
Section: Discussionmentioning
confidence: 99%