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	<title>Centre de Conf&#233;rences Jules Janssen</title>
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		<title>Massive Galaxies from the CARLA survey</title>
		<link>https://centre-janssen.observatoiredeparis.psl.eu/Massive-Galaxies-from-the-CARLA-survey-298</link>
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		<dc:date>2026-04-16T00:00:00Z</dc:date>
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&lt;p&gt;At present, around ten clusters are known at z&gt;1.6. Current surveys are extending our samples of an order of magnitude, and give us insights on galaxy and large-scale structure evolution at the very first epochs of cluster formation. &lt;br class='autobr' /&gt;
Clusters Around Radio-loud AGN program (CARLA ; Galametz et al. 2012 ; Wylezalek et al. 2013) is one of the major surveys of clusters and proto-clusters at high redshift and searches for overdensities around radio-loud AGNs. Twenty of the 200 CARLA cluster (&#8230;)&lt;/p&gt;


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 <content:encoded>&lt;div class='rss_texte'&gt;&lt;p&gt;At present, around ten clusters are known at z&gt;1.6. Current surveys are extending our samples of an order of magnitude, and give us insights on galaxy and large-scale structure evolution at the very first epochs of cluster formation.&lt;/p&gt;
&lt;p&gt;Clusters Around Radio-loud AGN program (CARLA ; Galametz et al. 2012 ; Wylezalek et al. 2013) is one of the major surveys of clusters and proto-clusters at high redshift and searches for overdensities around radio-loud AGNs. Twenty of the 200 CARLA cluster candidates (Wylezalek et al. 2013, 2014), with 1.4 &lt; z &lt; 2.8, have been observed with the HST WFC3 in F140W imaging and G141 grism spectroscopy (PI : Daniel Stern ; Noirot et al. 2016). HST observations permitted us to confirm cluster candidates and obtain galaxy morphology. Galaxy colors are available from combined space and ground-based observations. Recent results from Noirot et al. (2016) have shown that these high redshift overdensities host galaxies with different stellar populations, with some having already formed a red sequence and others showing star-forming galaxies overdensities. We recently had a program accepted at IRAM/NOEMA, in collaboration with F. Combes and P. Salome, and ALMA, we will dedicate the last day to discuss results from these two programs and plan for the future.&lt;/p&gt;
&lt;p&gt;We propose to host a collaboration meeting to discuss recent CARLA results, and prepare follow-up programs with both optical and radio telescopes, with the goal to understand how the first clusters and their galaxies form.&lt;/p&gt;
&lt;p&gt;We will invite members of the Spitzer South Pole Telescope Deep Field (SSDF ; Ashby et al. 2013) collaboration to discuss similarities and differences in two cluster/proto-cluster samples. In fact, the SSDF cluster sample (Rettura et al. 2014) has been selected using similar galaxy colors as CARLA, but most of the candidates do not host a radio loud AGN. A comparison of our findings will permit us to asses selection effects and biases when drawing conclusions about galaxy evolution.&lt;/p&gt;&lt;/div&gt;
		
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