scholarly journals Galaxy sizes as a function of environment at intermediate redshift from the ESO Distant Cluster Survey

2015 ◽  
Vol 450 (2) ◽  
pp. 1246-1255 ◽  
Author(s):  
Kshitija Kelkar ◽  
Alfonso Aragón-Salamanca ◽  
Meghan E. Gray ◽  
David Maltby ◽  
Benedetta Vulcani ◽  
...  
2002 ◽  
Vol 579 (1) ◽  
pp. 93-126 ◽  
Author(s):  
Marc Postman ◽  
Tod R. Lauer ◽  
William Oegerle ◽  
Megan Donahue

2008 ◽  
Vol 482 (2) ◽  
pp. 419-449 ◽  
Author(s):  
B. Milvang-Jensen ◽  
S. Noll ◽  
C. Halliday ◽  
B. M. Poggianti ◽  
P. Jablonka ◽  
...  

2006 ◽  
Vol 451 (2) ◽  
pp. 395-408 ◽  
Author(s):  
D. Clowe ◽  
P. Schneider ◽  
A. Aragón-Salamanca ◽  
M. Bremer ◽  
G. De Lucia ◽  
...  

2002 ◽  
Vol 571 (1) ◽  
pp. 129-135 ◽  
Author(s):  
Anthony H. Gonzalez ◽  
Dennis Zaritsky ◽  
Risa H. Wechsler

2006 ◽  
Vol 2 (S235) ◽  
pp. 201-201
Author(s):  
Stephanie M. Gogarten ◽  
Julianne J. Dalcanton ◽  
Luc Simard ◽  
Gregory Rudnick ◽  
Vandana Desai ◽  
...  

AbstractWe present the size-luminosity relation (SLR) for disk galaxies observed in eight clusters from the ESO Distant Cluster Survey (EDisCS). These clusters, at redshifts 0.4 < z < 0.8, were observed with the Hubble Space Telescope's Advanced Camera for Surveys. While we observe a change in the SLR with redshift, namely that there is an absence of low surface brightness galaxies at high redshift, we demonstrate that this could be a product of selection effects and thus is not a confirmation of evolution. We also compare the SLR for cluster and field galaxies in each redshift bin and see no significant effects of environment on the SLR.


2004 ◽  
Vol 2004 (IAUS225) ◽  
pp. 173-178
Author(s):  
Douglas Clowe ◽  
Peter Schneider ◽  
the EDisCS Consortium

2008 ◽  
Vol 387 (3) ◽  
pp. 1253-1263 ◽  
Author(s):  
I. M. Whiley ◽  
A. Aragón-Salamanca ◽  
G. De Lucia ◽  
A. von der Linden ◽  
S. P. Bamford ◽  
...  

2010 ◽  
Vol 721 (1) ◽  
pp. L19-L23 ◽  
Author(s):  
T. Valentinuzzi ◽  
B. M. Poggianti ◽  
R. P. Saglia ◽  
A. Aragón-Salamanca ◽  
L. Simard ◽  
...  

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