Differences

This shows you the differences between two versions of the page.

--- lensing [2013/09/04 17:42] – marra
+++ lensing [2013/09/04 17:45] – marra
@@ Line 1: / Line 1: @@
-{{ :lensing.png?350|}}
+{{ :lensing.png?400|}}
 Distance measurements - for instance coming from supernova observations - are affected by the large-scale structure of the universe through lensing.
 The ITP Cosmology group is studying the [[http://arxiv.org/abs/1304.7689|lensing probability distribution function]] of standard candles such as supernovae, gamma ray bursts, etc.
-In particular, lensing is studied by means of [[http://www.turbogl.org|turboGL]] code.
+In particular, lensing is studied by means of the publicly available [[http://www.turbogl.org|turboGL]] code.
-From one side the results of this program will help dealing with the systematic effects of lensing, usually seen as noise. From the other side, the finding of the Cosmology group will allow to quantify how lensing depends on clustering and thanks to the very large datasets available in the future it will possible to place competitive [[http://arxiv.org/abs/1307.1155|constraints]] on matter clustering and so on the nature of dark energy.
+From one side the results of this program will help dealing with the systematic effects of lensing, usually seen as noise. From the other side, the finding of the Cosmology group will allow to quantify how lensing depends on clustering and thanks to the very large datasets available in the future it will be possible to place competitive [[http://arxiv.org/abs/1307.1155|constraints]] on matter clustering and so on the nature of dark energy.

Cosmology Group

Differences