Differences

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

Link to this comparison view

Both sides previous revision Previous revision
Next revision
Previous revision
Last revision Both sides next revision
references [2014/01/15 18:19]
admin
references [2014/01/18 13:53]
admin [New SALT trainings]
Line 1: Line 1:
 ====== References ====== ====== References ======
-  ​* Betoule et al. (2014), //Improved cosmological constraints from a joint analysis of the SDSS-II and SNLS supernova samples// +===== New SALT trainings ===== 
-  * Mosher et al. (2014), //​Cosmological Parameter Uncertainties from SALT-II Type Ia Supernova Light Curve Models//+  ​[[http://​arxiv.org/​abs/​1401.4064|Betoule et al. (2014)]], //Improved cosmological constraints from a joint analysis of the SDSS-II and SNLS supernova samples//
   * [[http://​adsabs.harvard.edu/​abs/​2010A%26A...523A...7G|Guy et al. (2010)]], //The Supernova Legacy Survey 3-year sample: Type Ia supernovae photometric distances and cosmological constraints//​   * [[http://​adsabs.harvard.edu/​abs/​2010A%26A...523A...7G|Guy et al. (2010)]], //The Supernova Legacy Survey 3-year sample: Type Ia supernovae photometric distances and cosmological constraints//​
   * [[http://​adsabs.harvard.edu/​abs/​2007A%26A...466...11G|Guy et al. (2007)]], //SALT2: using distant supernovae to improve the use of Type Ia supernovae as distance indicators//​   * [[http://​adsabs.harvard.edu/​abs/​2007A%26A...466...11G|Guy et al. (2007)]], //SALT2: using distant supernovae to improve the use of Type Ia supernovae as distance indicators//​
   * [[http://​adsabs.harvard.edu/​abs/​2005A%26A...443..781G|Guy et al. (2005)]], //SALT: a spectral adaptive light curve template for type Ia supernovae//​   * [[http://​adsabs.harvard.edu/​abs/​2005A%26A...443..781G|Guy et al. (2005)]], //SALT: a spectral adaptive light curve template for type Ia supernovae//​
  
 +===== SALT tests with simulations ===== 
 +  * Mosher et al. (2014), //​Cosmological Parameter Uncertainties from SALT-II Type Ia Supernova Light Curve Models//