Difference between revisions of "Olga Petrova at NOvA"

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|| [[Image:Olga Petrova FD.png | 200px]]  ||
 
|| [[Image:Olga Petrova FD.png | 200px]]  ||
  
'''Position''' : PhD student
+
'''Position''' : staff
 
* joined to NOvA at 2013, collaborator since Feb. 2015
 
* joined to NOvA at 2013, collaborator since Feb. 2015
  
 
'''Working time''' :
 
'''Working time''' :
* 70% FTE (including all activities)
+
* 75% FTE (including all activities)
 
* 100% ExFTE (including just experimental activities)
 
* 100% ExFTE (including just experimental activities)
  
'''Main group activity''' : Analysis exotics
+
'''Main group activity''' : Exotics analysis
  
  
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'''Tasks description'''
 
'''Tasks description'''
  
Please, describe your current work and work done.
+
* East-West Cosmic ray asymmetry in Far Detector.
 +
* QECC cross sections with approach of running axial mass of nucleon.

Revision as of 19:01, 31 March 2016

Olga Petrova FD.png

Position : staff

  • joined to NOvA at 2013, collaborator since Feb. 2015

Working time :

  • 75% FTE (including all activities)
  • 100% ExFTE (including just experimental activities)

Main group activity : Exotics analysis


Tasks description

  • East-West Cosmic ray asymmetry in Far Detector.
  • QECC cross sections with approach of running axial mass of nucleon.