Difference between revisions of "NOvA Experiment"

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[[Image:NOvA_Picture_of_May1_2019.png | 300 px]]
 
[[Image:NOvA_Picture_of_May1_2019.png | 300 px]]
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'''May-2019''' ROC-Dubna excursion by [[Alexander Antoshkin at NOvA|Alexander Antoshkin]]
 
'''May-2019''' ROC-Dubna excursion by [[Alexander Antoshkin at NOvA|Alexander Antoshkin]]
  
 
[[Image:NOvA_Picture_of_May2_2019.png | 300 px]]
 
[[Image:NOvA_Picture_of_May2_2019.png | 300 px]]
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'''May-2019''' Results presented at AYSS-2019 conference by [[Anastasia Kalitkina at NOvA|Anastasia Kalitkina]]
 
'''May-2019''' Results presented at AYSS-2019 conference by [[Anastasia Kalitkina at NOvA|Anastasia Kalitkina]]
  
 
[[Image:NOvA_Picture_of_June_2019.png | 300 px]]
 
[[Image:NOvA_Picture_of_June_2019.png | 300 px]]
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'''June-2019''' Efficiency vs. SN distance for various methods of detectors combination. Percents show the fraction of SN candidates in our galaxy, covered by the combined trigger.
 
'''June-2019''' Efficiency vs. SN distance for various methods of detectors combination. Percents show the fraction of SN candidates in our galaxy, covered by the combined trigger.
 
Last combination method - "Comb" is the best way to do it, where we set a weight to each detector, proportional to their sensitivity to SN signal. The picture by [[Andrey Sheshukov at NOvA|Andrey Sheshukov]]
 
Last combination method - "Comb" is the best way to do it, where we set a weight to each detector, proportional to their sensitivity to SN signal. The picture by [[Andrey Sheshukov at NOvA|Andrey Sheshukov]]
  
 
[[Image:NOvA_Picture_of_July_2019.png | 300 px]]
 
[[Image:NOvA_Picture_of_July_2019.png | 300 px]]
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'''July-2019''' SN Betelgeuse neutrino signal simulation based on SND data . The picture by [[Maria Petropavlova at NOvA|Maria Petropavlova]]
 
'''July-2019''' SN Betelgeuse neutrino signal simulation based on SND data . The picture by [[Maria Petropavlova at NOvA|Maria Petropavlova]]
  

Revision as of 10:46, 14 August 2019

NOvA In short
NOvA Graphic 14-0241-01.jpeg
Picture of the month Archive

NOvA Picture of May1 2019.png

May-2019 ROC-Dubna excursion by Alexander Antoshkin

NOvA Picture of May2 2019.png

May-2019 Results presented at AYSS-2019 conference by Anastasia Kalitkina

NOvA Picture of June 2019.png

June-2019 Efficiency vs. SN distance for various methods of detectors combination. Percents show the fraction of SN candidates in our galaxy, covered by the combined trigger. Last combination method - "Comb" is the best way to do it, where we set a weight to each detector, proportional to their sensitivity to SN signal. The picture by Andrey Sheshukov

NOvA Picture of July 2019.png

July-2019 SN Betelgeuse neutrino signal simulation based on SND data . The picture by Maria Petropavlova


OlegSamoylov (talk) 01:04, 1 October 2018 (MSK)