Difference between revisions of "NOvA Experiment"

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| style="background:#efefef;" | '''Picture of the month''' [[NOvA pictures of the month|Archive]]
 
| style="background:#efefef;" | '''Picture of the month''' [[NOvA pictures of the month|Archive]]
 
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| style="text-align: center;" | [[Image:NOvA_Picture_of_April_2019.png | 300 px]]
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| style="text-align: center;" |  
'''Apr-2019''' GENIE comparison workshop at Liverpool, 8-12 April 2019. The picture by [[Igor Kakorin at NOvA|Igor Kakorin]]
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[[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]]
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[[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]]
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[[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.
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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]]
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[[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]]
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[[User:OlegSamoylov|OlegSamoylov]] ([[User talk:OlegSamoylov|talk]]) 01:04, 1 October 2018 (MSK)
 
[[User:OlegSamoylov|OlegSamoylov]] ([[User talk:OlegSamoylov|talk]]) 01:04, 1 October 2018 (MSK)

Revision as of 10:38, 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)