Skip to main page content
Access keys NCBI Homepage MyNCBI Homepage Main Content Main Navigation

Search Page

MyNCBI Filters
Results by year

Table representation of search results timeline featuring number of search results per year.

Year Number of Results
2008 2
2010 1
2012 1
2015 1
2016 2
2017 3
2018 1
2020 0
Text availability
Article attribute
Article type
Publication date

Search Results

11 results
Results by year
Filters applied: . Clear all
Page 1
Did you mean carbamate L[au] (1 results)?
An algorithm for the reconstruction of high-energy neutrino-induced particle showers and its application to the ANTARES neutrino telescope
Albert A, et al. Eur Phys J C Part Fields 2017. Among authors: Caramete L. PMID 28775667 Free PMC article.
A [Formula: see text] C.L. upper limit on the diffuse astrophysical neutrino flux with a value per neutrino flavour of [Formula: see text] is set, applicable to the energy range from 23 TeV to 7.8 PeV, assuming an unbroken [Formula: see text] spectrum and neutrino flavour equipartition at Earth....
A [Formula: see text] C.L. upper limit on the diffuse astrophysical neutrino flux with a value per neutrino flavour of [Formula: see …
Upper limit on the diffuse flux of ultrahigh energy tau neutrinos from the Pierre Auger Observatory
Abraham J, et al. Phys Rev Lett 2008. Among authors: Caramete L. PMID 18518595
Assuming an E(nu)(-2) differential energy spectrum the limit set at 90% C.L. is E(nu)(2)dN(nu)(tau)/dE(nu)<1.3 x 10(-7) GeV cm(-2) s(-1) sr(-1) in the energy range 2 x 10(17) eV< E(nu)< 2 x 10(19) eV....
Assuming an E(nu)(-2) differential energy spectrum the limit set at 90% C.L. is E(nu)(2)dN(nu)(tau)/dE(nu)<1.3 x 10(-7) GeV cm(-2) …
11 results
Jump to page
Feedback