Marcocci, S
303  results:
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1

Search for low-energy neutrinos from astrophysical sources ..:

Agostini, M ; Altenmüller, K ; Bravo, D...
info:eu-repo/semantics/altIdentifier/doi/10.1016/j.astropartphys.2020.102509.  , 2021
 
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2

Search for low-energy neutrinos from astrophysical sources ..:

Agostini, M ; Altenmüller, K ; Appel, S...
https://discovery.ucl.ac.uk/id/eprint/10111984/10/Agostini_Search%20for%20low-energy%20neutrinos%20from%20astrophysical%20sources%20with%20Borexino_AAM.pdf.  , 2021
 
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3

Search for low-energy neutrinos from astrophysical sources ..:

Agostini M ; Altenmuller K ; Appel S...
info:eu-repo/semantics/altIdentifier/wos/WOS:000576790400003.  , 2021
 
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4

Comprehensive geoneutrino analysis with Borexino:

Agostini, M ; Altenmüller, K ; Bravo, D...
info:eu-repo/semantics/altIdentifier/doi/10.1103/PhysRevD.101.012009.  , 2020
 
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5

Constraints on flavor-diagonal non-standard neutrino intera..:

Agarwalla, S. K ; Agostini, M ; Bonfini, G...
info:eu-repo/semantics/altIdentifier/wos/WOS:000520506100001.  , 2020
 
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6

Improved measurement of B8 solar neutrinos with 1.5 kt·y of..:

Agostini, M ; Altenmüller, K ; Appel, S...
info:eu-repo/semantics/altIdentifier/wos/WOS:000518459600001.  , 2020
 
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7

Comprehensive geoneutrino analysis with Borexino:

Agostini M ; Altenmuller K ; Appel S...
info:eu-repo/semantics/altIdentifier/wos/WOS:000508453600004.  , 2020
 
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9

Analysis strategies for the updated geoneutrino measurement..:

Kumaran S ; Agostini M ; Altenmuller K...
info:eu-repo/semantics/altIdentifier/wos/WOS:000539995300183.  , 2020
 
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11

Comprehensive geoneutrino analysis with Borexino:

Agostini M ; Altenmuller K ; Appel S...
info:eu-repo/semantics/altIdentifier/wos/WOS:000508453600004.  , 2020
 
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12

Updated geoneutrino measurement with Borexino:

Ludhova L ; Agostini M ; Altenmuller K...
info:eu-repo/semantics/altIdentifier/wos/WOS:000539995300210.  , 2020
 
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15

Comprehensive geoneutrino analysis with Borexino:

Agostini, M ; Altenmüller, K ; Bravo, D...
info:eu-repo/semantics/altIdentifier/doi/10.1103/PhysRevD.101.012009.  , 2020
 
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