225 citations · 1k across the 19 of their papers we have counts for
19 papers
First Directional Measurement of sub-MeV Solar Neutrinos with Borexino
M. Agostini, K. Altenmüller, S. Appel +94
We report the measurement of sub-MeV solar neutrinos through the use of their associated Cherenkov radiation, performed with the Borexino detector at the Laboratori Nazionali del G…
Correlated and Integrated Directionality for sub-MeV solar neutrinos in Borexino
M. Agostini, K. Altenmüller, S. Appel +94
Liquid scintillator detectors play a central role in the detection of neutrinos from various sources. In particular, it is the only technique used so far for the precision spectros…
Identification of the cosmogenic C background in large volumes of liquid scintillators with Borexino
M. Agostini, K. Altenmüller, S. Appel +93
Cosmogenic radio-nuclei are an important source of background for low-energy neutrino experiments. In Borexino, cosmogenic C decays outnumber solar and CNO neutrino ev…
The Low Polonium Field of Borexino and its significance for the CNO neutrino detection
S. Kumaran, M. Agostini, K. Altenmüller +93
Borexino is a liquid scintillator detector located at the Laboratori Nazionale del Gran Sasso, Italy with the main goal to measure solar neutrinos. The experiment recently provided…
First detection of CNO neutrinos with Borexino
G. Settanta, M. Agostini, K. Altenmüller +93
Neutrinos are elementary particles which are known since many years as fundamental messengers from the interior of the Sun. The Standard Solar Model, which gives a theoretical desc…
Experimental evidence of neutrinos produced in the CNO fusion cycle in the Sun
M. Agostini, K. Altenmüller, S. Appel +93
For most of their existence stars are fueled by the fusion of hydrogen into helium proceeding via two theoretically well understood processes, namely the chain and the CNO cyc…
Sensitivity to neutrinos from the solar CNO cycle in Borexino
M. Agostini, K. Altenmüller, S. Appel +91
Neutrinos emitted in the carbon, nitrogen, oxygen (CNO) fusion cycle in the Sun are a sub-dominant, yet crucial component of solar neutrinos whose flux has not been measured yet. T…
Search for low-energy neutrinos from astrophysical sources with Borexino
M. Agostini, K. Altenmüller, S. Appel +101
We report on searches for neutrinos and antineutrinos from astrophysical sources performed with the Borexino detector at the Laboratori Nazionali del Gran Sasso in Italy. Electron…
Comprehensive geoneutrino analysis with Borexino
M. Agostini, K. Altenmüller, S. Appel +109
This paper presents a geoneutrino measurement using 3262.74 days of data taken with the Borexino detector at LNGS in Italy. By observing $52.6 ^{+9.4}_{-8.6} ({\rm stat}) ^{+2.7}_{…
Constraints on Flavor-Diagonal Non-Standard Neutrino Interactions from Borexino Phase-II
S. K. Agarwalla, M. Agostini, K. Altenmüller +103
The Borexino detector measures solar neutrino fluxes via neutrino-electron elastic scattering. Observed spectra are determined by the solar- survival probability …
Modulations of the Cosmic Muon Signal in Ten Years of Borexino Data
The Borexino Collaboration, M. Agostini, K. Altenmüller +113
We have measured the flux of cosmic muons in the Laboratori Nazionali del Gran Sasso at 3800\,m\,w.e. to be based on ten y…
Speeding up complex multivariate data analysis in Borexino with parallel computing based on Graphics Processing Unit
X. F. Ding, M. Agostini, K. Altenmuller +104
A spectral fitter based on the graphics processor unit (GPU) has been developed for Borexino solar neutrino analysis. It is able to shorten the fitting time to a superior level com…
Improved measurement of B solar neutrinos with 1.5 kt y of Borexino exposure
The Borexino Collaboration, M. Agostini, K. Altenmüller +95
We report on an improved measurement of the B solar neutrino interaction rate with the Borexino experiment at the Laboratori Nazionali del Gran Sasso. Neutrinos are detected vi…
Limiting neutrino magnetic moments with Borexino Phase-II solar neutrino data
M. Agostini, K. Altenmüller, S. Appel +104
A search for the solar neutrino effective magnetic moment has been performed using data from 1291.5 days exposure during the second phase of the Borexino experiment. No significant…
Simultaneous Precision Spectroscopy of , Be, and Solar Neutrinos with Borexino Phase-II
M. Agostini, K. Altenmuller, S. Appel +104
We present the first simultaneous measurement of the interaction rates of , Be, and solar neutrinos performed with a global fit to the Borexino data in an extended en…
A search for low-energy neutrinos correlated with gravitational wave events GW150914, GW151226 and GW170104 with the Borexino detector
M. Agostini, K. Altenmuller, S. Appel +99
We present the results of a low-energy neutrino search using the Borexino detector in coincidence with the gravitational wave (GW) events GW150914, GW151226 and GW170104. We search…
The Monte Carlo simulation of the Borexino detector
M. Agostini, K. Altenmuller, S. Appel +97
We describe the Monte Carlo (MC) simulation package of the Borexino detector and discuss the agreement of its output with data. The Borexino MC 'ab initio' simulates the energy los…
Seasonal Modulation of the Be Solar Neutrino Rate in Borexino
M. Agostini, K. Altenmuller, S. Appel +99
We detected the seasonal modulation of the Be neutrino interaction rate with the Borexino detector at the Laboratori Nazionali del Gran Sasso in Italy. The period, amplitude, a…
A search for low-energy neutrino and antineutrino signals correlated with gamma-ray bursts with Borexino
M. Agostini, K. Altenmeuller, S. Appel +97
A search for neutrino and antineutrino events correlated with 2,350 gamma-ray bursts (GRBs) is performed with Borexino data collected between December 2007 and November 2015. No st…