Calibration of Super-Kamiokande Using an Electron Linac
arXiv:hep-ex/9807027 · doi:10.1016/S0168-9002(98)01200-5
Abstract
In order to calibrate the Super-Kamiokande experiment for solar neutrino measurements, a linear accelerator (LINAC) for electrons was installed at the detector. LINAC data were taken at various positions in the detector volume, tracking the detector response in the variables relevant to solar neutrino analysis. In particular, the absolute energy scale is now known with less than 1 percent uncertainty.
24 pages, 16 figures, Submitted to NIM A
References in corpus (2)
Cited by in corpus (66)
- Solar 8B and hep Neutrino Measurements from 1258 Days of Super-Kamiokande Data
- Solar neutrino measurements in Super-Kamiokande-I
- The angular distribution of the reaction
- Solar neutrino measurements in Super-Kamiokande-II
- Solar neutrino results in Super-Kamiokande-III
- Measurement of the solar neutrino energy spectrum using neutrino-electron scattering
- Explosion Mechanism, Neutrino Burst, and Gravitational Wave in Core-Collapse Supernovae
- Solar Neutrino Measurements in Super-Kamiokande-IV
- Search for Supernova Relic Neutrinos at Super-Kamiokande
- Supernova Relic Neutrino Search at Super-Kamiokande
- Do solar neutrinos decay?
- A Redetermination of the Neutrino Mass-Squared Difference in Tri-Maximal Mixing with Terrestrial Matter Effects
- Search for Supernova Neutrino Bursts at Super-Kamiokande
- Search for Proton Decay via p -> e+ pi0 in a Large Water Cherenkov Detector
- Calibration of the Super-Kamiokande Detector
- Neutrino magnetic moments, flavor mixing, and the SuperKamiokande solar data
- Where Are We With Light Sterile Neutrinos?
- Can a supernova be located by its neutrinos?
- Imprint of SNO neutral current data on the solar neutrino problem
- Diffuse Supernova Neutrino Background Search at Super-Kamiokande
- Supernova pointing with low- and high-energy neutrino detectors
- Identifying Earth matter effects on supernova neutrinos at a single detector
- Limit On the Neutrino Magnetic Moment Using 1496 Days of Super-Kamiokande-i Solar Neutrino Data
- Detectability of the Supernova Relic Neutrinos and Neutrino Oscillation
- Optical properties of bialkali photocathodes
- Weak proton capture on 3He
- Neutrinos from Supernovae as a Trigger for Gravitational Wave Search
- Neutrino mass bound in the standard scenario for supernova electronic antineutrino emission
- Search for anti-electron-neutrinos from the Sun at Super-Kamiokande-I
- Search for neutrinos from Gamma-Ray Bursts using Super-Kamiokande
- Solar neutrino measurements using the full data period of Super-Kamiokande-IV
- Detecting the QCD phase transition in the next Galactic supernova neutrino burst
- What can we learn on supernova neutrino spectra with water Cherenkov detectors?
- Light Scalars and Dark Photons in Borexino and LSND Experiments
- 16-N as a calibration source for Super-Kamiokande
- Large Extra Dimensions, Sterile neutrinos and Solar Neutrino Data
- A new fit to solar neutrino data in models with large extra dimensions
- Search for Neutrinos in Super-Kamiokande associated with the GW170817 neutron-star merger
- Search for Neutrinos in Super-Kamiokande associated with Gravitational Wave Events GW150914 and GW151226
- Measurement of the neutrino-oxygen neutral-current interaction cross section by observing nuclear deexcitation rays
- Measurement of neutrino and antineutrino neutral-current quasielastic-like interactions on oxygen by detecting nuclear de-excitation -rays
- Solar Neutrino Precision Measurements using all 1496 Days of Super-Kamiokande-I Data
- Determination of Neutrino mixing parameters after SNO oscillation evidence
- Global analysis of Solar neutrino oscillation evidence including SNO and implications for Borexino
- Measuring the neutron star compactness and binding energy with supernova neutrinos
- Determining the Supernova Direction by its Neutrinos
- MeV-Scale Dark Matter Deep Underground
- The likelihood for supernova neutrino analyses
- On the possible observational signatures of white dwarf dynamical interactions
- Search for supernova bursts in Super-Kamiokande IV
- LSND reloaded
- Exploring the sub-eV neutrino mass range with supernova neutrinos
- Constraints on neutrino masses from a Galactic supernova neutrino signal at present and future detectors
- Are there nu_mu or nu_tau in the flux of solar neutrinos on earth?
- Another Look at Just-So Solar Neutrino Oscillations
- Tracking Performance of the Scintillating Fiber Detector in the K2K Experiment
- XMASS
- Establishing a nu_{mu,tau} Component in the Solar Neutrino Flux
- An Experimentalist's View of Neutrino Oscillations
- Status of a Supersymmetric Flavour Violating Solution to the Solar Neutrino Puzzle with Three Generations
- Maximal solution to the solar neutrino problem: just-so, MSW or energy independent?
- Potential measurement of the weak mixing angle with neutrino-electron scattering at low energy
- Supernova Neutrino Scattering off Gadolinium Even Isotopes in Water Cherenkov Detectors
- Self-Calibration of Neutrino Detectors using characteristic Backgrounds
- Measurements of the charge ratio and polarization of cosmic-ray muons with the Super-Kamiokande detector
- Measurement of the solar neutrino interaction rate below 3.49 MeV in Super-Kamiokande-IV