The DOI matches its Crossref record; 16 of the 16 references it cites were found in a registry or an index.
Complete results for five years of GNO solar neutrino observations
Open accessAbstract
We report the complete GNO solar neutrino results for the measuring periods GNO III, GNO II, and GNO I. The result for GNO III (last 15 solar runs) is [54.3−9.3+9.9(stat)±2.3(syst)]SNU (1σ) or [54.3−9.6+10.2(incl. syst)]SNU (1σ) with errors combined. The GNO experiment is now terminated after altogether 58 solar exposure runs that were performed between 20 May 1998 and 9 April 2003. The combined result for GNO (I + II + III) is [62.9−5.3+5.5(stat)±2.5(syst)]SNU (1σ) or [62.9−5.9+6.0]SNU (1σ) with errors combined in quadrature. Overall, gallium based solar observations at LNGS (first in GALLEX, later in GNO) lasted from 14 May 1991 through 9 April 2003. The joint result from 123 runs in GNO and GALLEX is [69.3±5.5(incl. syst)]SNU (1σ). The distribution of the individual run results is consistent with the hypothesis of a neutrino flux that is constant in time. Implications from the data in particle- and astrophysics are reiterated.
Overview
The claims and statistics of this paper haven’t been checked yet.
Run the check — free, no account needed. It reads the open-access text and checks the sources it cites.
Integrity signals
Registry
Cites
Statistics
Verification
Claims the paper makes
The claims and statistics of this paper haven’t been checked yet.
Run the check — free, no account needed. It reads the open-access text and checks the sources it cites.
Self-check
Percentages, sums and reported differences re-computed from the paper’s own numbers.
The self-check needs the paper’s full text.
Citations
Cites
Scargle, J. D. (1982) · The Astrophysical Journal · doi:10.1086/160554 · Cited by 7,376
Least-squares frequency analysis of unequally spaced data
Lomb, N. R. (1976) · Astrophysics and Space Science · doi:10.1007/bf00648343 · Cited by 5,717
Measurement of the Solar Electron Neutrino Flux with the Homestake Chlorine Detector
Cleveland, B. T., Daily, T., Davis, Jr., Distel, J. R., Lande, K., Lee, C. K., Wildenhain, P. S., & Ullman, J. (1998) · The Astrophysical Journal · doi:10.1086/305343 · Cited by 1,974
GALLEX solar neutrino observations: results for GALLEX IV
Hampel, W., Handt, J., Heusser, G., Kiko, J., Kirsten, T., Laubenstein, M., Pernicka, E., Rau, W., Wojcik, M., Zakharov, Y., et al. (1999) · Physics Letters B · doi:10.1016/s0370-2693(98)01579-2 · Cited by 1,329
Self-citationSolar Models: Current Epoch and Time Dependences, Neutrinos, and Helioseismological Properties
Bahcall, J. N., Pinsonneault, M. H., & Basu, S. (2001) · The Astrophysical Journal · doi:10.1086/321493 · Cited by 885
Ahmed, S. N., Anthony, A. E., Beier, E. W., Bellerive, A., Biller, S. D., Boger, J., Boulay, M. G., Bowler, M. G., Bowles, T. J., Brice, S. J., et al. (2004) · Physical Review Letters · doi:10.1103/physrevlett.92.181301 · Cited by 773
Solar Models: current epoch and time dependences, neutrinos, and helioseismological properties
Bahcall, J. N., Pinsonneault, M. H., & Basu, S. (2001) · CERN Document Server (European Organization for Nuclear Research) · Cited by 561
GNO solar neutrino observations: results for GNO I
Altmann, M., Balata, M., Belli, P., Bellotti, E., Bernabei, R., Burkert, E., Cattadori, C., Cerichelli, G., Chiarini, M., Cribier, M., et al. (2000) · Physics Letters B · doi:10.1016/s0370-2693(00)00915-1 · Cited by 523
Self-citationA Reappraisal of the Solar Photospheric C/O Ratio
Allende Prieto, C., Lambert, D. L., & Asplund, M. (2002) · The Astrophysical Journal · doi:10.1086/342095 · Cited by 429
Where do we stand with solar neutrino oscillations?
Bahcall, J. N., Krastev, P. I., & Smirnov, A. Y. (1998) · Physical Review D · doi:10.1103/physrevd.58.096016 · Cited by 411
Cited by
First year performance of the IceCube neutrino telescope
Achterberg, A., Ackermann, M., Adams, J., Ahrens, J., Andeen, K., Atlee, D. W., Baccus, J., Bahcall, J. N., Bai, X., Baret, B., et al. (2006) · Astroparticle Physics · doi:10.1016/j.astropartphys.2006.06.007 · Cited by 477
Global analysis of three-flavor neutrino masses and mixings
Fogli, G. L., Lisi, E., Marrone, A., & Palazzo, A. (2006) · Progress in Particle and Nuclear Physics · doi:10.1016/j.ppnp.2005.08.002 · Cited by 386
Supernova Neutrinos: Production, Oscillations and Detection
Mirizzi, A., Tamborra, I., Janka, H., Saviano, N., Scholberg, K., Bollig, R., Hüdepohl, L., & Chakraborty, S. (2015) · arXiv (Cornell University) · doi:10.15161/oar.it/1446204340.05 · Cited by 366
From the Trees to the Forest: A Review of Radiative Neutrino Mass Models
Cai, Y., Herrero García, J., Schmidt, M. A., Vicente, A., & Volkas, R. R. (2017) · Frontiers in Physics · doi:10.3389/fphy.2017.00063 · Cited by 341
Nobel Lecture: The Sudbury Neutrino Observatory: Observation of flavor change for solar neutrinos
McDonald, A. B. (2016) · Reviews of Modern Physics · doi:10.1103/revmodphys.88.030502 · Cited by 303
Metadata
- Authors
- Altmann, M., Balata, M., Belli, P., Bellotti, E., Bernabei, R., Burkert, E., Cattadori, C., Cerulli, R., Chiarini, M., Cribier, M., d'Angelo, S., Del Re, G., Ebert, K. H., von Feilitzsch, F., Ferrari, N., Hampel, W., Hartmann, F. X., Henrich, E., Heusser, G., Kaether, F., Kiko, J., Kirsten, T., Lachenmaier, T., Lanfranchi, J., Laubenstein, M., Lützenkirchen, K., Mayer, K., Moegel, P., Motta, D., Nisi, S., Oehm, J., Pandola, L., Petricca, F., Potzel, W., Richter, H., Schoenert, S., Wallenius, M., Wojcik, M., & Zanotti, L.
- Venue
- Physics Letters B
- Publisher
- Elsevier BV
- Published
- 2005-06
- Volume
- 616
- Issue
- 3-4
- Pages
- 174-190
- ISSN
- 0370-2693 (ISSN-L)
- OpenAlex
- W2013362937
- Cited by
- 408
- References
- 16
- FWCI
- 17.92
- Type
- journal article
- Language
- en
- Open access
- hybrid
About these checks
Registry, retraction, Cites and statistics results are computed, not judged, with one exception: a printed reference that no index lists is read once by a model before it counts as a citation error. Claims are extracted by a model and kept only when their quote appears verbatim in the text; each cited source is then checked, with a model’s help, for whether it says what the claim relies on. Those verdicts can be wrong — read the claim’s quote and the cited source before relying on one.
Statistics and arithmetic are recomputed, not judged.
Confidence bands are shown only for fields calibrated on our annotated test set. None is calibrated yet, so no band is shown.
What counts as a claim ›How we measure confidence ›How we check this ›
Are you an author, or do you see a problem with this page? Request a review
How to cite
Cite CoChat for the checks on this page, and the paper for its own findings.
- This page
- CoChat. (2026). Citation check: Complete results for five years of GNO solar neutrino observations. https://app.cochat.ai/papers/10.1016/j.physletb.2005.04.068
- The paper
- Altmann, M., Balata, M., Belli, P., Bellotti, E., Bernabei, R., Burkert, E., Cattadori, C., Cerulli, R., Chiarini, M., Cribier, M., d'Angelo, S., Del Re, G., Ebert, K. H., von Feilitzsch, F., Ferrari, N., Hampel, W., Hartmann, F. X., Henrich, E., Heusser, G., . . . Zanotti, L. (2005). Complete results for five years of GNO solar neutrino observations. Physics Letters B. https://doi.org/10.1016/j.physletb.2005.04.068
Data sources
Bibliographic data: Semantic Scholar, OpenAlex, Crossref.
Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).
Semantic Scholar’s data is described in: Kinney, R., et al. (2023). The Semantic Scholar Open Data Platform. arXiv:2301.10140.