Student or educator? Sign up with your school email and get 6 months of Pro free.
Cited by 294

The DOI matches its Crossref record; 88 of the 88 references it cites were found in a registry or an index.

The Giant Radio Array for Neutrino Detection (GRAND): Science and design

Open access
Álvarez-Muñiz, Jaime, Alves Batista, Rafael, Balagopal V., Aswathi, Bolmont, Julien, Bustamante, Mauricio, Carvalho, Washington, Charrier, Didier, Cognard, Ismaël, Decoene, Valentin, Denton, Peter B., De Jong, Sijbrand, De Vries, Krijn D., Engel, Ralph, Fang, Ke, Finley, Chad, Gabici, Stefano, Gou, QuanBu, Gu, JunHua, Guépin, Claire, Hu, HongBo, Huang, Yan, Kotera, Kumiko, Le Coz, Sandra, Lenain, Jean-Philippe, Lü, GuoLiang, Martineau-Huynh, Olivier, Mostafá, Miguel, Mottez, Fabrice, Murase, Kohta, Niess, Valentin, Oikonomou, Foteini, Pierog, Tanguy, Qian, XiangLi, Qin, Bo, Ran, Duan, Renault-Tinacci, Nicolas, Roth, Markus, Schröder, Frank G., Schüssler, Fabian, Tasse, Cyril, Timmermans, Charles, Tueros, Matías, Wu, XiangPing, Zarka, Philippe, Zech, Andreas, Zhang, B. Theodore, Zhang, JianLi, Zhang, Yi, Zheng, Qian, Zilles, Anne·2020·Science China Physics, Mechanics & Astronomy

Abstract

The Giant Radio Array for Neutrino Detection (GRAND) is a planned large-scale observatory of ultra-high-energy (UHE) cosmic particles, with energies exceeding 108 GeV. Its goal is to solve the long-standing mystery of the origin of UHE cosmic rays. To do this, GRAND will detect an unprecedented number of UHE cosmic rays and search for the undiscovered UHE neutrinos and gamma rays associated to them with unmatched sensitivity. GRAND will use large arrays of antennas to detect the radio emission coming from extensive air showers initiated by UHE particles in the atmosphere. Its design is modular: 20 separate, independent sub-arrays, each of 10000 radio antennas deployed over 10000 km2. A staged construction plan will validate key detection techniques while achieving important science goals early. Here we present the science goals, detection strategy, preliminary design, performance goals, and construction plans for GRAND.

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.

A few free checks a day · papers already verified open instantly · results are public

Integrity signals

Registry

Crossref · 10.1007/s11433-018-9385-7

Cites

88 of 88 references verified0 citation errors · 0 not checkable

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.

A few free checks a day · papers already verified open instantly · results are public

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

Show all 88 references

Metadata

Authors
Álvarez-Muñiz, J., Alves Batista, R., Balagopal V., A., Bolmont, J., Bustamante, M., Carvalho, W., Charrier, D., Cognard, I., Decoene, V., Denton, P. B., De Jong, S., De Vries, K. D., Engel, R., Fang, K., Finley, C., Gabici, S., Gou, Q., Gu, J., Guépin, C., Hu, H., Huang, Y., Kotera, K., Le Coz, S., Lenain, J.-P., Lü, G., Martineau-Huynh, O., Mostafá, M., Mottez, F., Murase, K., Niess, V., Oikonomou, F., Pierog, T., Qian, X., Qin, B., Ran, D., Renault-Tinacci, N., Roth, M., Schröder, F. G., Schüssler, F., Tasse, C., Timmermans, C., Tueros, M., Wu, X., Zarka, P., Zech, A., Zhang, B. T., Zhang, J., Zhang, Y., Zheng, Q., & Zilles, A.
Venue
Science China Physics, Mechanics & Astronomy
Published
2019-08-04
Volume
63
Issue
1
ISSN
  • 1869-1927 (ISSN-L)
  • 1674-7348
OpenAlex
W2897415481
Cited by
294
References
88
FWCI
19.38
Type
journal article
Language
en
Open access
green

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: The Giant Radio Array for Neutrino Detection (GRAND): Science and design. https://app.cochat.ai/papers/10.1007/s11433-018-9385-7
The paper
Álvarez-Muñiz, J., Alves Batista, R., Balagopal V., A., Bolmont, J., Bustamante, M., Carvalho, W., Charrier, D., Cognard, I., Decoene, V., Denton, P. B., De Jong, S., De Vries, K. D., Engel, R., Fang, K., Finley, C., Gabici, S., Gou, Q., Gu, J., Guépin, C., . . . Zilles, A. (2020). The Giant Radio Array for Neutrino Detection (GRAND): Science and design. Science China Physics, Mechanics & Astronomy. https://doi.org/10.1007/s11433-018-9385-7

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.