The DOI matches its Crossref record.
Finding an upper limit in the presence of an unknown background
Open accessAbstract
Experimenters report an upper limit if the signal they are trying to detect is nonexistent or below their experiment's sensitivity. Such experiments may be contaminated with a background too poorly understood to subtract. If the background is distributed differently in some parameter from the expected signal, it is possible to take advantage of this difference to get a stronger limit than would be possible if the difference in distribution were ignored. We discuss the ``maximum gap'' method, which finds the best gap between events for setting an upper limit, and generalize to the ``optimum interval'' method, which uses intervals with especially few events. These methods, which apply to the case of relatively small backgrounds, do not use binning, are relatively insensitive to cuts on the range of the parameter, are parameter independent (i.e., do not change when a one-one change of variables is made), and provide true, though possibly conservative, classical one-sided confidence intervals.
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
Cited by
Results from 730 kg days of the CRESST-II Dark Matter search
Angloher, G., Bauer, M., Bavykina, I., Bento, A., Bucci, C., Ciemniak, C., Deuter, G., von Feilitzsch, F., Hauff, D., Huff, P., et al. (2012) · The European Physical Journal C · doi:10.1140/epjc/s10052-012-1971-8 · Cited by 771
First Results from the XENON10 Dark Matter Experiment at the Gran Sasso National Laboratory
Angle, J., Aprile, E., Arneodo, F., Baudis, L., Bernstein, A., Bolozdynya, A., Brusov, P., Coelho, L. C. C., Dahl, C. E., DeViveiros, L., et al. (2008) · Physical Review Letters · doi:10.1103/physrevlett.100.021303 · Cited by 648
Search for Low-Mass Weakly Interacting Massive Particles with SuperCDMS
Agnese, R., Anderson, A. J., Asai, M., Balakishiyeva, D., Basu Thakur, R., Bauer, D. A., Beaty, J., Billard, J., Borgland, A., Bowles, M. A., et al. (2014) · Physical Review Letters · doi:10.1103/physrevlett.112.241302 · Cited by 517
Self-citationAhmed, Z., Akerib, D. S., Arrenberg, S., Attisha, M. J., Bailey, C. N., Baudis, L., Bauer, D. A., Beaty, J., Brink, P. L., Bruch, T., et al. (2009) · Physical Review Letters · doi:10.1103/physrevlett.102.011301 · Cited by 419
Self-citationProjected sensitivity of the SuperCDMS SNOLAB experiment
Agnese, R., Anderson, A. J., Aramaki, T., Arnquist, I., Baker, W., Barker, D., Basu Thakur, R., Bauer, D. A., Borgland, A., Bowles, M. A., et al. (2017) · Physical Review D · doi:10.1103/physrevd.95.082002 · Cited by 287
Self-citation
Metadata
- Authors
- Yellin, S.
- Venue
- Physical Review D
- Publisher
- American Physical Society (APS)
- Published
- 2002-08-20
- Volume
- 66
- Issue
- 3
- ISSN
- 0556-2821 (ISSN-L)
- 1089-4918
- OpenAlex
- W2131670150
- Cited by
- 291
- References
- 0
- FWCI
- 1.95
- 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: Finding an upper limit in the presence of an unknown background. https://app.cochat.ai/papers/10.1103/physrevd.66.032005
- The paper
- Yellin, S. (2002). Finding an upper limit in the presence of an unknown background. Physical Review D. https://doi.org/10.1103/physrevd.66.032005
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.