The DOI matches its Crossref record; 58 of the 60 references it cites were found in a registry or an index.
FUNDAMENTAL LIMITATIONS OF HIGH CONTRAST IMAGING SET BY SMALL SAMPLE STATISTICS
Open accessAbstract
In this paper, we review the impact of small sample statistics on detection thresholds and corresponding confidence levels (CLs) in high-contrast imaging at small angles. When looking close to the star, the number of resolution elements decreases rapidly toward small angles. This reduction of the number of degrees of freedom dramatically affects CLs and false alarm probabilities. Naively using the same ideal hypothesis and methods as for larger separations, which are well understood and commonly assume Gaussian noise, can yield up to one order of magnitude error in contrast estimations at fixed CL. The statistical penalty exponentially increases toward very small inner working angles. Even at 5–10 resolution elements from the star, false alarm probabilities can be significantly higher than expected. Here we present a rigorous statistical analysis that ensures robustness of the CL, but also imposes a substantial limitation on corresponding achievable detection limits (thus contrast) at small angles. This unavoidable fundamental statistical effect has a significant impact on current coronagraphic and future high-contrast imagers. Finally, the paper concludes with practical recommendations to account for small number statistics when computing the sensitivity to companions at small angles and when exploiting the results of direct imaging planet surveys.
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.
Claims other papers make about this one
Each is checked against this paper’s own text: does it say what the citing paper says it does?
The cited source says what the claim attributes to it.
In the citing paper
“The small number of statistically independent patches close to the central star means that a correction is required to the sensitivity as described in Mawet et al. (2014), and we apply this correction to the contrast curve.”
From ALMA and NACO observations towards the young exoring transit system J1407 (V1400 Cen) (2020) · cites this paper as Mawet et al. 2014
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
An analysis of variance test for normality (complete samples)
SHAPIRO, S. S., & WILK, M. B. (1965) · Biometrika · doi:10.1093/biomet/52.3-4.591 · Cited by 23,480
Individual Comparisons by Ranking Methods
Wilcoxon, F. (1945) · Biometrics Bulletin · doi:10.2307/3001968 · Cited by 15,354
Student (1908) · Biometrika · doi:10.1093/biomet/6.1.1 · Cited by 1,363
Angular Differential Imaging: A Powerful High‐Contrast Imaging Technique
Marois, C., Lafreniére, D., Doyon, R., Macintosh, B., & Nadeau, D. (2006) · The Astrophysical Journal · doi:10.1086/500401 · Cited by 1,092
Self-citationRobust Statistical Modeling Using the t Distribution
Lange, K. L., Little, R. J. A., & Taylor, J. M. G. (1989) · Journal of the American Statistical Association · doi:10.1080/01621459.1989.10478852 · Cited by 1,040
Soummer, R., Pueyo, L. A., & Larkin, J. (2012) · The Astrophysical Journal Letters · doi:10.1088/2041-8205/755/2/l28 · Cited by 816
Self-citationRevised standards for statistical evidence
Johnson, V. E. (2013) · Proceedings of the National Academy of Sciences · doi:10.1073/pnas.1313476110 · Cited by 808
Angular Differential Imaging: a Powerful High-Contrast Imaging Technique
Marois, C., Lafreniére, D., Doyon, R., Macintosh, B., & Nadeau, D. (2005) · OSTI OAI (U.S. Department of Energy Office of Scientific and Technical Information) · Cited by 558
Self-citationLafreniére, D., Marois, C., Doyon, R., Nadeau, D., & Artigau, É. (2007) · The Astrophysical Journal · doi:10.1086/513180 · Cited by 479
Self-citationLafreniére, D., Marois, C., Doyon, R., Nadeau, D., & Artigau, É. (2007) · CERN Document Server (European Organization for Nuclear Research) · Cited by 448
Self-citation
Research works printed but not linked: 5
- Kasper, 2012, Msngr, 149, 17
- Kenworthy, 2010, Msngr, 141, 2
- Lange, 1989, J. Am. Stat. Assoc., 84, 881
- Mawet, 2011, OptL, 36, 1506
- Razali, 2012, J. Stat. Modeling Anal., 2, 21
Cited by
Sorted by citations
SPHERE: the exoplanet imager for the Very Large Telescope
Beuzit, J.-L., Vigan, A., Mouillet, D., Dohlen, K., Gratton, R., Boccaletti, A., Sauvage, J.-F., Schmid, H. M., Langlois, M., Petit, C., et al. (2019) · Astronomy and Astrophysics · doi:10.1051/0004-6361/201935251 · Cited by 712
Self-citationDiscovery and spectroscopy of the young jovian planet 51 Eri b with the Gemini Planet Imager
Macintosh, B., Graham, J., Barman, T., de Rosa, R. D., Konopacky, Q., Marley, M., Marois, C., Nielsen, E., Pueyo, L., Rajan, A., et al. (2015) · Science · doi:10.1126/science.aac5891 · Cited by 495
Self-citationImaging Extrasolar Giant Planets
Bowler, B. P. (2016) · Publications of the Astronomical Society of the Pacific · doi:10.1088/1538-3873/128/968/102001 · Cited by 450
Accreting protoplanets in the LkCa 15 transition disk
Sallum, S., Follette, K. B., Eisner, J. A., Close, L. M., Hinz, P. M., Kratter, K. M., Males, J. R., Skemer, A. J. I., Macintosh, B., Tuthill, P., et al. (2015) · Nature · doi:10.1038/nature15761 · Cited by 299
Discovery and spectroscopy of the young jovian planet 51 Eri b with the Gemini Planet Imager
Macintosh, B., Graham, Jr., Barman, T., De Rosa, R., Konopacky, Q., Marley, M., Marois, C., Nielsen, E., Pueyo, L. A., Rajan, A., et al. (2015) · eScholarship (California Digital Library) · Cited by 292
Self-citation
Metadata
- Authors
- Mawet, D., Milli, J., Wahhaj, Z., Pelat, D., Absil, O., Delacroix, C., Boccaletti, A., Kasper, M., Kenworthy, M., Marois, C., Mennesson, B., & Pueyo, L.
- Affiliations
- European Southern Observatory (CL)
- Centre National de la Recherche Scientifique (FR)
- University of Liège (BE)
- European Southern Observatory (DE)
- Leiden University (NL)
- Herzberg Institute of Astrophysics (CA)
- Jet Propulsion Laboratory (US)
- Space Telescope Science Institute (US)
- ORCID
- Venue
- The Astrophysical Journal
- Publisher
- American Astronomical Society
- Published
- 2014-08-21
- Volume
- 792
- Issue
- 2
- Pages
- 97
- ISSN
- 0004-637X (ISSN-L)
- 1538-4357
- OpenAlex
- W2147778163
- Cited by
- 369
- References
- 56
- Citations by year
- 2026: 13 · 2025: 27 · 2024: 29 · 2023: 34 · 2022: 32 · 2021: 34 · 2020: 40 · 2019: 37 · 2018: 41 · 2017: 31 · 2016: 25 · 2015: 20 · 2014: 6
- FWCI
- 13.59
- Type
- journal article
- Language
- en
- Open access
- bronze
- doi.org
- Licence
- Locations
- The Astrophysical Journal (publishedVersion)
- arXiv (Cornell University) (submittedVersion)
- CaltechAUTHORS (California Institute of Technology) (submittedVersion)
- HAL (submittedVersion)
- NPARC (submittedVersion)
- ORBi (University of Liège) (submittedVersion, other-oa)
- arXiv (Cornell University)
- Funders
- National Aeronautics and Space Administration
- California Institute of Technology
- European Commission
- Fédération Wallonie-Bruxelles
- European Southern Observatory
- Jet Propulsion Laboratory
- Topics
- Physical Sciences › Physics and Astronomy › Atomic and Molecular Physics, and Optics › Adaptive optics and wavefront sensing
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Stellar, planetary, and galactic studies
- Physical Sciences › Physics and Astronomy › Instrumentation › Astronomy and Astrophysical Research
- Keywords
- high-contrast imaging, small sample statistics, detection threshold, confidence level, false alarm probability, inner working angle, coronagraphy, exoplanet direct imaging, statistical limitations, contrast estimation
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