The DOI matches its Crossref record; 5 of the 5 references it cites were found in a registry or an index.
CLASH: THREE STRONGLY LENSED IMAGES OF A CANDIDATE z≈ 11 GALAXY
Open accessAbstract
We present a candidate for the most distant galaxy known to date with a photometric redshift of z = 10.7 +0.6 −0.4 (95% confidence limits; with z < 9.5 galaxies of known types ruled out at 7.2σ). This J -dropout Lyman break galaxy, named MACS0647-JD, was discovered as part of the Cluster Lensing and Supernova survey with Hubble (CLASH). We observe three magnified images of this galaxy due to strong gravitational lensing by the galaxy cluster MACSJ0647.7+7015 at z = 0.591. The images are magnified by factors of ∼80, 7, and 2, with the brighter two observed at ∼26th magnitude AB (∼0.15 μJy) in the WFC3/IR F160W filter (∼1.4–1.7 μm) where they are detected at ≳12σ. All three images are also confidently detected at ≳6σ in F140W (∼1.2–1.6 μm), dropping out of detection from 15 lower wavelength Hubble Space Telescope filters (∼0.2–1.4 μm), and lacking bright detections in Spitzer /IRAC 3.6 μm and 4.5 μm imaging (∼3.2–5.0 μm). We rule out a broad range of possible lower redshift interlopers, including some previously published as high-redshift candidates. Our high-redshift conclusion is more conservative than if we had neglected a Bayesian photometric redshift prior. Given CLASH observations of 17 high-mass clusters to date, our discoveries of MACS0647-JD at z ∼ 10.8 and MACS1149-JD at z ∼ 9.6 are consistent with a lensed luminosity function extrapolated from lower redshifts. This would suggest that low-luminosity galaxies could have reionized the universe. However, given the significant uncertainties based on only two galaxies, we cannot yet rule out the sharp drop-off in number counts at z ≳ 10 suggested by field searches.
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
Schlegel, D. J., Finkbeiner, D. P., & Davis, M. (1998) · The Astrophysical Journal · doi:10.1086/305772 · Cited by 15,126
The Structure of Cold Dark Matter Halos
Navarro, J. F., Frenk, C. S., & White, S. D. M. (1996) · The Astrophysical Journal · doi:10.1086/177173 · Cited by 8,544 · cited 1×
“The Lenstool model consisted of an ellipsoidal NFW halo (Navarro et al. 1996) plus cluster galaxies modeled as truncated PIEMDs (pseudo-isothermal elliptical mass distributions; Kassiola & Kovner 1993).”
MethodPowell, M. J. D. (1964) · The Computer Journal · doi:10.1093/comjnl/7.2.155 · Cited by 4,632 · cited 1×
“Finally, we ran Powell (1964) minimizations to find the best fitting SEDs at each of these redshifts.”
MethodStarburst99: Synthesis Models for Galaxies with Active Star Formation
Leitherer, C., Schaerer, D., Goldader, J. D., Delgado, R. M. G., Robert, C., Kune, D. F., de Mello, D. F., Devost, D., & Heckman, T. M. (1999) · The Astrophysical Journal Supplement Series · doi:10.1086/313233 · Cited by 4,126
FOCUSING COSMIC TELESCOPES: EXPLORING REDSHIFT z∼ 5-6 GALAXIES WITH THE BULLET CLUSTER 1E0657 – 56
Bradač, M., Treu, T., Applegate, D., Gonzalez, A. H., Clowe, D., Forman, W., Jones, C., Marshall, P., Schneider, P., & Zaritsky, D. (2009) · The Astrophysical Journal · doi:10.1088/0004-637x/706/2/1201 · Cited by 128
Cited by
UV LUMINOSITY FUNCTIONS AT REDSHIFTS z∼ 4 TO z∼ 10: 10,000 GALAXIES FROM HST LEGACY FIELDS
Bouwens, R. J., Illingworth, G. D., Oesch, P. A., Trenti, M., Labbé, I., Bradley, L., Carollo, M., van Dokkum, P. G., Gonzalez, V., Holwerda, B., et al. (2015) · The Astrophysical Journal · doi:10.1088/0004-637x/803/1/34 · Cited by 1,298
Self-citationCosmic structure as the quantum interference of a coherent dark wave
Schive, H.-Y., Chiueh, T., & Broadhurst, T. (2014) · Nature Physics · doi:10.1038/nphys2996 · Cited by 930
Self-citationFinkelstein, S. L., Ryan, R. E., Papovich, C., Dickinson, M., Song, M., Somerville, R. S., Ferguson, H. C., Salmon, B., Giavalisco, M., Koekemoer, A. M., et al. (2015) · The Astrophysical Journal · doi:10.1088/0004-637x/810/1/71 · Cited by 729
Self-citationCANDELS MULTI-WAVELENGTH CATALOGS: SOURCE DETECTION AND PHOTOMETRY IN THE GOODS-SOUTH FIELD
Guo, Y., Ferguson, H. C., Giavalisco, M., Barro, G., Willner, S. P., Ashby, M. L. N., Dahlen, T., Donley, J. L., Faber, S. M., Fontana, A., et al. (2013) · The Astrophysical Journal Supplement Series · doi:10.1088/0067-0049/207/2/24 · Cited by 526
Self-citationEllis, R. S., McLure, R. J., Dunlop, J. S., Robertson, B. E., Ono, Y., Schenker, M. A., Koekemoer, A., Bowler, R. A. A., Ouchi, M., Rogers, A. B., et al. (2013) · The Astrophysical Journal · doi:10.1088/2041-8205/763/1/l7 · Cited by 512
Self-citation
Metadata
- Authors
- Coe, D., Zitrin, A., Carrasco, M., Shu, X., Zheng, W., Postman, M., Bradley, L., Koekemoer, A., Bouwens, R., Broadhurst, T., Monna, A., Host, O., Moustakas, L. A., Ford, H., Moustakas, J., van der Wel, A., Donahue, M., Rodney, S. A., Benítez, N., Jouvel, S., Seitz, S., Kelson, D. D., & Rosati, P.
- Venue
- The Astrophysical Journal
- Publisher
- American Astronomical Society
- Published
- 2012-12-13
- Volume
- 762
- Issue
- 1
- Pages
- 32
- ISSN
- 0004-637X (ISSN-L)
- 1538-4357
- OpenAlex
- W2023842147
- Cited by
- 374
- References
- 5
- FWCI
- 23.56
- Type
- journal article
- Language
- en
- Open access
- bronze
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: CLASH: THREE STRONGLY LENSED IMAGES OF A CANDIDATE z≈ 11 GALAXY. https://app.cochat.ai/papers/10.1088/0004-637x/762/1/32
- The paper
- Coe, D., Zitrin, A., Carrasco, M., Shu, X., Zheng, W., Postman, M., Bradley, L., Koekemoer, A., Bouwens, R., Broadhurst, T., Monna, A., Host, O., Moustakas, L. A., Ford, H., Moustakas, J., van der Wel, A., Donahue, M., Rodney, S. A., Benítez, N., . . . Rosati, P. (2013). CLASH: THREE STRONGLY LENSED IMAGES OF A CANDIDATE z≈ 11 GALAXY. The Astrophysical Journal. https://doi.org/10.1088/0004-637x/762/1/32
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.