The DOI matches its Crossref record; 14 of the 14 references it cites were found in a registry or an index.
A New Catalog of Photometric Redshifts in the Hubble Deep Field
Open accessAbstract
Using the newly available infrared images of the Hubble Deep Field in the J , H , and K bands and an optimal photometric method, we have refined a technique to estimate the redshifts of 1067 galaxies. A detailed comparison of our results with the spectroscopic redshifts in those cases where the latter are available shows that this technique gives very good results for bright enough objects [ AB (8140)<26.0]. From a study of the distribution of residuals [Δ z rms /(1+ z )≈0.1 at all redshifts], we conclude that the observed errors are mainly due to cosmic variance. This very important result allows for the assessment of errors in quantities to be directly or indirectly measured from the catalog. We present some of the statistical properties of the ensemble of galaxies in the catalog, and we finish by presenting a list of bright high-redshift ( z ≈5) candidates extracted from our catalog together with recent spectroscopic redshift determinations confirming that two of them are at z =5.34 and z =5.60.
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
SExtractor: Software for source extraction
Bertin, E., & Arnouts, S. (1996) · Astronomy and Astrophysics Supplement Series · doi:10.1051/aas:1996164 · Cited by 10,866
Colors and magnitudes predicted for high redshift galaxies
Coleman, G. D., Wu, C.-C., & Weedman, D. W. (1980) · The Astrophysical Journal Supplement Series · doi:10.1086/190674 · Cited by 1,213
Radiative transfer in a clumpy universe: The colors of high-redshift galaxies
Madau, P. (1995) · The Astrophysical Journal · doi:10.1086/175332 · Cited by 1,175
The Hubble Deep Field: Observations, Data Reduction, and Galaxy Photometry
Williams, R. E., Blacker, B., Dickinson, M., Dixon, W. V. D., Ferguson, H. C., Fruchter, A. S., Giavalisco, M., Gilliland, R. L., Heyer, I., Katsanis, R., et al. (1996) · The Astronomical Journal · doi:10.1086/118105 · Cited by 1,076
Slicing Through Multicolor Space: Galaxy Redshifts from Broadband Photometry
Connolly, A. J., Csabai, I., Szalay, A. S., Koo, D. C., Kron, R. G., & Munn, J. A. (1995) · The Astronomical Journal · doi:10.1086/117720 · Cited by 332
An atlas of ultraviolet spectra of star-forming galaxies
Kinney, A. L., Bohlin, R. C., Calzetti, D., Panagia, N., & Wyse, R. F. Ġ. (1993) · The Astrophysical Journal Supplement Series · doi:10.1086/191771 · Cited by 260
The Lyman Continuum in Starburst Galaxies Observed with the Hopkins Ultraviolet Telescope
Leitherer, C., Ferguson, H. C., Heckman, T. M., & Lowenthal, J. D. (1995) · The Astrophysical Journal · doi:10.1086/309760 · Cited by 256
Star-forming galaxies at very high redshifts
Lanzetta, K. M., Yahil, A., & Fernández-Soto, A. (1996) · Nature · doi:10.1038/381759a0 · Cited by 212
Self-citationPhotometric redshifts of galaxies
Loh, E. D., & Spillar, E. J. (1986) · The Astrophysical Journal · doi:10.1086/164062 · Cited by 115
A Blind Test of Photometric Redshift Prediction
Hogg, D. W., Cohen, J. G., Blandford, R. D., et al. (1998) · The Astronomical Journal · doi:10.1086/300277 · Cited by 112
Cited by
Riess, A. G., Strolger, L., Tonry, J., Casertano, S., Ferguson, H. C., Mobasher, B., Challis, P., Filippenko, A. V., Jha, S., Li, W., et al. (2004) · The Astrophysical Journal · doi:10.1086/383612 · Cited by 4,315
“In the majority of cases we found that the data from Fernández-Soto et al. (1999) and Gwynn & Hartwick (1996) contained detections in only three or four bands, whereas the NICMOS data provided a total of five to seven bands and with greater leverage.”
COSMOS PHOTOMETRIC REDSHIFTS WITH 30-BANDS FOR 2-deg2
Ilbert, O., Capak, P., Salvato, M., Aussel, H., McCracken, H. J., Sanders, D. B., Scoville, N., Kartaltepe, J., Arnouts, S., Floc'h, E. L., et al. (2009) · The Astrophysical Journal · doi:10.1088/0004-637x/690/2/1236 · Cited by 1,259
Measuring and modelling the redshift evolution of clustering: the Hubble Deep Field North
Arnouts, S., Cristiani, S., Moscardini, L., Matarrese, S., Lucchin, F., Fontana, A., & Giallongo, E. (1999) · Monthly Notices of the Royal Astronomical Society · doi:10.1046/j.1365-8711.1999.02978.x · Cited by 985
Detection of weak gravitational lensing by large-scale structure
Bacon, D. J., Refregier, A. R., & Ellis, R. S. (2000) · Monthly Notices of the Royal Astronomical Society · doi:10.1046/j.1365-8711.2000.03851.x · Cited by 594
The Stellar Populations and Evolution of Lyman Break Galaxies
Papovich, C., Dickinson, M., & Ferguson, H. C. (2001) · The Astrophysical Journal · doi:10.1086/322412 · Cited by 593
Metadata
- Authors
- Fernandez‐Soto, A., Lanzetta, K. M., & Yahil, A.
- Venue
- The Astrophysical Journal
- Publisher
- American Astronomical Society
- Published
- 1999-03
- Volume
- 513
- Issue
- 1
- Pages
- 34-50
- ISSN
- 0004-637X (ISSN-L)
- 1538-4357
- OpenAlex
- W1992083220
- Cited by
- 390
- References
- 14
- FWCI
- 39.72
- 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: A New Catalog of Photometric Redshifts in the Hubble Deep Field. https://app.cochat.ai/papers/10.1086/306847
- The paper
- Fernandez‐Soto, A., Lanzetta, K. M., & Yahil, A. (1999). A New Catalog of Photometric Redshifts in the Hubble Deep Field. The Astrophysical Journal. https://doi.org/10.1086/306847
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.