The DOI matches its Crossref record; 1 of the 1 references it cites were found in a registry or an index.
GEMS: Galaxy Evolution from Morphologies and SEDs
Open accessAbstract
GEMS (Galaxy Evolution from Morphologies and SEDs) is a large-area (800 arcmin 2 ) two-color (F606W and F850LP) imaging survey with the Advanced Camera for Surveys on the Hubble Space Telescope . Centered on the Chandra Deep Field-South, it covers an area of ~28' × 28', or about 120 Hubble Deep Field areas, to a depth of m AB (F606W) = 28.3(5 σ) and m AB (F850LP) = 27.1(5 σ) for compact sources. In its central ~1/4, GEMS incorporates ACS imaging from the GOODS project. Focusing on the redshift range 0.2 ≲ z ≲ 1.1, GEMS provides morphologies and structural parameters for nearly 10,000 galaxies where redshift estimates, luminosities, and SEDs exist from COMBO-17. At the same time, GEMS contains detectable host galaxy images for several hundred faint active galactic nuclei. This paper provides an overview of the science goals, the experiment design, the data reduction, and the science analysis plan for GEMS.
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
Spergel, D. N., Verde, L., Peiris, H. V., Komatsu, E., Nolta, M. R., Bennett, C. L., Halpern, M., Hinshaw, G., Jarosik, N., Kogut, A., et al. (2003) · The Astrophysical Journal Supplement Series · doi:10.1086/377226 · Cited by 10,976
Cited by
CALIFA, the Calar Alto Legacy Integral Field Area survey: I. Survey presentation⋆
Sánchez, S. F., Kennicutt, R. C., Gil de Paz, A., van de Ven, G., Vílchez, J. M., Wisotzki, L., Walcher, C. J., Mast, D., Aguerri, J. A. L., Albiol-Pérez, S., et al. (2012) · Astronomy & Astrophysics · doi:10.1051/0004-6361/201117353 · Cited by 1,254
Self-citationKiDS-450: cosmological parameter constraints from tomographic weak gravitational lensing
Hildebrandt, H., Viola, M., Heymans, C., Joudaki, S., Kuijken, K., Blake, C., Erben, T., Joachimi, B., Klaes, D., Miller, L., et al. (2017) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stw2805 · Cited by 1,021
Toward an Understanding of the Rapid Decline of the Cosmic Star Formation Rate
Bell, E. F., Papovich, C., Wolf, C., Le Floc’h, E., Caldwell, J. A. R., Barden, M., Egami, E., McIntosh, D. H., Meisenheimer, K., Perez‐Gonzalez, P. G., et al. (2005) · The Astrophysical Journal · doi:10.1086/429552 · Cited by 494
Self-citationTHE MAJOR AND MINOR GALAXY MERGER RATES AT z < 1.5
Lotz, J. M., Jonsson, P., Cox, T. J., Croton, D., Primack, J. R., Somerville, R. S., & Stewart, K. (2011) · The Astrophysical Journal · doi:10.1088/0004-637x/742/2/103 · Cited by 450
Self-citationBouwens, R. J., Illingworth, G. D., Blakeslee, J. P., & Franx, M. (2006) · The Astrophysical Journal · doi:10.1086/498733 · Cited by 344
Metadata
- Authors
- Rix, H., Barden, M., Beckwith, S. V. W., Bell, E. F., Borch, A., Caldwell, J. A. R., Haussler, B., Jahnke, K., Jogee, S., McIntosh, D. H., Meisenheimer, K., Peng, C. Y., Sanchez, S. F., Somerville, R. S., Wisotzki, L., & Wolf, C.
- Venue
- The Astrophysical Journal Supplement Series
- Publisher
- American Astronomical Society
- Published
- 2004-06
- Volume
- 152
- Issue
- 2
- Pages
- 163-173
- ISSN
- 0067-0049 (ISSN-L)
- 1538-4365
- OpenAlex
- W2066202006
- Cited by
- 420
- References
- 1
- FWCI
- 19.89
- 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: GEMS: Galaxy Evolution from Morphologies and SEDs. https://app.cochat.ai/papers/10.1086/420885
- The paper
- Rix, H., Barden, M., Beckwith, S. V. W., Bell, E. F., Borch, A., Caldwell, J. A. R., Haussler, B., Jahnke, K., Jogee, S., McIntosh, D. H., Meisenheimer, K., Peng, C. Y., Sanchez, S. F., Somerville, R. S., Wisotzki, L., & Wolf, C. (2004). GEMS: Galaxy Evolution from Morphologies and SEDs. The Astrophysical Journal Supplement Series. https://doi.org/10.1086/420885
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.
