The DOI matches its Crossref record; 104 of the 104 references it cites were found in a registry or an index.
New Determinations of the UV Luminosity Functions from z ∼ 9 to 2 Show a Remarkable Consistency with Halo Growth and a Constant Star Formation Efficiency
Open accessAbstract
Here we provide the most comprehensive determinations of the rest-frame UV luminosity function (LF) available to date with the Hubble Space Telescope (HST) at z ∼ 2–9. Essentially all of the noncluster extragalactic legacy fields are utilized, including the Hubble Ultra Deep Field, the Hubble Frontier Fields parallel fields, and all five CANDELS fields, for a total survey area of 1136 arcmin 2. Our determinations include galaxies at z ∼ 2–3 leveraging the deep HDUV, UVUDF, and ERS WFC3/UVIS observations available over an ∼150 arcmin 2 area in the GOODS-North and GOODS-South regions. All together, our collective samples include >24,000 sources, >2.3× larger than previous selections with HST. We identify 5766, 6332, 7240, 3449, 1066, 601, 246, and 33 sources at z ∼ 2, 3, 4, 5, 6, 7, 8, and 9, respectively. Combining our results with an earlier z ∼ 10 LF determination by Oesch et al., we quantify the evolution of the UV LF. Our results indicate that there is (1) a smooth flattening of the faint-end slope α from α ∼ −2.4 at z ∼ 10 to α ∼ −1.5 at z ∼ 2, (2) minimal evolution in the characteristic luminosity M* at z ≥ 2.5, and (3) a monotonic increase in the normalization log 10 ϕ * from z ∼ 10 to 2, which can be well described by a simple second-order polynomial, consistent with an “accelerated” evolution scenario. We find that each of these trends (from z ∼ 10 to 2.5 at least) can be readily explained on the basis of the evolution of the halo mass function and a simple constant star formation efficiency model.
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
Madau, P., & Dickinson, M. (2014) · Annual Review of Astronomy and Astrophysics · doi:10.1146/annurev-astro-081811-125615 · Cited by 3,898
Croton, D. J., Springel, V., White, S. D. M., De Lucia, G., Frenk, C. S., Gao, L., Jenkins, A., Kauffmann, G., Navarro, J. F., & Yoshida, N. (2006) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2005.09675.x · Cited by 3,685
Secondary standard stars for absolute spectrophotometry
Oke, J. B., & Gunn, J. E. (1983) · The Astrophysical Journal · doi:10.1086/160817 · Cited by 2,811
THE AVERAGE STAR FORMATION HISTORIES OF GALAXIES IN DARK MATTER HALOS FROM z = 0-8
Behroozi, P. S., Wechsler, R. H., & Conroy, C. (2013) · The Astrophysical Journal · doi:10.1088/0004-637x/770/1/57 · Cited by 2,167
CANDELS: THE COSMIC ASSEMBLY NEAR-INFRARED DEEP EXTRAGALACTIC LEGACY SURVEY
Grogin, N. A., Kocevski, D. D., Faber, S. M., Ferguson, H. C., Koekemoer, A. M., Riess, A. G., Acquaviva, V., Alexander, D. M., Almaini, O., Ashby, M. L. N., et al. (2011) · The Astrophysical Journal Supplement Series · doi:10.1088/0067-0049/197/2/35 · Cited by 2,133
Self-citationHigh-redshift galaxies in the Hubble Deep Field: colour selection and star formation history to z 4
Madau, P., Ferguson, H. C., Dickinson, M. E., Giavalisco, M., Steidel, C. C., & Fruchter, A. (1996) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/283.4.1388 · Cited by 2,055
Koekemoer, A. M., Faber, S. M., Ferguson, H. C., Grogin, N. A., Kocevski, D. D., Koo, D. C., Lai, K., Lotz, J. M., Lucas, R. A., McGrath, E. J., et al. (2011) · The Astrophysical Journal Supplement Series · doi:10.1088/0067-0049/197/2/36 · Cited by 2,052
Self-citationPeng, Y.-J., Lilly, S. J., Kovač, K., Bolzonella, M., Pozzetti, L., Renzini, A., Zamorani, G., Ilbert, O., Knobel, C., Iovino, A., et al. (2010) · The Astrophysical Journal · doi:10.1088/0004-637x/721/1/193 · Cited by 1,994
Self-citationEAZY: A Fast, Public Photometric Redshift Code
Brammer, G. B., van Dokkum, P. G., & Coppi, P. (2008) · The Astrophysical Journal · doi:10.1086/591786 · Cited by 1,841
Cited by
JADES: The diverse population of infant black holes at 4 < z < 11: Merging, tiny, poor, but mighty
Maiolino, R., Scholtz, J., Curtis-Lake, E., Carniani, S., Baker, W., de Graaff, A., Tacchella, S., Übler, H., D’Eugenio, F., Witstok, J., et al. (2024) · Astronomy & Astrophysics · doi:10.1051/0004-6361/202347640 · Cited by 373
A Long Time Ago in a Galaxy Far, Far Away: A Candidate z ∼ 12 Galaxy in Early JWST CEERS Imaging
Finkelstein, S. L., Bagley, M. B., Arrabal Haro, P., Dickinson, M., Ferguson, H. C., Kartaltepe, J. S., Papovich, C., Burgarella, D., Kocevski, D. D., Huertas-Company, M., et al. (2022) · The Astrophysical Journal Letters · doi:10.3847/2041-8213/ac966e · Cited by 339
Self-citationThe GLASS-JWST Early Release Science Program. I. Survey Design and Release Plans
Treu, T., Roberts-Borsani, G., Bradac, M., Brammer, G., Fontana, A., Henry, A., Mason, C., Morishita, T., Pentericci, L., Wang, X., et al. (2022) · The Astrophysical Journal · doi:10.3847/1538-4357/ac8158 · Cited by 270
Self-citation
Metadata
- Authors
- Bouwens, R. J., Oesch, P. A., Stefanon, M., Illingworth, G., Labbé, I., Reddy, N., Atek, H., Montes, M., Naidu, R., Nanayakkara, T., Nelson, E., & Wilkins, S.
- Venue
- The Astronomical Journal
- Publisher
- American Astronomical Society
- Published
- 2021-07-07
- Volume
- 162
- Issue
- 2
- Pages
- 47
- ISSN
- 0004-6256 (ISSN-L)
- 1538-3881
- OpenAlex
- W3132462017
- Cited by
- 406
- References
- 104
- FWCI
- 34.47
- 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: New Determinations of the UV Luminosity Functions from z ∼ 9 to 2 Show a Remarkable Consistency with Halo Growth and a Constant Star Formation Efficiency. https://app.cochat.ai/papers/10.3847/1538-3881/abf83e
- The paper
- Bouwens, R. J., Oesch, P. A., Stefanon, M., Illingworth, G., Labbé, I., Reddy, N., Atek, H., Montes, M., Naidu, R., Nanayakkara, T., Nelson, E., & Wilkins, S. (2021). New Determinations of the UV Luminosity Functions from z ∼ 9 to 2 Show a Remarkable Consistency with Halo Growth and a Constant Star Formation Efficiency. The Astronomical Journal. https://doi.org/10.3847/1538-3881/abf83e
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.