The DOI matches its Crossref record; 1 of the 1 references it cites were found in a registry or an index.
GOODS-Herschel: dust attenuation properties of UV selected high redshift galaxies
Open accessAbstract
Context. Dust attenuation in galaxies is poorly known, especially at high redshift. And yet the amount of dust attenuation is a key parameter to deduce accurate star formation rates from ultraviolet (UV) rest-frame measurements. The wavelength dependence of the dust attenuation is also of fundamental importance to interpret the observed spectral energy distributions (SEDs) and to derive photometric redshifts or physical properties of galaxies.
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
Synthetic properties of starburst galaxies
Leitherer, C., & Heckman, T. M. (1995) · The Astrophysical Journal Supplement Series · doi:10.1086/192112 · Cited by 672 · cited 2×
“The average age of the young stellar component is 40 Myr: a steady state in the production of the UV continuum is not reached (Leitherer & Heckman, 1995).”
Background
Cited by
CIGALE: a python Code Investigating GALaxy Emission
Boquien, M., Burgarella, D., Roehlly, Y., Buat, V., Ciesla, L., Corre, D., Inoue, A. K., & Salas, H. (2019) · Astronomy & Astrophysics · doi:10.1051/0004-6361/201834156 · Cited by 1,302
Self-citationModeling the Panchromatic Spectral Energy Distributions of Galaxies
Conroy, C. (2013) · Annual Review of Astronomy and Astrophysics · doi:10.1146/annurev-astro-082812-141017 · Cited by 959
Dusty star-forming galaxies at high redshift
Casey, C. M., Narayanan, D., & Cooray, A. (2014) · Physics Reports · doi:10.1016/j.physrep.2014.02.009 · Cited by 800
THE DUST ATTENUATION LAW IN DISTANT GALAXIES: EVIDENCE FOR VARIATION WITH SPECTRAL TYPE
Kriek, M., & Conroy, C. (2013) · The Astrophysical Journal · doi:10.1088/2041-8205/775/1/l16 · Cited by 386
Towards universal hybrid star formation rate estimators
Boquien, M., Kennicutt, R., Calzetti, D., Dale, D., Galametz, M., Sauvage, M., Croxall, K., Draine, B., Kirkpatrick, A., Kumari, N., et al. (2016) · Astronomy & Astrophysics · doi:10.1051/0004-6361/201527759 · Cited by 96
Metadata
- Authors
- Buat, V., Noll, S., Burgarella, D., Giovannoli, E., Charmandaris, V., Pannella, M., Hwang, H. S., Elbaz, D., Dickinson, M., Magdis, G., Reddy, N., & Murphy, E. J.
- Venue
- Astronomy & Astrophysics
- Publisher
- EDP Sciences
- Published
- 2012-09
- Volume
- 545
- Pages
- A141
- ISSN
- 0004-6361 (ISSN-L)
- 1432-0746
- OpenAlex
- W2145084846
- Cited by
- 192
- References
- 1
- FWCI
- 7.80
- 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: GOODS-Herschel: dust attenuation properties of UV selected high redshift galaxies. https://app.cochat.ai/papers/10.1051/0004-6361/201219405
- The paper
- Buat, V., Noll, S., Burgarella, D., Giovannoli, E., Charmandaris, V., Pannella, M., Hwang, H. S., Elbaz, D., Dickinson, M., Magdis, G., Reddy, N., & Murphy, E. J. (2012). GOODS-Herschel: dust attenuation properties of UV selected high redshift galaxies. Astronomy & Astrophysics. https://doi.org/10.1051/0004-6361/201219405
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.
