The DOI matches its Crossref record; 3 of the 3 references it cites were found in a registry or an index.
Semi-analytic modelling of galaxy formation: the local Universe
Open accessAbstract
Using semi-analytic models of galaxy formation, we investigate galaxy properties such as the Tully-Fisher relation, the B- and K-band LFs, cold gas contents, sizes, metallicities and colours, and compare our results with observations of local galaxies. We investigate several different recipes for star formation and supernova feedback, including choices that are similar to the treatment by Kauffmann, White & Guiderdoni and Cole et al., as well as some new recipes. We obtain good agreement with all of the key local observations mentioned above. In particular, in our best models, we simultaneously produce good agreement with both the observed B- and K-band LFs and the I-band Tully-Fisher relation. Improved cooling and supernova feedback modelling, inclusion of dust extinction and an improved Press-Schechter model all contribute to this success. We present results for several variants of the CDM family of cosmologies, and find that models with values of Ω0≃0.3–0.5 give the best agreement with observations.
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
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
The origin of dwarf galaxies, cold dark matter, and biased galaxy formation
Dekel, A., & Silk, J. (1986) · The Astrophysical Journal · doi:10.1086/164050 · Cited by 1,919 · cited 1×
“Following the general argu- c© 0000 RAS, MNRAS 000, 000–000 ments of Dekel & Silk (1986), we now calculate the rate at which gas can escape from the disk: ṁrh, disk = 2frh,disk ǫ̇SN 〈v2 esc, disk〉 , (9) and from the halo (same expression with 〈v2esc, halo〉).”
BackgroundContraction of dark matter galactic halos due to baryonic infall
Blumenthal, G. R., Faber, S. M., Flores, R., & Primack, J. R. (1986) · The Astrophysical Journal · doi:10.1086/163867 · Cited by 1,213 · cited 3×
“We neglect the modification of the inner profile of the dark matter due to the infall of the baryons, which will tend to lead to smaller disks (Blumenthal et al. 1986; Flores et al. 1993; Mo, Mao, & White 1998).”
BackgroundInfluentialSelf-citation
Cited by
Cole, S., Lacey, C. G., Baugh, C. M., & Frenk, C. S. (2002) · Monthly Notices of the Royal Astronomical Society · doi:10.1046/j.1365-8711.2000.03879.x · Cited by 1,952
Large-scale structure of the Universe and cosmological perturbation theory
Bernardeau, F., Colombi, S., Gaztañaga, E., & Scoccimarro, R. (2002) · Physics Reports · doi:10.1016/s0370-1573(02)00135-7 · Cited by 1,922
A HIGHLY CONSISTENT FRAMEWORK FOR THE EVOLUTION OF THE STAR-FORMING “MAIN SEQUENCE” FROM z ∼ 0-6
Speagle, J. S., Steinhardt, C. L., Capak, P. L., & Silverman, J. D. (2014) · The Astrophysical Journal Supplement Series · doi:10.1088/0067-0049/214/2/15 · Cited by 1,646
The EAGLE simulations of galaxy formation: calibration of subgrid physics and model variations
Crain, R. A., Schaye, J., Bower, R. G., Furlong, M., Schaller, M., Theuns, T., Dalla Vecchia, C., Frenk, C. S., McCarthy, I. G., Helly, J. C., et al. (2015) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stv725 · Cited by 1,451
Theoretical Challenges in Galaxy Formation
Naab, T., & Ostriker, J. P. (2017) · Annual Review of Astronomy and Astrophysics · doi:10.1146/annurev-astro-081913-040019 · Cited by 722
Metadata
- Authors
- Somerville, R. S., & Primack, J. R.
- Venue
- Monthly Notices of the Royal Astronomical Society
- Publisher
- Oxford University Press (OUP)
- Published
- 1999-12
- Volume
- 310
- Issue
- 4
- Pages
- 1087-1110
- ISSN
- 0035-8711 (ISSN-L)
- 1365-2966
- OpenAlex
- W1969514664
- Cited by
- 1,073
- References
- 3
- FWCI
- 46.89
- 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: Semi-analytic modelling of galaxy formation: the local Universe. https://app.cochat.ai/papers/10.1046/j.1365-8711.1999.03032.x
- The paper
- Somerville, R. S., & Primack, J. R. (1999). Semi-analytic modelling of galaxy formation: the local Universe. Monthly Notices of the Royal Astronomical Society. https://doi.org/10.1046/j.1365-8711.1999.03032.x
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.
