The DOI matches its Crossref record; 54 of the 54 references it cites were found in a registry or an index.
Evidence for mature bulges and an inside-out quenching phase 3 billion years after the Big Bang
Open accessAbstract
Eat your heart out, old galaxies: Most galaxies exceeding 100 billion solar masses are dense spheroids that exhibit no star-forming activity in the present day. Nevertheless, galaxies of the same size were actively forming stars when the universe was only a few billion years old. Tacchella et al. used integral-field spectroscopy and high-resolution imaging to map the distributions of star formation rates and stellar mass densities within ancient galaxies. Star formation apparently quenched first in the center, while remaining lively in the galactic outskirts, with quenching taking a few billion years to proceed outward. Science , this issue p. 314
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
Stellar population synthesis at the resolution of 2003
Bruzual, G., & Charlot, S. (2003) · Monthly Notices of the Royal Astronomical Society · doi:10.1046/j.1365-8711.2003.06897.x · Cited by 10,500
The Sloan Digital Sky Survey: Technical Summary
York, D. G., Adelman, J., Anderson, Jr., Anderson, S. F., Annis, J., Bahcall, N. A., Bakken, J. A., Barkhouser, R., Bastian, S., Berman, E., et al. (2000) · The Astronomical Journal · doi:10.1086/301513 · Cited by 10,366
Galactic Stellar and Substellar Initial Mass Function
Chabrier, G. (2003) · Publications of the Astronomical Society of the Pacific · doi:10.1086/376392 · Cited by 9,071
STAR FORMATION IN GALAXIES ALONG THE HUBBLE SEQUENCE
Kennicutt, R. C. (1998) · Annual Review of Astronomy and Astrophysics · doi:10.1146/annurev.astro.36.1.189 · Cited by 6,578
The Dust Content and Opacity of Actively Star‐forming Galaxies
Calzetti, D., Armus, L., Bohlin, R. C., Kinney, A. L., Koornneef, J., & Storchi‐Bergmann, T. (2000) · The Astrophysical Journal · doi:10.1086/308692 · Cited by 5,717
NINE-YEAR WILKINSON MICROWAVE ANISOTROPY PROBE ( WMAP ) OBSERVATIONS: COSMOLOGICAL PARAMETER RESULTS
Hinshaw, G., Larson, D., Komatsu, E., Spergel, D. N., Bennett, C. L., Dunkley, J., Nolta, M. R., Halpern, M., Hill, R. S., Odegard, N., et al. (2013) · The Astrophysical Journal Supplement Series · doi:10.1088/0067-0049/208/2/19 · Cited by 5,121
Galactic Stellar and Substellar Initial Mass FunctionPreprint
Chabrier, G. (2003) · Cited by 4,970
Star Formation in Galaxies Along the Hubble Sequence
Kennicutt, R. C., & Words, K. (1998) · Cited by 3,712
Astrophysics of Gaseous Nebulae and Active Galactic Nuclei
Osterbrock, D. E., & Michael Shull, J. (1989) · Physics Today · doi:10.1063/1.2811187 · Cited by 3,699
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
Cited by
Cool outflows in galaxies and their implications
Veilleux, S., Maiolino, R., Bolatto, A. D., & Aalto, S. (2020) · The Astronomy and Astrophysics Review · doi:10.1007/s00159-019-0121-9 · Cited by 466
Davidzon, I., Ilbert, O., Laigle, C., Coupon, J., McCracken, H. J., Delvecchio, I., Masters, D., Capak, P., Hsieh, B. C., Le Fèvre, O., et al. (2017) · Astronomy & Astrophysics · doi:10.1051/0004-6361/201730419 · Cited by 420
A unified model for galactic discs: star formation, turbulence driving, and mass transport
Krumholz, M. R., Burkhart, B., Forbes, J. C., & Crocker, R. M. (2018) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/sty852 · Cited by 319
FORMING COMPACT MASSIVE GALAXIES
van Dokkum, P. G., Nelson, E. J., Franx, M., Oesch, P., Momcheva, I., Brammer, G., Schreiber, N. M. F., Skelton, R. E., Whitaker, K. E., Wel, A. V. D., et al. (2015) · The Astrophysical Journal · doi:10.1088/0004-637x/813/1/23 · Cited by 311
Self-citationEvolution of density profiles in high-z galaxies: compaction and quenching inside-out
Tacchella, S., Dekel, A., Carollo, C. M., Ceverino, D., DeGraf, C., Lapiner, S., Mandelker, N., & Primack, J. R. (2016) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stw303 · Cited by 293
Self-citation
Metadata
- Authors
- Tacchella, S., Carollo, C. M., Renzini, A., Schreiber, N. M. F., Lang, P., Wuyts, S., Cresci, G., Dekel, A., Genzel, R., Lilly, S. J., Mancini, C., Newman, S., Onodera, M., Shapley, A., Tacconi, L., Woo, J., & Zamorani, G.
- Venue
- Science
- Published
- 2015-04-17
- Volume
- 348
- Issue
- 6232
- Pages
- 314-317
- ISSN
- 0036-8075 (ISSN-L)
- 1095-9203
- OpenAlex
- W2158012372
- Cited by
- 310
- References
- 54
- FWCI
- 21.80
- Type
- journal article
- Language
- en
- Open access
- green
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: Evidence for mature bulges and an inside-out quenching phase 3 billion years after the Big Bang. https://app.cochat.ai/papers/10.1126/science.1261094
- The paper
- Tacchella, S., Carollo, C. M., Renzini, A., Schreiber, N. M. F., Lang, P., Wuyts, S., Cresci, G., Dekel, A., Genzel, R., Lilly, S. J., Mancini, C., Newman, S., Onodera, M., Shapley, A., Tacconi, L., Woo, J., & Zamorani, G. (2015). Evidence for mature bulges and an inside-out quenching phase 3 billion years after the Big Bang. Science. https://doi.org/10.1126/science.1261094
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.