The DOI matches its Crossref record; 14 of the 14 references it cites were found in a registry or an index.
MOJAVE. XV. VLBA 15 GHz Total Intensity and Polarization Maps of 437 Parsec-scale AGN Jets from 1996 to 2017
Open accessAbstract
We present 5321 mas-resolution total intensity and linear polarization maps of 437 active galactic nuclei (AGNs) obtained with the VLBA at 15 GHz as part of the MOJAVE survey, and also from the NRAO data archive. The former is a long-term program to study the structure and evolution of powerful parsec-scale outflows associated with AGNs. The targeted AGNs are drawn from several flux-limited radio and γ-ray samples, and all have correlated VLBA flux densities greater than ∼50 mJy at 15 GHz. Approximately 80% of these AGNs are associated with γ-ray sources detected by the Fermi LAT instrument. The vast majority were observed with the VLBA on 5–15 occasions between 1996 January 19 and 2016 December 26, at intervals ranging from a month to several years, with the most typical sampling interval being six months. A detailed analysis of the linear and circular polarization evolutions of these AGN jets is presented in the other papers in this series.
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
Observational Evidence of Active Galactic Nuclei Feedback
Fabian, A. C. (2012) · Annual Review of Astronomy and Astrophysics · doi:10.1146/annurev-astro-081811-125521 · Cited by 2,795
The Third EGRET Catalog of High-Energy Gamma-Ray Sources
Chen, A. W., Michelson, P. F., Thompson, D. J., et al. (1998) · NASA Technical Reports Server (NASA) · Cited by 1,670
FERMI LARGE AREA TELESCOPE THIRD SOURCE CATALOG
Acero, F., Ackermann, M., Ajello, M., Albert, A., Atwood, W. B., Axelsson, M., Baldini, L., Ballet, J., Barbiellini, G., Bastieri, D., et al. (2015) · The Astrophysical Journal Supplement Series · doi:10.1088/0067-0049/218/2/23 · Cited by 1,461
Heckman, T. M., & Best, P. N. (2014) · Annual Review of Astronomy and Astrophysics · doi:10.1146/annurev-astro-081913-035722 · Cited by 1,271
FERMI LARGE AREA TELESCOPE FIRST SOURCE CATALOG
Abdo, A. A., Ackermann, M., Ajello, M., Allafort, A., Antolini, E., Atwood, W. B., Axelsson, M., Baldini, L., Ballet, J., Barbiellini, G., et al. (2010) · The Astrophysical Journal Supplement Series · doi:10.1088/0067-0049/188/2/405 · Cited by 1,262
THE SECOND CATALOG OF ACTIVE GALACTIC NUCLEI DETECTED BY THE FERMI LARGE AREA TELESCOPE
Ackermann, M., Ajello, M., Allafort, A., Antolini, E., Atwood, W. B., Axelsson, M., Baldini, L., Ballet, J., Barbiellini, G., Bastieri, D., et al. (2011) · The Astrophysical Journal · doi:10.1088/0004-637x/743/2/171 · Cited by 651
The linear polarization of quasi-stellar radio sources at 3.71 and 11.1 centimeters
Wardle, J. F. C., & Kronberg, P. P. (1974) · The Astrophysical Journal · doi:10.1086/153240 · Cited by 603
THE THIRD CATALOG OF ACTIVE GALACTIC NUCLEI DETECTED BY THE FERMI LARGE AREA TELESCOPE
Ackermann, M., Ajello, M., Atwood, W. B., Baldini, L., Ballet, J., Barbiellini, G., Bastieri, D., Gonzalez, J. B., Bellazzini, R., Bissaldi, E., et al. (2015) · The Astrophysical Journal · doi:10.1088/0004-637x/810/1/14 · Cited by 512
DiFX-2: A More Flexible, Efficient, Robust, and Powerful Software Correlator
Deller, A. T., Brisken, W. F., Phillips, C. J., Morgan, J., Alef, W., Cappallo, R., Middelberg, E., Romney, J., Rottmann, H., Tingay, S. J., et al. (2011) · Publications of the Astronomical Society of the Pacific · doi:10.1086/658907 · Cited by 511
Lister, M. L., & Homan, D. C. (2005) · The Astronomical Journal · doi:10.1086/432969 · Cited by 339
Self-citation
Cited by
First M87 Event Horizon Telescope Results. I. The Shadow of the Supermassive Black Hole
The Event Horizon Telescope Collaboration, Akiyama, K., Alberdi, A., Alef, W., Asada, K., Azulay, R., Baczko, A.-K., Ball, D., Baloković, M., Barrett, J., et al. (2019) · The Astrophysical Journal Letters · doi:10.3847/2041-8213/ab0ec7 · Cited by 4,205
Self-citationBroderick, A. E., Gold, R., Georgiev, B., Pesce, D. W., Tiede, P., Ni, C., Moriyama, K., Akiyama, K., Alberdi, A., Alef, W., et al. (2022) · The Astrophysical Journal Letters · doi:10.3847/2041-8213/ac6584 · Cited by 38
Self-citation
Metadata
- Authors
- Lister, M. L., Aller, M. F., Aller, H. D., Hodge, M. A., Homan, D. C., Kovalev, Y. Y., Pushkarev, A. B., & Savolainen, T.
- Venue
- The Astrophysical Journal Supplement Series
- Publisher
- American Astronomical Society
- Published
- 2018-01-01
- Volume
- 234
- Issue
- 1
- Pages
- 12
- ISSN
- 0067-0049 (ISSN-L)
- 1538-4365
- OpenAlex
- W2768671855
- Cited by
- 299
- References
- 14
- FWCI
- 15.98
- 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: MOJAVE. XV. VLBA 15 GHz Total Intensity and Polarization Maps of 437 Parsec-scale AGN Jets from 1996 to 2017. https://app.cochat.ai/papers/10.3847/1538-4365/aa9c44
- The paper
- Lister, M. L., Aller, M. F., Aller, H. D., Hodge, M. A., Homan, D. C., Kovalev, Y. Y., Pushkarev, A. B., & Savolainen, T. (2018). MOJAVE. XV. VLBA 15 GHz Total Intensity and Polarization Maps of 437 Parsec-scale AGN Jets from 1996 to 2017. The Astrophysical Journal Supplement Series. https://doi.org/10.3847/1538-4365/aa9c44
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.
