The DOI matches its Crossref record; 2 of the 2 references it cites were found in a registry or an index.
A catalog of galaxy clusters observed by XMM-Newton
Open accessAbstract
Aims.We present a uniform catalog of the images and radial profiles of the temperature, abundance, and brightness for 70 clusters of galaxies observed by XMM-Newton.
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Citations
Cites
A Universal Density Profile from Hierarchical Clustering
Navarro, J. F., Frenk, C. S., & White, S. D. M. (1997) · The Astrophysical Journal · doi:10.1086/304888 · Cited by 9,917
ROSAT Survey Diffuse X‐Ray Background Maps. II.
Snowden, S. L., Egger, R., Freyberg, M. J., McCammon, D., Plucinsky, P. P., Sanders, W. T., Schmitt, J. H. M. M., Trumper, J., & Voges, W. (1997) · The Astrophysical Journal · doi:10.1086/304399 · Cited by 602 · cited 2×
“7 displays the ROSAT All-Sky Survey (RASS) sky maps in the 14 keV, 3 4 keV, and 1.5 keV band from Snowden et al. (1997).”
BackgroundInfluentialSelf-citation
Cited by
CHANDRA STUDIES OF THE X-RAY GAS PROPERTIES OF GALAXY GROUPS
Sun, M., Voit, G. M., Donahue, M., Jones, C., Forman, W., & Vikhlinin, A. (2009) · The Astrophysical Journal · doi:10.1088/0004-637x/693/2/1142 · Cited by 600
INNOVATIONS IN THE ANALYSIS OF CHANDRA-ACIS OBSERVATIONS
Broos, P. S., Townsley, L. K., Feigelson, E. D., Getman, K. V., Bauer, F. E., & Garmire, G. P. (2010) · The Astrophysical Journal · doi:10.1088/0004-637x/714/2/1582 · Cited by 288
The EPIC-MOS particle-induced background spectra
Kuntz, K. D., & Snowden, S. L. (2008) · Astronomy & Astrophysics · doi:10.1051/0004-6361:20077912 · Cited by 262
Self-citationGlimpses of the past activity of Sgr A★ inferred from X-ray echoes in Sgr C
Chuard, D., Terrier, R., Goldwurm, A., Clavel, M., Soldi, S., Morris, M. R., Ponti, G., Walls, M., & Chernyakova, M. (2018) · Astronomy & Astrophysics · doi:10.1051/0004-6361/201731864 · Cited by 42
On the distance to the North Polar Spur and the local CO-H2factor
Lallement, R., Snowden, S., Kuntz, K. D., Dame, T. M., Koutroumpa, D., Grenier, I., & Casandjian, J. M. (2016) · Astronomy & Astrophysics · doi:10.1051/0004-6361/201629453 · Cited by 32
“The processing of the XMM data (background modeling and subtraction, point source excision, exposure correction) followed the procedures outlined in Snowden et al. (2008) based on the calibration of Kuntz & Snowden (2008).”
MethodSelf-citation
Metadata
- Authors
- Snowden, S. L., Mushotzky, R. F., Kuntz, K. D., & Davis, D. S.
- Venue
- Astronomy & Astrophysics
- Publisher
- EDP Sciences
- Published
- 2007-10-09
- Volume
- 478
- Issue
- 2
- Pages
- 615-658
- ISSN
- 0004-6361 (ISSN-L)
- 1432-0746
- OpenAlex
- W2010438020
- Cited by
- 388
- References
- 2
- FWCI
- 14.09
- Type
- journal article
- Language
- en
- Open access
- green
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- CoChat. (2026). Citation check: A catalog of galaxy clusters observed by XMM-Newton. https://app.cochat.ai/papers/10.1051/0004-6361:20077930
- The paper
- Snowden, S. L., Mushotzky, R. F., Kuntz, K. D., & Davis, D. S. (2008). A catalog of galaxy clusters observed by XMM-Newton. Astronomy & Astrophysics. https://doi.org/10.1051/0004-6361%3A20077930
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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.
