The DOI matches its Crossref record; 9 of the 9 references it cites were found in a registry or an index.
The EPIC-MOS particle-induced background spectra
Open accessAbstract
Context.To analyze diffuse emission that fills the field of view, one must accurately characterize the instrumental backgrounds. For the XMM-Newton EPIC-MOS instrument these backgrounds include a temporally variable “quiescent” component, as well as the strongly variable soft proton contamination.
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Cites
The European Photon Imaging Camera on XMM-Newton: The MOS cameras
Turner, M. J. L., Abbey, A., Arnaud, M., Balasini, M., Barbera, M., Belsole, E., Bennie, P. J., Bernard, J. P., Bignami, G. F., Boer, M., et al. (2001) · Astronomy & Astrophysics · doi:10.1051/0004-6361:20000087 · Cited by 2,351
Hydromagnetic flow around the magnetosphere
Spreiter, J. R., Summers, A. L., & Alksne, A. Y. (1966) · Planetary and Space Science · doi:10.1016/0032-0633(66)90124-3 · Cited by 945
A catalog of galaxy clusters observed by XMM-Newton
Snowden, S. L., Mushotzky, R. F., Kuntz, K. D., & Davis, D. S. (2008) · Astronomy & Astrophysics · doi:10.1051/0004-6361:20077930 · Cited by 388
Self-citationX-ray background measurements with XMM-Newton EPIC
Lumb, D. H., Warwick, R. S., Page, M., & De Luca, A. (2002) · Astronomy & Astrophysics · doi:10.1051/0004-6361:20020531 · Cited by 386
XMM‐Newton Observation of Solar Wind Charge Exchange Emission
Snowden, S. L., Collier, M. R., & Kuntz, K. D. (2004) · The Astrophysical Journal · doi:10.1086/421841 · Cited by 270
Self-citationASCA and ROSAT observations of the QSF3 field: the X-ray background in the 0.1-7 keV band
Chen, L. W., Fabian, A. C., & Gendreau, K. C. (1997) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/285.3.449 · Cited by 105
Charge-transfer induced EUV and soft X-ray emissions in the heliosphere
Koutroumpa, D., Lallement, R., Kharchenko, V., Dalgarno, A., Pepino, R., Izmodenov, V., & Quémerais, É. (2006) · Astronomy and Astrophysics · doi:10.1051/0004-6361:20065250 · Cited by 104
XMM‐NewtonEPIC Background Modeling for Extended Sources
Nevalainen, J., Markevitch, M. L., & Lumb, D. (2005) · The Astrophysical Journal · doi:10.1086/431198 · Cited by 83
Charge-Transfer induced EUV and Soft X-ray emissions in the Heliosphere
Koutroumpa, D., Lallement, R., Kharchenko, V. A., Dalgarno, A., Pepino, R. T., Измоденов, В. В., & Quémerais, É. (2006) · Springer Link (Chiba Institute of Technology) · doi:10.1051/0004-6361:20065250/pdf · Cited by 59
Cited by
Unidentified Line in X-Ray Spectra of the Andromeda Galaxy and Perseus Galaxy Cluster
Boyarsky, A., Ruchayskiy, O., Iakubovskyi, D., & Franse, J. (2014) · Physical Review Letters · doi:10.1103/physrevlett.113.251301 · Cited by 686
CONSTRAINING THE MILKY WAY'S HOT GAS HALO WITH O VII AND O VIII EMISSION LINES
Miller, M. J., & Bregman, J. N. (2015) · The Astrophysical Journal · doi:10.1088/0004-637x/800/1/14 · Cited by 273
The XMM–Newton view of the central degrees of the Milky Way
Ponti, G., Morris, M. R., Terrier, R., Haberl, F., Sturm, R., Clavel, M., Soldi, S., Goldwurm, A., Predehl, P., Nandra, K., et al. (2015) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stv1331 · Cited by 125
AN XMM-NEWTON SURVEY OF THE SOFT X-RAY BACKGROUND. III. THE GALACTIC HALO X-RAY EMISSION
Henley, D. B., & Shelton, R. L. (2013) · The Astrophysical Journal · doi:10.1088/0004-637x/773/2/92 · Cited by 116
THE INTERACTION OF THE FERMI BUBBLES WITH THE MILKY WAY’S HOT GAS HALO
Miller, M. J., & Bregman, J. N. (2016) · The Astrophysical Journal · doi:10.3847/0004-637x/829/1/9 · Cited by 91
Metadata
- Authors
- Kuntz, K. D., & Snowden, S. L.
- Venue
- Astronomy & Astrophysics
- Publisher
- EDP Sciences
- Published
- 2007-12-04
- Volume
- 478
- Issue
- 2
- Pages
- 575-596
- ISSN
- 0004-6361 (ISSN-L)
- 1432-0746
- OpenAlex
- W2082316064
- Cited by
- 262
- References
- 9
- FWCI
- 8.04
- Type
- journal article
- Language
- en
- Open access
- bronze
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Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).
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