The EPIC-MOS particle-induced background spectra

By K. Kuntz, S. Snowden. 2008

198 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics

View Paper: https://www.semanticscholar.org/paper/ec1449060e593a1a9b36e301362559b01ef46196

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In Astronomy and Astrophysics

1. M. Miller
2. J. Bregman
3. H. Böhringer
4. S. Randall
5. M. Markevitch
6. L. Lovisari
7. G. Schellenberger
8. T. Reiprich

In Nuclear and High Energy Physics

1. G. Schellenberger
2. T. Reiprich
3. L. Lovisari
4. J. Bregman
5. O. Urban
6. Steven W. Allen
7. Norbert Werner
8. A. Simionescu

Citations in the corpus

• Scaling Properties of a Complete X-ray Selected Galaxy Group Sample (2014, background): “All these different components exhibit different spectral and temporal characteristics (e.g., Lumb et al. 2002; Read & Ponman 2003; Kuntz & Snowden 2008; Snowden et al. 2008).”
• DETECTION OF AN UNIDENTIFIED EMISSION LINE IN THE STACKED X-RAY SPECTRUM OF GALAXY CLUSTERS (2014, methodology): “Since small variations in the gain and the line strengths between the source and background spectra can lead to residuals in the spectral fitting (Kuntz & Snowden 2008) and XMM-ESAS software does not include these instrumental lines in the QPB spectra, we modeled these instrumental lines spectrally ”
• X-ray spectroscopy of the Virgo Cluster out to the virial radius (2011, methodology): “The filtering and extraction of the MOS data products and the subtraction of their instrumental background was performed using the XMM-Newton Extended Source Analysis Software (XMM-ESAS) and methods described in Kuntz & Snowden (2008); Snowden et al. (2008); Snowden & Kuntz (2010).”
• CONSTRAINING THE MILKY WAY'S HOT GAS HALO WITH O vii AND O viii EMISSION LINES (2014, methodology): “Data Filtering The 5698 archival XMM-Newton observations were processed with the standardXMM-Newton Science Analysis System 1 version 11.0.1, including the XMM-Newton Extended Source Analysis Software 2 (XMM -ESAS; Kuntz & Snowden 2008; Snowden & Kuntz 2011).”
• Probing cosmic isotropy with a new X-ray galaxy cluster sample through the LX–T scaling relation (2020, unknown): “In a nutshell, every observation was treated for solar flares, anomalous state of CCDs (Kuntz & Snowden 2008), instrumental background and exposure correction.”