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Browsing by Author "Bautz, Mark W."

Browsing by Author "Bautz, Mark W."

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  • Characterization of the Particle-induced Background of XMM-Newton EPIC-pn: Short- and Long-term Variability 
    Bulbul, Esra; Kraft, Ralph; Nulsen, Paul; Freyberg, Michael; Miller, Eric D.; Grant, Catherine; Bautz, Mark W.; Burrows, David N.; Allen, Steven; Eraerds, Tanja; Fioretti, Valentina; Gastaldello, Fabio; Ghirardini, Vittorio; Hall, David; Meidinger, Norbert; Molendi, Silvano; Rau, Arne; Wilkins, Dan; Wilms, Joern (2020)
    The particle-induced background of X-ray observatories is produced by galactic cosmic ray (GCR) primary protons, electrons, and He ions. Events due to direct interaction with the detector are usually removed by onboard ...
  • Laboratory Measurements of X-Ray Emission from Highly Charged Argon Ions 
    Bulbul, Esra; Foster, Adam; Brown, Gregory V.; Bautz, Mark W.; Beiersdorfer, Peter; Hell, Natalie; Kilbourne, Caroline; Kraft, Ralph; Kelley, Richard; Leutenegger, Maurice A.; Miller, Eric D.; Porter, F. Scott; Smith, Randall K. (2019)
    Uncertainties in atomic models will introduce noticeable additional systematics in calculating the flux of weak dielectronic recombination (DR) satellite lines, affecting the detection and flux measurements of other weak ...
  • Searching for the 3.5 keV Line in the Deep Fields with Chandra: The 10 Ms Observations 
    Cappelluti, Nico; Bulbul, Esra; Foster, Adam; Natarajan, Priyamvada; Urry, Megan C.; Bautz, Mark W.; Civano, Francesca; Miller, Eric; Smith, Randall K. (2018)
    We report a systematic search for an emission line around 3.5 keV in the spectrum of the cosmic X-ray background using a total of ~10 Ms Chandra observations toward the COSMOS Legacy and Extended Chandra Deep Field South ...
  • A Very Deep Chandra Observation of A1795: The Cold Front and Cooling Wake 
    Ehlert, Steven; McDonald, Michael; David, Laurence P.; Miller, Eric D.; Bautz, Mark W. (2015)
    We present a new analysis of very deep Chandra observations of the galaxy cluster A1795. Utilizing nearly 750 ks of net ACIS imaging, we are able to resolve the thermodynamic structure of the intracluster medium (ICM) on ...
  • X-Ray Properties of SPT-selected Galaxy Clusters at 0.2 < z < 1.5 Observed with XMM-Newton 
    Bulbul, Esra; Chiu, I. -Non; Mohr, Joseph J.; McDonald, Michael; Benson, Bradford; Bautz, Mark W.; Bayliss, Matthew; Bleem, Lindsey; Brodwin, Mark; Bocquet, Sebastian; Capasso, Raffaella; Dietrich, Jörg P.; Forman, Bill; Hlavacek-Larrondo, Julie; Holzapfel, W. L.; Khullar, Gourav; Klein, Matthias; Kraft, Ralph; Miller, Eric D.; Reichardt, Christian; Saro, Alex; Sharon, Keren; Stalder, Brian; Schrabback, Tim; Stanford, Adam (2019)
    We present measurements of the X-ray observables of the intracluster medium (ICM), including luminosity L <SUB> X </SUB>, ICM mass M <SUB>ICM</SUB>, emission-weighted mean temperature T <SUB> X </SUB>, and integrated ...

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