Foster, Adam
All People
Staff of Smithsonian Astrophysical Observatory
Background And Education
Research And Grants
co-principal investigator on
investigator on
Publications
selected publications
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article
- Spectral Implications of Atomic Uncertainties in Optically Thin Hot Plasmas 2021
- Atomic data and uncertainties with PyAtomDB 2020
- Comparisons Between Jupiter's X-ray, UV and Radio Emissions and In-Situ Solar Wind Measurements During 2007 2020
- Jupiter's X-ray Emission During the 2007 Solar Minimum 2020
- Plasma Diagnostics of the Supernova Remnant N132D using Deep XMM-Newton Observations with the Reflection Grating Spectrometer 2020
- PyAtomDB: Extending the AtomDB Atomic Database to Model New Plasma Processes and Uncertainties 2020
- EBIT Observation of Ar Dielectronic Recombination Lines near the Unknown Faint X-Ray Feature Found in the Stacked Spectrum of Galaxy Clusters 2019
- Laboratory Measurements of X-Ray Emission from Highly Charged Argon Ions 2019
- Nonequilibrium Ionization in Mixed-morphology Supernova Remnants 2019
- X-Ray Spectra from Plasmas with High-energy Electrons: κ-distributions and e−─e− Bremsstrahlung 2019
- XMM-Newton RGS Spectroscopy of the M31 Bulge. I. Evidence for a Past AGN Half a Million Years Ago 2019
- Chandrasekhar and Sub-Chandrasekhar Models for the X-Ray Emission of Type Ia Supernova Remnants. I. Bulk Properties 2018
- Detection of polarized gamma-ray emission from the Crab nebula with the Hitomi Soft Gamma-ray Detector 2018
- Eigenvalue Method for NEI Unit in FLASH Code 2018
- Evidence for Rapid Adiabatic Cooling as an Origin of the Recombining Plasma in the Supernova Remnant W49B Revealed by NuSTAR Observations 2018
- Searching for the 3.5 keV Line in the Deep Fields with Chandra: The 10 Ms Observations 2018
- Electron-impact single and double ionization of W 2017
- Hitomi Constraints on the 3.5 keV Line in the Perseus Galaxy Cluster 2017
- Numerical Simulations of Supernova Remnant Evolution in a Cloudy Interstellar Medium 2017
- Optimisation and assessment of theoretical impurity line power coefficients relevant to ITER and DEMO 2017
- SNR 1E 0102.2-7219 as an X-ray calibration standard in the 0.5-1.0 keV bandpass and its application to the CCD instruments aboard Chandra, Suzaku, Swift and XMM-Newton 2017
- Radial Profile of the 3.5 keV Line Out to R200 in the Perseus Cluster 2016
- Searching for the 3.5 keV Line in the Stacked Suzaku Observations of Galaxy Clusters 2016
- The quiescent intracluster medium in the core of the Perseus cluster 2016
- A Chandrasekhar Mass Progenitor for the Type Ia Supernova Remnant 3C 397 from the Enhanced Abundances of Nickel and Manganese 2015
- Multi-wavelength Analysis of the Galactic Supernova Remnant MSH 11-61A 2015
- Detection of an Unidentified Emission Line in the Stacked X-Ray Spectrum of Galaxy Clusters 2014
- New Evidence for Efficient Collisionless Heating of Electrons at the Reverse Shock of a Young Supernova Remnant 2014
- Resolving the Origin of the Diffuse Soft X-Ray Background 2014
- Spectral Modeling of the Charge-exchange X-Ray Emission from M82 2014
- Cross-calibration of the x-ray instruments onboard the Chandra, Suzaku, Swift, and XMM- Newton Observatories using the SNR 1E 0102.2-7219 2012
- High-resolution XMM-Newton Spectroscopy of the Cooling Flow Cluster A3112 2012
- The ASTRO-H X-ray Observatory 2012
- Updated Atomic Data and Calculations for X-Ray Spectroscopy 2012
- Fe IX Calculations for the Solar Dynamics Observatory 2011
Other
Location
- Smithsonian Astrophysical Observatory Academic Department
