Bayesian insights into the Tycho supernova remnant: A detailed mapping of ejecta properties. By Leila Godinaud | @univparissaclay.bsky.social , @cea.fr, @cnrs-paris-saclay.bsky.social.
🔗https://www.the-athena-x-ray-observatory.eu/en/node/900
Bayesian insights into the Tycho supernova remnant: A detailed mapping of ejecta properties. By Leila Godinaud | @univparissaclay.bsky.social , @cea.fr, @cnrs-paris-saclay.bsky.social.
🔗https://www.the-athena-x-ray-observatory.eu/en/node/900
Vander Meulen, Hu, Grinberg & Krawczynski (A&A submitted): "Predictions for the X-ray polarisation modulation in Cygnus X-1 from reflection off the stellar companion and its wind"
-- we set up a radiative transfer model combining a general […]
[Original post on mastodon.social]
Vander Meulen, Hu, Grinberg & Krawczynski (A&A submitted): "Predictions for the X-ray polarisation modulation in Cygnus X-1 from reflection off the stellar companion and its wind"
-- we set up a radiative transfer model combining a general […]
[Original post on mastodon.social]
✏️ Summary of the paper: Cooling rate and turbulence in the intracluster medium of the cool-core cluster Abell 2667. By Marika Lepore | INAF-Osservatorio Astrofisico di Arcetri.
🔗https://www.the-athena-x-ray-observatory.eu/en/node/901
✏️ Summary of the paper: Cooling rate and turbulence in the intracluster medium of the cool-core cluster Abell 2667. By Marika Lepore | INAF-Osservatorio Astrofisico di Arcetri.
🔗https://www.the-athena-x-ray-observatory.eu/en/node/901
✏️ Summary of the paper: Modelling absorption and emission profiles from accretion disc winds with WINE , by A. Luminari, INAF - Istituto di Astrofisica e Planetologia Spaziali (IAPS).
🔗 www.the-athena-x-ray-observatory.eu/es/node/873
✏️ Summary of the paper: Modelling absorption and emission profiles from accretion disc winds with WINE , by A. Luminari, INAF - Istituto di Astrofisica e Planetologia Spaziali (IAPS).
🔗 www.the-athena-x-ray-observatory.eu/es/node/873
✏️ Summary of the paper: About the accuracy of the relxill/relxill_nk models in view of the next generation of X-ray missions. By Honghui Liu | Fudan University.
🔗 www.the-athena-x-ray-observatory.eu/es/node/887
✏️ Summary of the paper: About the accuracy of the relxill/relxill_nk models in view of the next generation of X-ray missions. By Honghui Liu | Fudan University.
🔗 www.the-athena-x-ray-observatory.eu/es/node/887
✏️ Summary of the paper: Benefits of the Use of Monte Carlo Simulations in Cryogenic Detector Design. By S. Lotti | INAF - Istituto di Astrofisica e Planetologia Spaziali (IAPS).
🔗 www.the-athena-x-ray-observatory.eu/en/node/898
✏️ Summary of the paper: Benefits of the Use of Monte Carlo Simulations in Cryogenic Detector Design. By S. Lotti | INAF - Istituto di Astrofisica e Planetologia Spaziali (IAPS).
🔗 www.the-athena-x-ray-observatory.eu/en/node/898
✏️ Summary: The Athena proton response matrix encodes the soft proton transmission into RMF and ARF files to quickly simulate the soft proton background with Xspec, by V. Fioretti and T. Mineo, INAF
🔗 www.the-athena-x-ray-observatory.eu/es/node/879
✏️ Summary: The Athena proton response matrix encodes the soft proton transmission into RMF and ARF files to quickly simulate the soft proton background with Xspec, by V. Fioretti and T. Mineo, INAF
🔗 www.the-athena-x-ray-observatory.eu/es/node/879
✏️ Summary of the paper: Detection of a Highly Ionized Outflow in the Quasiperiodically Erupting Source GSN 069. By Peter Kosec / Smithsonian Astrophysical Observatory.
🔗 www.the-athena-x-ray-observatory.eu/es/node/886
✏️ Summary of the paper: Detection of a Highly Ionized Outflow in the Quasiperiodically Erupting Source GSN 069. By Peter Kosec / Smithsonian Astrophysical Observatory.
🔗 www.the-athena-x-ray-observatory.eu/es/node/886