Bringing #NewAthenaScience #NewAthenaPapers #Papertime!
✏️ 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
April 10, 2025 at 12:44 PM
Bringing #NewAthenaScience #NewAthenaPapers #Papertime!
✏️ 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
Bringing #NewAthenaScience #NewAthenaPapers #Papertime!
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
March 31, 2025 at 10:43 AM
Bringing #NewAthenaScience #NewAthenaPapers #Papertime!
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
Bringing #NewAthenaScience #NewAthenaPapers #Papertime!
✏️ 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
March 13, 2025 at 5:32 PM
Bringing #NewAthenaScience #NewAthenaPapers #Papertime!
✏️ 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
Bringing #NewAthenaScience #NewAthenaPapers #Papertime!
✏️ 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
February 27, 2025 at 1:16 PM
Bringing #NewAthenaScience #NewAthenaPapers #Papertime!
✏️ 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
Bringing #NewAthenaScience #NewAthenaPapers #Papertime!
✏️ 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
February 25, 2025 at 10:57 AM
Bringing #NewAthenaScience #NewAthenaPapers #Papertime!
✏️ 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
#NewAthenaScience #NewAthenaPapers #Papertime!
✏️ 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
January 28, 2025 at 1:33 PM
#NewAthenaScience #NewAthenaPapers #Papertime!
✏️ 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
Bringing #NewAthenaScience #NewAthenaPapers #Papertime!
✏️ 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
January 14, 2025 at 11:40 AM
Bringing #NewAthenaScience #NewAthenaPapers #Papertime!
✏️ 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