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AXIS Community Science Conference 14 – 16 May 2025 in Annapolis, MD

25 April 2025

The AXIS (Advanced X-Ray Imaging Satellite) Community Science Conference will be held at The Graduate Hotel in Annapolis, Maryland, on 14 – 16 May 2025. A welcome reception will be held in the evening on Wednesday, 14th May.

Registration and hotel block can be accessed on this webpage. Early-bird registration and abstracts are due by 24 April 2025. Regular online registration is possible until 5 May 2025.

AXIS is the next-generation X-ray imaging observatory, delivering arcsecond-resolution imaging and high sensitivity in the 0.3–10 keV energy band. AXIS is an excellent facility for transient science, with ~hour response time to alerts and onboard rapid transient detection. Further, AXIS will be a powerful and synergistic addition to JWST, Roman, Rubin, ngVLA, LISA, and other major facilities of the 2030s. Importantly, >70% of AXIS observing time will be open to the community through a competitive Guest Observer program, making it a truly community-driven facility.

This conference will focus on the community science enabled by AXIS, the evolving landscape of US astronomy in which AXIS will be operating, and a celebration of the achievements of our precursor flagships Chandra and XMM. We invite all members of the astrophysics community to celebrate the 25 years of Chandra and XMM, and to discuss the future potential of X-ray astronomy with AXIS. This is a chance to help shape the science case and community engagement for AXIS. We especially encourage participation by early-career researchers!

The topics discussed will include:

  • Current status of the AXIS project
  • Legacy of Chandra and XMM
  • The Future of US Astronomy (and the Evolving Landscape)
  • Supermassive black holes: seeding, growth, and feedback
  • Stellar activity and exoplanet environments
  • Compact objects and remnants
  • Time-domain and multi-messenger astronomy; LISA synergies
  • Coordination with next-decade observatories (JWST, Rubin, Roman, ngVLA, LISA, and more)

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An illustration of Sun-like star HD 181327 and its surrounding debris disk. The star is at top right. It is surrounded by a far larger debris disk that forms an incomplete ellpitical path and is cut off at right. There’s a huge cavity between the star and the disk. The debris disk is shown in shades of light gray. Toward the top and left, there are finer, more discrete points in a range of sizes. The disk appears hazier and smokier at the bottom. The star is bright white at center, with a hazy blue region around it. The background of space is black. The label Artist's Concept appears at lower left.