Suggested Searches

 

The 248th Meeting of the American Astronomical Society

Physics of the Cosmos about The 248th Meeting of the American Astronomical Society

Location

Pasadena, California

Dates

14-18 June 2026

Community

Physics of the Cosmos

Type

Meeting

AAS Meeting 248

Joint AAS with HEAD and Laboratory Astrophysics Divisions Meeting

14-18 June 2026 at the Pasadena Convention Center

Meeting Overview about Joint AAS with HEAD and Laboratory Astrophysics Divisions Meeting
Pasadena Convention Center

Monday, 15 June 2026

TimeSessionLocation
10:00am ‑ 11:30am PTNASA’s Future Large Gamma Ray (FLAG) Mission Concepts Working GroupPasadena Convention Center ‑  
Conference Center, 204
SummaryThe Future Large Gamma-ray Mission Concepts working group will hold a hybrid work session to review progress and needed inputs for a technical report on gamma-ray instrumentation. Working group members will present updates and lead discussions to complete gathering of input on gamma-ray capabilities, mission concepts, and technologies. The group will work on identifying and filling gaps in the draft and refining the content of the report.

Wednesday, 17 June 2026

TimeSessionLocation
11:40am ‑ 1:10pm PTXR SIG Special SessionPasadena Convention Center ‑ 
Conference Center, 211

XR SIG Special Session Agenda

Session TitleHEAD: Toward the 2030 Decadal: Science Cases for Potential Future X-ray Mission Concepts
Session ChairBreanna Binder
SummaryThis special session will present outcomes from four X-ray Science Interest Group (XRSIG)-led Science Analysis Groups (SAGs) convened to evaluate potential future X-ray mission concepts and their scientific return. Over the past ~year, the SAGs conducted an initial exploration of science enabled by four candidate mission architectures: (1) a Lynx-like observatory concept with potential augmentations, (2) an ultra-high angular resolution X-ray interferometer mission, (3) a mission spanning a substantially broader energy band than would be feasible for a Lynx-like design, and (4) a dedicated X-ray timing mission concept. In this session, we will summarize the scope, activities, and key findings of each SAG, highlighting representative science cases, capability-driven requirements, and points of convergence and differentiation across the architectures. We will also review relevant technology developments identified by the SAGs that could improve mission feasibility and inform community discussions as planning proceeds toward the next Decadal Survey.

News Straight to Your Inbox

Subscribe to your community email news list

We will never share your email address.

Privacy Policy

Sign Up
This cropped horizontal image has layers of semi-opaque rusty red colored gas and dust that starts at the bottom right and goes toward the top left. There are three prominent pillars rising toward the top left. The left pillar is the largest and widest. The peaks of the second and third pillars are set off in darker shades of brown and have red outlines.