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2024 Astrophysics Biennial Technology Report Web Release

4 October 2024

The COR, ExEP, and PhysCOS Program Office technologists are happy to announce that the 2024 Astrophysics Biennial Technology Report (ABTR) is now available for downloading. The ABTR includes messages from Dr. Mark Clampin, Astrophysics Division Director and Dr. Mario Perez, Astrophysics Division Chief Technologist; a list of 12 new Strategic Astrophysics Technology (SAT) grants awarded in the most recent cycle; updated technology development statistics and portfolios; the 2024 combined Strategic Astrophysics Technology Gaps List of 61 gaps; updated technology infusion lists; descriptions of Astrophysics-Division-funded technology development and test facilities, and technology development project highlights.

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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.