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1. More data than you want, fewer data than you need: machine learning approaches to starlight subtraction with MagAO-X

2. On-sky, real-time optical gain calibration on MagAO-X using incoherent speckles

3. Emerging adaptive optics facility at Large Binocular Telescope Observatory

5. SHARK-NIR commissioning and early science runs

6. Innovations in the design and construction of the GMT-Consortium Large Earth Finder (G-CLEF), a first-light instrument for the Giant Magellan Telescope (GMT)

8. Approaches to lowering the cost of large space telescopes

10. XPipeline: starlight subtraction at scale for MagAO-X

14. Integration and test of the natural guide star wavefront sensor prototype for the Giant Magellan Telescope: the pyramid sensor

15. Adaptive optics development at the Giant Magellan Telescope: recent progress

16. High-contrast imaging at first-light of the GMT: the PDR optical and mechanical design for the GMagAO-X ExAO system and results from the HCAT testbed with an HDFS phased parallel DM prototype

17. The Giant Magellan Telescope’s high contrast adaptive optics testbed: NGAO wavefront sensing and control laboratory results

18. Challenge of direct imaging of exoplanets within structures: disentangling real signal from point source from background light

19. MagAO-X: commissioning results and status of ongoing upgrades

24. Approaches to lowering the cost of large space telescopes.

25. Multi-core fibre-fed integral-field unit (MCIFU): overview and first-light

26. MagAO-X first light

28. SHARK-NIR, toward the installation at the Large Binocular Telescope

29. Prediction of the planet yield of the MaxProtoPlanetS high-contrast survey for H-alpha protoplanets with MagAO-X based on first light contrasts

36. SHARK-NIR: the coronagraphic camera for LBT in the AIV phase at INAF-Padova

38. Modeling coronagraphic extreme wavefront control systems for high contrast imaging in ground and space telescope missions

46. Opto-mechanical designs for the HARMONI adaptive optics systems

47. Extending the pyramid WFS to LGSs: the INGOT WFS

48. NFIRAOS adaptive optics for the Thirty Meter Telescope

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