![]() We describe two ExAO optical system designs, one each for ground-based telescopes and space-based missions, and examine them using the angular spectrum Fresnel propagation module within the Physical Optics Propagation in Python (POPPY) package. The challenges of high contrast imaging (HCI) for detecting exoplanets for both ground and space applications can be met with extreme adaptive optics (ExAO), a high-order adaptive optics system that performs wavefront sensing (WFS) and correction at high speed. When these Phase II upgrades are complete we plan to conduct a survey of nearby exoplanets in reflected light. These upgrades include a new post-AO 1000-actuator deformable mirror inside the coronagraph, latest generation sCMOS detectors for wavefront sensing, optimized PIAACMC coronagraphs, and computing system upgrades. Finally, we will present the status of a comprehensive upgrade to MagAO-X to enable extreme-contrast characterization of exoplanets in reflected light. We will provide an overview of these projects, and report the results of our commissioning and science run in April, 2022. MagAO-X also serves as the AO system for the Giant Magellan Telescope High Contrast Adaptive Optics Testbed. Highlights include implementation of several focal plane and low-order wavefront sensing algorithms, development of a new predictive control algorithm, and the addition of an IFU module. In the interim, MagAO-X has served as a lab testbed. First light was in Dec, 2019, but subsequent commissioning runs were canceled due to COVID-19. Our primary science goals are detection and characterization of Solar System-like exoplanets, ranging from very young, still-accreting planets detected at H-alpha, to older temperate planets which will be characterized using reflected starlight. MagAO-X is optimized for high contrast imaging at visible wavelengths. Learn more about this subject by checking out the additional resources listed below.We present a status update for MagAO-X, a 2000 actuator, 3.6 kHz adaptive optics and coronagraph system for the Magellan Clay 6.5 m telescope. To exit Dynamic Mirror mode, deselect the Dynamic Mirror icon. Add some holes on either side of the centerline. Of course, geometry does not have to be connected to the centerline. SOLIDWORKS creates another single line here. Sketch another horizontal line and stop at the centerline to create the rectangle. Sketch another vertical line down from the horizontal line endpoint. SOLIDWORKS creates a single line across the centerline instead of two connected lines. Start sketching a horizontal line from the centerline to the left. This indicates Dynamic Mirror Mode is active. Notice two perpendicular lines above and below the selected centerline. To use a Dynamic Mirror entity, a 2D sketch only needs a centerline or model edge to mirror about. Dynamic Mirror can be added to the toolbar by searching for the command and dragging over the icon.Where to find Dynamic Mirror Entities in SOLIDWORKS: Then, window-select the entities to be mirrored.Ĭlick the Mirror about box to activate, then select the centerline.Ī preview will appear. Ĭlick in the Entities to mirror box to activate it. Click Mirror Entities on the Sketch Toolbar. With Mirror Entities, a 2D sketch must first have sketch entities to mirror and a centerline to mirror about. Click Mirror Entities on the Sketch Toolbar.Where to find Mirror Entities in SOLIDWORKS : With Dynamic Mirror Entities, geometry can be sketched and mirrored simultaneously. Mirror Entities allows a user to mirror their sketches about a common centerline after the sketch has been created. SOLIDWORKS Mirror Entities and Dynamic Mirror Entities are two excellent tools for mirroring 2D sketches.
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