papers

Publications (8)

astro-ph.IM2022

The Holographic Dispersed Fringe Sensors (HDFS): phasing the Giant Magellan Telescope

Sebastiaan Y. Haffert, Laird M. Close, Alexander D. Hedglen +14

The next generation of Giant Segmented Mirror Telescopes (GSMT) will have large gaps between the segments either caused by the shadow of the mechanical structure of the secondary m…

astro-ph.IM2022

MagAO-X: current status and plans for Phase II

Jared R. Males, Laird M. Close, Sebastiaan Haffert +15

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. MagAO-X is optimized for high contras…

astro-ph.SR2023

HIP 67506 C: MagAO-X Confirmation of a New Low-Mass Stellar Companion to HIP 67506 A

Logan A. Pearce, Jared R. Males, Sebastiaan Y. Haffert +17

We report the confirmation of HIP 67506 C, a new stellar companion to HIP 67506 A. We previously reported a candidate signal at 2/D (240~mas) in L in MagAO/Clio imag…

astro-ph.IM2022

XPipeline: Starlight subtraction at scale for MagAO-X

Joseph D. Long, Jared R. Males, Sebastiaan Y. Haffert +15

MagAO-X is an extreme adaptive optics (ExAO) instrument for the Magellan Clay 6.5-meter telescope at Las Campanas Observatory in Chile. Its high spatial and temporal resolution can…

astro-ph.IM2022

Experimental Trials With The Optical Differentiation Wavefront Sensor For Extended Objects

Meghan Farris O'Brien, Sebastiaan Y. Haffert, Joseph D. Long +4

Commonly used wavefront sensors, the Shack Hartmann wavefront sensor and the pyramid wavefront sensor, for example, have large dynamic range or high sensitivity, trading one regime…

astro-ph.IM2022

The Giant Magellan Telescope high contrast adaptive optics phasing testbed (p-HCAT): lab tests of segment/petal phasing with a pyramid wavefront sensor and a holographic dispersed fringe sensor (HDFS) in turbulence

Alexander D. Hedglen, Laird M. Close, Sebastiaan Y. Haffert +14

The Giant Magellan Telescope (GMT) design consists of seven circular 8.4-m diameter mirror segments that are separated by large > 30 cm gaps, creating the possibility of fluctuatio…

astro-ph.IM2018

MagAO-X: project status and first laboratory results

Jared R. Males, Laird M. Close, Kelsey Miller +32

MagAO-X is an entirely new "extreme" adaptive optics system for the Magellan Clay 6.5 m telescope, funded by the NSF MRI program starting in Sep 2016. The key science goal of MagAO…

astro-ph.IM2021

Data-driven subspace predictive control of adaptive optics for high-contrast imaging

Sebastiaan Y. Haffert, Jared R. Males, Laird M. Close +11

The search for exoplanets is pushing adaptive optics systems on ground-based telescopes to their limits. One of the major limitations at small angular separations, exactly where ex…