activity
20142026
most citedThe HOSTS survey for exozodiacal dust: Observational results from the complete survey

124 citations · 370 across the 26 of their papers we have counts for

collaborators

33 papers

astro-ph.IM2026

The final design of GMagAO-X: the wavefront sensing and control (WFS&C) architecture of GMagAO-X

Sebastiaan Y. Haffert, Jared R. Males, Laird M. Close +10

The Giant Magellan Adaptive Optics eXtreme (GMagAO-X) instrument has now been selected as an official part of the Giant Magellan Telescope's (GMT) instrument suite. The instrument…

astro-ph.IM2026

Upgrading LBTI/NOMIC with a quadruple annular groove phase mask and GeoSnap detector for imaging nearby, habitable-zone exoplanets

Kevin Wagner, Manny Montoya, Steve Ertel +32

The Large Binocular Telescope Interferometer (LBTI)'s Nulling-Optimized Mid-Infrared Camera (NOMIC) is among the most capable thermal-infrared imaging systems available for high-co…

astro-ph.IM2026

The final design of GMagAO-X: high-contrast imaging at first-light of the GMT

Jared R. Males, Laird M. Close, Sebastiaan Y. Haffert +13

GMagAO-X will be the first-light high-contrast imager on the 25 m Giant Magellan Telescope. The driving science case for GMagAO-X is characterization of the atmospheres of nearby r…

astro-ph.IM2026

The Space Coronagraph Optical Bench (SCoOB): 11. Modeling and correction of chromatic aberrations

Kyle Van Gorkom, Ramya M. Anche, Saraswathi Kalyani Subramanian +12

The space coronagraph optical bench (SCoOB) is a high contrast imaging testbed designed to demonstrate starlight suppression techniques at visible wavelengths in a space-like vacuu…

astro-ph.IM2026

The Space Coronagraph Optical Bench (SCoOB): X. Dark zone maintenance

Saraswathi Kalyani Subramanian, Kyle Van Gorkom, Ramya Anche +12

The Space Coronagraph Optical Bench (SCoOB) is a vacuum high contrast imaging testbed designed to demonstrate starlight suppression at optical wavelengths and obtain contrasts bett…

astro-ph.IM2025

The Space Coronagraph Optical Bench (SCoOB): 8. end-to-end numerical modeling of the testbed to estimate the contrast limits

Ramya M Anche, Kyle Van Gorkom, Kian Milani +9

The space coronagraph optical bench (SCoOB) at the University of Arizona is a high-contrast imaging testbed designed to operate in a vacuum to obtain a contrast better than 1e-8 in…

astro-ph.IM2025

MIRAC-5 on the MMT with MAPS: annular groove phase mask N-band coronagraphic upgrade

Alyssa L. Miller, Jarron Leisenring, Michael Meyer +15

We describe the coronagraphic upgrade underway for the Mid-Infrared Array Camera-5 (MIRAC-5) to be used with the 6.5-m MMT telescope utilizing the new MMT Adaptive optics exoPlanet…

astro-ph.IM2024

Commissioning of the MIRAC-5 Mid-Infrared Instrument on the MMT

Rory Bowens, Jarron Leisenring, Michael R. Meyer +11

We present results from commissioning observations of the mid-IR instrument, MIRAC-5, on the 6.5-m MMT telescope. MIRAC-5 is a novel ground-based instrument that utilizes a state-o…

astro-ph.IM2024

Tuning the MAPS Adaptive Secondary Mirror: Actuator Control, PID Tuning, Power Spectra and Failure Diagnosis

Jess A. Johnson, Amali Vaz, Manny Montoya +17

The MMT Adaptive optics exoPlanet characterization System (MAPS) is currently in its engineering phase, operating on-sky at the MMT Telescope on Mt. Hopkins in southern Arizona. Th…

astro-ph.IM2024★ 1 cited

High-contrast imaging at first-light of the GMT: the wavefront sensing and control architecture of GMagAO-X

Sebastiaan Y. Haffert, Jared R Males, Laird M. Close +3

The Giant Magellan Adaptive Optics eXtreme (GMagAO-X) instrument is a first-light high-contrast imaging instrument for the Giant Magellan Telescope (GMT). GMagAO-X's broad waveleng…

astro-ph.IM2024

High-Contrast Imaging at First-Light of the GMT: The Preliminary Design of GMagAO-X

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

We present the preliminary design of GMagAO-X, the first-light high-contrast imager planned for the Giant Magellan Telescope. GMagAO-X will realize the revolutionary increase in sp…

astro-ph.IM2024★ 1 cited

The space coronagraph optical bench (SCoOB): 4. vacuum performance of a high contrast imaging testbed

Kyle Van Gorkom, Ewan S Douglas, Kian Milani +8

The Space Coronagraph Optical Bench (SCoOB) is a high-contrast imaging testbed built to demonstrate starlight suppression techniques at visible wavelengths in a space-like vacuum e…

astro-ph.IM2023★ 5 cited

SOUL at LBT: commissioning results, science and future

Enrico Pinna, Fabio Rossi, Guido Agapito +27

The SOUL systems at the Large Bincoular Telescope can be seen such as precursor for the ELT SCAO systems, combining together key technologies such as EMCCD, Pyramid WFS and adaptiv…

astro-ph.IM2023

GMagAO-X: A First Light Coronagraphic Adaptive Optics System for the GMT

Maggie Kautz, Jared R. Males, Laird M. Close +17

GMagAO-X is a visible to NIR extreme adaptive optics (ExAO) system that will be used at first light for the Giant Magellan Telescope (GMT). GMagAO-X is designed to deliver diffract…

astro-ph.IM2023

The MAPS Adaptive Secondary Mirror: First Light, Laboratory Work, and Achievements

Jess A. Johnson, Amali Vaz, Manny Montoya +23

The MMT Adaptive Optics exoPlanet Characterization System (MAPS) is a comprehensive update to the first generation MMT adaptive optics system (MMTAO), designed to produce a facilit…

astro-ph.IM2022★ 2 cited

A Near-Infrared Pyramid Wavefront Sensor for the MMT

Jacob Taylor, Suresh Sivanandam, Narsireddy Anugu +8

The MMTO Adaptive optics exoPlanet characterization System (MAPS) is an ongoing upgrade to the 6.5-meter MMT Observatory on Mount Hopkins in Arizona. MAPS includes an upgraded adap…

astro-ph.IM2022

The Optical and Mechanical Design for the 21,000 Actuator ExAO System for the Giant Magellan Telescope: GMagAO-X

Laird M. Close, Jared R. Males, Olivier Durney +9

GMagAO-X is the near first light ExAO coronagraphic instrument for the 25.4m GMT. It is designed for a slot on the folded port of the GMT. To meet the strict ExAO fitting and servo…

astro-ph.IM2022

The space coronagraph optical bench (SCoOB): 2. wavefront sensing and control in a vacuum-compatible coronagraph testbed for spaceborne high-contrast imaging technology

Kyle Van Gorkom, Ewan S. Douglas, Jaren N. Ashcraft +9

The 2020 Decadal Survey on Astronomy and Astrophysics endorsed space-based high contrast imaging for the detection and characterization of habitable exoplanets as a key priority fo…

astro-ph.IM2022

The Space Coronagraph Optical Bench (SCoOB): 1. Design and Assembly of a Vacuum-compatible Coronagraph Testbed for Spaceborne High-Contrast Imaging Technology

Jaren N. Ashcraft, Heejoo Choi, Ewan S. Douglas +14

The development of spaceborne coronagraphic technology is of paramount importance to the detection of habitable exoplanets in visible light. In space, coronagraphs are able to bypa…

astro-ph.IM2021★ 3 cited

Design of the vacuum high contrast imaging testbed for CDEEP, the Coronagraphic Debris and Exoplanet Exploring Pioneer

Erin R. Maier, Ewan S. Douglas, Daewook Kim +26

The Coronagraphic Debris Exoplanet Exploring Payload (CDEEP) is a Small-Sat mission concept for high contrast imaging of circumstellar disks. CDEEP is designed to observe disks in…

astro-ph.IM2020★ 1 cited

Design and development of a high-speed Visible Pyramid Wavefront Sensor for the MMT AO system

Narsireddy Anugu, Olivier Durney, Katie M. Morzinski +16

MAPS, MMT Adaptive optics exoPlanet characterization System, is the upgrade of legacy 6.5m MMT adaptive optics system. It is an NSF MSIP-funded project that includes (i) refurbishi…

astro-ph.IM2020★ 18 cited

Final Design and On-Sky Testing of the iLocater SX Acquisition Camera: Broadband Single-Mode Fiber Coupling

Jonathan Crass, Andrew Bechter, Brian Sands +22

Enabling efficient injection of light into single-mode fibers (SMFs) is a key requirement in realizing diffraction-limited astronomical spectroscopy on ground-based telescopes. SMF…

astro-ph.SR2020★ 124 cited

The HOSTS survey for exozodiacal dust: Observational results from the complete survey

Steve Ertel, Denis Defrère, Philip M. Hinz +43

The Large Binocular Telescope Interferometer (LBTI) enables nulling interferometric observations across the N band (8 to 13 um) to suppress a star's bright light and probe for fain…

astro-ph.EP2018★ 2 cited

The HOSTS Survey for Exozodiacal Dust: Preliminary results and future prospects

S. Ertel, G. M. Kennedy, D. Defrère +40

[abridged] The presence of large amounts of dust in the habitable zones of nearby stars is a significant obstacle for future exo-Earth imaging missions. We executed an N band nulli…