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Related papers: Gemini North Adaptive Optics (GNAO) facility overv…

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Astrometry was not a science case of the Gemini Multiconjugate adaptive optics System (GeMS) at its design stage. However, since GeMS has been in regular science operation with the Gemini South Adaptive Optics Imager (GSAOI), their…

Instrumentation and Methods for Astrophysics · Physics 2019-03-22 Mauro Patti , Giuliana Fiorentino

Lithium niobate-on-insulator (LNOI) is an emerging photonic platform that exhibits favorable material properties (such as low optical loss, strong nonlinearities, and stability) and enables large-scale integration with stronger optical…

Using five independent analytic and Monte Carlo simulation codes, we have studied the performance of wide field ground layer adaptive optics (GLAO), which can use a single, relatively low order deformable mirror to correct the wavefront…

This project is focused on evaluating the slowly-varying ground layer seeing component at the optical telescopes of ARIES. To achieve this, we assembled the instrument, consisting of a filter wheel, a CCD camera, and a tip-tilt enabled…

Instrumentation and Methods for Astrophysics · Physics 2024-01-22 Purvi Udhwani , Amitesh Omar , Krishna Reddy

The Gemini Planet Imager (GPI) is a high performance adaptive optics system being designed and built for the Gemini Observatory. GPI is optimized for high contrast imaging, combining precise and accurate wavefront control, diffraction…

This paper proposes an illumination-robust visual odometry (VO) system that incorporates both accelerated learning-based corner point algorithms and an extended line feature algorithm. To be robust to dynamic illumination, the proposed…

Robotics · Computer Science 2023-12-20 Kuan Xu , Yuefan Hao , Shenghai Yuan , Chen Wang , Lihua Xie

Habitable Worlds Observatory (HWO) presents a key challenge for technology development in the coming years, requiring a $>$ $100\times$ more stable system than \textit{JWST}. WaveDriver is a concept for a laser guide star spacecraft coupled…

In recent years, graph neural networks (GNNs) have shown tremendous promise in solving problems in high energy physics, materials science, and fluid dynamics. In this work, we introduce a new application for GNNs in the physical sciences:…

Instrumentation and Methods for Astrophysics · Physics 2026-02-17 Sidharth Kannan , Pooyan Goodarzi , Evangelos E. Papalexakis , Jonathan W. Richardson

We present the conceptual design of GMagAO-X, an extreme adaptive optics system for the 25 m Giant Magellan Telescope (GMT). We are developing GMagAO-X to be available at or shortly after first-light of the GMT, to enable early high…

The Multi-conjugate Adaptive optics Demonstrator, MAD, successfully demonstrated on sky the MCAO technique both in Layer Oriented and Star Oriented modes. As results of the Guaranteed Time Observations in Layer Oriented mode quality…

Instrumentation and Methods for Astrophysics · Physics 2010-09-20 Carmelo Arcidiacono , Matteo Lombini , Alessia Moretti , Roberto Ragazzoni , Jacopo Farinato , Renato Falomo , Marco Gullieuszik , Giampaolo Piotto

"MagAO" is the adaptive optics instrument at the Magellan Clay telescope at Las Campanas Observatory, Chile. MagAO has a 585-actuator adaptive secondary mirror and 1000-Hz pyramid wavefront sensor, operating on natural guide stars from…

In this paper we present the Adaptive Optics Lucky Imager (AOLI), a state-of-the-art instrument which makes use of two well proved techniques for extremely high spatial resolution with ground-based telescopes: Lucky Imaging (LI) and…

MORFEO (Multi-conjugate adaptive Optics Relay For ELT Observations, formerly MAORY), the MCAO system for the ELT, will provide diffraction-limited optical quality to the large field camera MICADO. MORFEO has officially passed the…

Instrumentation and Methods for Astrophysics · Physics 2024-06-06 Lorenzo Busoni , Guido Agapito , Alessandro Ballone , Alfio Puglisi , Alexander Goncharov , Amedeo Petrella , Amico Di Cianno , Andrea Balestra , Andrea Baruffolo , Andrea Bianco , Andrea Di Dato , Angelo Valentini , Benedetta Di Francesco , Benoit Sassolas , Bernardo Salasnich , Carmelo Arcidiacono , Cedric Plantet , Christian Eredia , Daniela Fantinel , Danilo Selvestrel , Deborah Malone , Demetrio Magrin , Domenico D'Auria , Edoardo Redaelli , Elena Carolo , Elia Costa , Elisa Portaluri , Enrico Cascone , Enrico Giro , Federico Battaini , Francesca Annibali , Fulvio Laudisio , Gabriele Rodeghiero , Gabriele Umbriaco , Gael Chauvin , Gianluca Di Rico , Giorgio Pariani , Giulia Carlà , Giulio Capasso , Giuseppe Cosentino , Jean Jacques Correia , Italo Foppiani , Ivan Di Antonio , Jacopo Farinato , Kalyan Kumar Radhakrishnan , Laurence Gluck , Laurent Pinard , Luca Marafatto , Marcello Agostino Scalera , Marco Gullieuszik , Marco Bonaglia , Marco Riva , Marco Xompero , Maria Bergomi , Matteo Aliverti , Matteo Genoni , Matteo Munari , Mauro Dolci , Michel Christophe , Michele Cantiello , Mirko Colapietro , Nicholas Devaney , Nicolò Azzaroli , Paolo Grani , Paolo Ciliegi , Patrick Rabou , Philippe Feautrier , Pietro Schipani , Roberto Ragazzoni , Rosanna Sordo , Runa Briguglio , Salvatore Lampitelli , Salvatore Savarese , Simone Benedetti , Simone Di Filippo , Simone Esposito , Simonetta Chinellato , Sylvain Oberti , Sylvain Rochat , Tommaso Lapucci , Ugo Di Giammatteo , Vincenzo Cianniello , Vincenzo De Caprio , Zoltan Hubert

We describe a device (adapter) for off-axis guiding and photometric calibration of wide-angle spectrographs operating in the prime focus of the 6-m telescope of the Special Astrophysical Observatory of the Russian Academy of Sciences. To…

Instrumentation and Methods for Astrophysics · Physics 2017-12-13 Victor L. Afanasiev , Vladimir R. Amirkhanyan , Alexei V. Moiseev , Roman I. Uklein , Alexander E. Perepelitsyn

Adaptive optics (AO) systems allow a telescope to reach its diffraction limit at near infrared wavelengths. But to achieve this, a bright natural guide star (NGS) is needed for the wavefront sensing, severely limiting the fraction of the…

A new high-order adaptive optics system is now being commissioned at the Lick Observatory Shane 3-meter telescope in California. This system uses a high return efficiency sodium beacon and a combination of low and high-order deformable…

As we enter the era of TESS and JWST, instrumentation that can carry out radial velocity measurements of exoplanet systems is in high demand. We will address this demand by upgrading the UC Lick Observatory's 2.4-meter Automated Planet…

Instrumentation and Methods for Astrophysics · Physics 2023-08-29 Rachel Bowens-Rubin , Arjo Bos , Philip Hinz , Bradford Holden , Matt Radovan

Adaptive optics (AO) is a powerful image correction technique with proven benefits for many life-science microscopy methods. However, the complexity of adding a reflective wavefront modulator and a wavefront sensor into already complicated…

Robo-AO is an autonomous laser guide star adaptive optics system recently commissioned at the Kitt Peak 2.1-m telescope. Now operating every clear night, Robo-AO at the 2.1-m telescope is the first dedicated adaptive optics observatory.…

Instrumentation and Methods for Astrophysics · Physics 2017-12-27 Rebecca Jensen-Clem , Dmitry A. Duev , Reed Riddle , Maïssa Salama , Christoph Baranec , Nicholas M. Law , S. R. Kulkarni , A. N. Ramprakash

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 contrast imaging at visible wavelengths. Our primary science goals…