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Related papers: The MICADO first light imager for the ELT: the PSF…

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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

The Euclid ERO showcase Euclid's capabilities in advance of its main mission, targeting 17 astronomical objects, from galaxy clusters, nearby galaxies, globular clusters, to star-forming regions. A total of 24 hours observing time was…

Instrumentation and Methods for Astrophysics · Physics 2025-04-30 J. -C. Cuillandre , E. Bertin , M. Bolzonella , H. Bouy , S. Gwyn , S. Isani , M. Kluge , O. Lai , A. Lançon , D. A. Lang , R. Laureijs , T. Saifollahi , M. Schirmer , C. Stone , Abdurro'uf , N. Aghanim , B. Altieri , F. Annibali , H. Atek , P. Awad , M. Baes , E. Bañados , D. Barrado , S. Belladitta , V. Belokurov , A. Boselli , F. Bournaud , J. Bovy , R. A. A. Bowler , G. Buenadicha , F. Buitrago , M. Cantiello , D. Carollo , S. Codis , M. L. M. Collins , G. Congedo , E. Dalessandro , V. de Lapparent , F. De Paolis , J. M. Diego , P. Dimauro , J. Dinis , H. Dole , P. -A. Duc , D. Erkal , M. Ezziati , A. M. N. Ferguson , A. Ferré-Mateu , A. Franco , R. Gavazzi , K. George , W. Gillard , J. B. Golden-Marx , B. Goldman , A. H. Gonzalez , R. Habas , W. G. Hartley , N. A. Hatch , R. Kohley , J. Hoar , J. M. Howell , L. K. Hunt , P. Jablonka , M. Jauzac , Y. Kang , J. H. Knapen , J. -P. Kneib , R. Kohley , P. B. Kuzma , S. S. Larsen , O. Marchal , J. Martín-Fleitas , P. Marcos-Arenal , F. R. Marleau , E. L. Martín , D. Massari , A. W. McConnachie , M. Meneghetti , M. Miluzio , J. Miro Carretero , H. Miyatake , M. Mondelin , M. Montes , A. Mora , O. Müller , C. Nally , K. Noeske , A. A. Nucita , P. A. Oesch , M. Oguri , R. F. Peletier , M. Poulain , L. Quilley , G. D. Racca , M. Rejkuba , J. Rhodes , P. -F. Rocci , J. Román , S. Sacquegna , E. Saremi , R. Scaramella , E. Schinnerer , S. Serjeant , E. Sola , J. G. Sorce , F. Tarsitano , I. Tereno , S. Toft , C. Tortora , M. Urbano , A. Venhola , K. Voggel , J. R. Weaver , X. Xu , M. Žerjal , R. Zöller , S. Andreon , N. Auricchio , M. Baldi , A. Balestra , S. Bardelli , A. Basset , R. Bender , C. Bodendorf , E. Branchini , S. Brau-Nogue , M. Brescia , J. Brinchmann , S. Camera , V. Capobianco , C. Carbone , J. Carretero , S. Casas , F. J. Castander , M. Castellano , S. Cavuoti , A. Cimatti , C. J. Conselice , L. Conversi , Y. Copin , F. Courbin , H. M. Courtois , M. Cropper , J. -G. Cuby , A. Da Silva , H. Degaudenzi , A. M. Di Giorgio , M. Douspis , C. A. J. Duncan , X. Dupac , S. Dusini , M. Fabricius , M. Farina , S. Farrens , S. Ferriol , S. Fotopoulou , M. Frailis , E. Franceschi , S. Galeotta , B. Garilli , B. Gillis , C. Giocoli , P. Gómez-Alvarez , A. Grazian , F. Grupp , L. Guzzo , S. V. H. Haugan , J. Hoar , H. Hoekstra , W. Holmes , I. Hook , F. Hormuth , A. Hornstrup , P. Hudelot , K. Jahnke , M. Jhabvala , E. Keihänen , S. Kermiche , A. Kiessling , M. Kilbinger , T. Kitching , B. Kubik , K. Kuijken , M. Kümmel , M. Kunz , H. Kurki-Suonio , O. Lahav , S. Ligori , P. B. Lilje , V. Lindholm , I. Lloro , D. Maino , E. Maiorano , O. Mansutti , O. Marggraf , K. Markovic , N. Martinet , F. Marulli , R. Massey , S. Maurogordato , H. J. McCracken , E. Medinaceli , Y. Mellier , G. Meylan , J. J. Mohr , M. Moresco , L. Moscardini , E. Munari , R. Nakajima , R. C. Nichol , S. -M. Niemi , C. Padilla , S. Paltani , F. Pasian , J. A. Peacock , K. Pedersen , W. J. Percival , V. Pettorino , S. Pires , G. Polenta , M. Poncet , L. A. Popa , L. Pozzetti , F. Raison , R. Rebolo , A. Refregier , A. Renzi , G. Riccio , Hans-Walter Rix , E. Romelli , M. Roncarelli , E. Rossetti , R. Saglia , D. Sapone , P. Schneider , T. Schrabback , A. Secroun , G. Seidel , S. Serrano , C. Sirignano , G. Sirri , J. Skottfelt , L. Stanco , P. Tallada-Crespí , A. N. Taylor , H. I. Teplitz , R. Toledo-Moreo , A. Tsyganov , I. Tutusaus , E. A. Valentijn , L. Valenziano , T. Vassallo , G. Verdoes Kleijn , Y. Wang , J. Weller , O. R. Williams , G. Zamorani , E. Zucca , C. Baccigalupi , C. Burigana , P. Casenove , P. Liebing , V. Scottez , P. Simon , D. Scott

The ELT is a 39m large, ground-based optical and near- to mid-infrared telescope under construction in the Chilean Atacama desert. Operation is planned to start around the middle of the next decade. All first light instruments will come…

The ESO-Spitzer extragalactic Imaging Survey (ESIS) is the optical follow up of the Spitzer Wide-Area InfraRed Extragalactic (SWIRE) survey in the ELAIS-S1 area. This paper presents B, V, R Wide Field Imager observations of the first 1.5…

The Large Binocular Telescope (LBT) has two 8.4-m primary mirrors that produce beams that can be combined coherently in a "Fizeau" interferometric mode. In principle, the Fizeau PSF enables the probing of structure at a resolution up to…

Instrumentation and Methods for Astrophysics · Physics 2022-01-19 Eckhart Spalding , Katie M. Morzinski , Phil Hinz , Jared Males , Michael Meyer , Sascha P. Quanz , Jarron Leisenring , Jennifer Power

We report results from numerical simulations assessing astrometry measurements with the Multiconjugate Adaptive Optics Relay for ELT Observations (MORFEO) instrument on the Extremely Large Telescope (ELT). Using the Advanced Exposure Time…

Context. The advent of the Extremely Large Telescope (ELT) will increase the collecting area by more than an order of magnitude compared to the individual Unit Telescopes of the Very Large Telescope (VLT). Fainter spectrophotometric…

Instrumentation and Methods for Astrophysics · Physics 2025-08-11 N. P. Gentile Fusillo , S. Moehler , N. Przybilla , A. K. Elms , P. -E. Tremblay , W. Kausch , F. Kerber

METIS, the Mid-infrared ELT Imager and Spectrograph (formerly called MIDIR), is a proposed instrument for the European Extremely Large Telescope (E-ELT), currently undergoing a phase-A study. The study is carried out within the framework of…

We introduce the first end-to-end learning-based solution to near-field Photometric Stereo (PS), where the light sources are close to the object of interest. This setup is especially useful for reconstructing large immobile objects. Our…

Computer Vision and Pattern Recognition · Computer Science 2022-03-31 Daniel Lichy , Soumyadip Sengupta , David W. Jacobs

In preparation of future Multi-Object Spectrographs (MOS) whose one of the major role is to provide an extensive statistical studies of high redshifted galaxies surveyed, the demonstrator Canary has been designed to tackle technical…

Instrumentation and Methods for Astrophysics · Physics 2016-11-23 O. A. Martin , C. M. Correia , E. Gendron , G. Rousset , D. Gratadour , F. Vidal , T. J. Morris , A. G. Basden , R. M. Myers , B. Neichel , T. Fusco

The achievement of $\mu$arcsec relative astrometry with ground-based, near infrared, extremely large telescopes requires a significant endeavour of calibration strategies. In this paper we address the removal of instrument optical…

We present a proof-of-concept end-to-end system for computational extended depth of field (EDOF) imaging. The acquisition is performed through a phase-coded aperture implemented by placing a thin wavelength-dependent optical mask inside the…

Computer Vision and Pattern Recognition · Computer Science 2016-08-04 Tal Remez , Or Litany , Shachar Yoseff , Harel Haim , Alex Bronstein

Single particle cryo-electron microscopy has become a critical tool in structural biology over the last decade, able to achieve atomic scale resolution in three dimensional models from hundreds of thousands of (noisy) two-dimensional…

Numerical Analysis · Mathematics 2023-07-19 Aaditya V. Rangan , Leslie Greengard

Here we describe a simple, efficient, and most importantly fully operational point-spread-function(PSF)-reconstruction approach for laser-assisted ground layer adaptive optics (GLAO) in the frame of the Multi Unit Spectroscopic Explorer…

Instrumentation and Methods for Astrophysics · Physics 2020-04-08 Thierry Fusco , R. Bacon , S. Kamann , S. Conseil , Benoit Neichel , Carlos Correia , Olivier Beltramo-Martin , Joel Vernet , Johann Kolb , Pierre-Yves Madec

Since 2014, the LBT's First Light Adaptive Optics (FLAO) system has also included a seldom used capability, known as Enhanced Seeing Mode (ESM), that can improve the angular resolution over a 4' x 4' field of view (FOV). In full AO…

Instrumentation and Methods for Astrophysics · Physics 2019-11-05 Barry Rothberg , Julian C. Christou , Douglas L. Miller , Dave Thompson , Gregory E. Taylor , Christian Veillet

MIDIR is the proposed thermal/mid-IR imager and spectrograph for the European Extremely Large Telescope (E-ELT). It will cover the wavelength range of 3 to at least 20 microns. Designed for diffraction-limited performance over the entire…

Astrophysics · Physics 2009-11-13 S. Kendrew , B. Brandl , R. Lenzen , L. Venema , H. U. Käufl , G. Finger , A. Glasse , R. Stuik

The Public European Southern Observatory Spectroscopic Survey of Transient Objects (PESSTO) began as a public spectroscopic survey in April 2012. We describe the data reduction strategy and data products which are publicly available through…

This paper discusses the reconstruction of partially sampled spectrum-images to accelerate the acquisition in scanning transmission electron microscopy (STEM). The problem of image reconstruction has been widely considered in the literature…

Image and Video Processing · Electrical Eng. & Systems 2020-02-05 Etienne Monier , Thomas Oberlin , Nathalie Brun , Xiaoyan Li , Marcel Tencé , Nicolas Dobigeon

We present the first on-sky results of the micro-lens ring tip-tilt (MLR-TT) sensor. This sensor utilizes a 3D printed micro-lens ring feeding six multi-mode fibers to sense misaligned light, allowing centroid reconstruction. A tip-tilt…

The EAGLE instrument is a Multi-Object Adaptive Optics (MOAO) fed, multiple Integral Field Spectrograph (IFS), working in the Near Infra-Red (NIR), on the European Extremely Large Telescope (E-ELT). A Phase A design study was delivered to…