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Realistic simulations of experiments at large scale photon facilities, such as optical laser laboratories, synchrotrons, and free electron lasers, are of vital importance for the successful preparation, execution, and analysis of these…

The availability and performance of laser-based adaptive optics (AO) systems are strongly dependent on the power and quality of the laser beam before being projected to the sky. Frequent and time-consuming alignment procedures are usually…

Instrumentation and Methods for Astrophysics · Physics 2014-05-23 Clémentine Béchet , Andrés Guesalaga , Benoit Neichel , Vincent Fesquet , Héctor González-Núñez , Sebastián Zúñiga , Pedro Escarate , Dani Guzman

We present a silicon-nitride-based optical phased array with built-in focusing and steering capability, that operates at 522 nm and is aimed at complementing a micro-electrode array for joint electrical and optical probing of retinal…

We study conditions for aberration-free imaging of inelastic x-ray scattering (IXS) spectra with x-ray echo spectrometers. Aberration-free imaging is essential for achieving instrumental functions with high resolution and high contrast.…

Instrumentation and Detectors · Physics 2019-05-29 Manuel Sánchez del Río , Yuri Shvyd'ko

We have recently demonstrated a very favorable, inexpensive modernization of lab-based x-ray absorption fine structure (XAFS) and high-resolution x-ray emission spectroscopy (XES) using only commercially-available optics and x-ray tube…

Instrumentation and Detectors · Physics 2016-06-22 Gerald T. Seidler , Devon R. Mortensen , Alexander S. Ditter , Neil A. Ball , Adam J. Remesnik

The results of a study of the accuracy characteristics and image quality on the SAO RAS optical telescopes, Zeiss-1000 and BTA, using the recently developed "Telescope Analyzer" device are described: a method for determining the…

Instrumentation and Methods for Astrophysics · Physics 2025-02-14 Edward Emelianov

Optical modules for X-ray telescopes comprise several double-reflection mirrors operating in grazing incidence. The concentration power of an optical module, which determines primarily the telescope's sensitivity, is in general expressed by…

Instrumentation and Methods for Astrophysics · Physics 2011-03-28 Daniele Spiga

We present the Spectroscopic Time-Resolving Observatory for Broadband Energy X-rays (STROBE-X), a probe-class mission concept selected for study by NASA. It combines huge collecting area, high throughput, broad energy coverage, and…

Instrumentation and Methods for Astrophysics · Physics 2019-03-11 Paul S. Ray , Zaven Arzoumanian , David Ballantyne , Enrico Bozzo , Soren Brandt , Laura Brenneman , Deepto Chakrabarty , Marc Christophersen , Alessandra DeRosa , Marco Feroci , Keith Gendreau , Adam Goldstein , Dieter Hartmann , Margarita Hernanz , Peter Jenke , Erin Kara , Tom Maccarone , Michael McDonald , Michael Nowak , Bernard Phlips , Ron Remillard , Abigail Stevens , John Tomsick , Anna Watts , Colleen Wilson-Hodge , Kent Wood , Silvia Zane , Marco Ajello , Will Alston , Diego Altamirano , Vallia Antoniou , Kavitha Arur , Dominic Ashton , Katie Auchettl , Tom Ayres , Matteo Bachetti , Mislav Balokovic , Matthew Baring , Altan Baykal , Mitch Begelman , Narayana Bhat , Slavko Bogdanov , Michael Briggs , Esra Bulbul , Petrus Bult , Eric Burns , Ed Cackett , Riccardo Campana , Amir Caspi , Yuri Cavecchi , Jerome Chenevez , Mike Cherry , Robin Corbet , Michael Corcoran , Alessandra Corsi , Nathalie Degenaar , Jeremy Drake , Steve Eikenberry , Teruaki Enoto , Chris Fragile , Felix Fuerst , Poshak Gandhi , Javier Garcia , Adam Goldstein , Anthony Gonzalez , Brian Grefenstette , Victoria Grinberg , Bruce Grossan , Sebastien Guillot , Tolga Guver , Daryl Haggard , Craig Heinke , Sebastian Heinz , Paul Hemphill , Jeroen Homan , Michelle Hui , Daniela Huppenkothen , Adam Ingram , Jimmy Irwin , Gaurava Jaisawal , Amruta Jaodand , Emrah Kalemci , David Kaplan , Laurens Keek , Jamie Kennea , Matthew Kerr , Michiel van der Klis , Daniel Kocevski , Mike Koss , Adam Kowalski , Dong Lai , Fred Lamb , Silas Laycock , Joseph Lazio , Davide Lazzati , Dana Longcope , Michael Loewenstein , Dipankair Maitra , Walid Majid , W. Peter Maksym , Christian Malacaria , Raffaella Margutti , Adrian Martindale , Ian McHardy , Manuel Meyer , Matt Middleton , Jon Miller , Cole Miller , Sara Motta , Joey Neilsen , Tommy Nelson , Scott Noble , Paul O'Brien , Julian Osborne , Rachel Osten , Feryal Ozel , Nipuni Palliyaguru , Dheeraj Pasham , Alessandro Patruno , Vero Pelassa , Maria Petropoulou , Maura Pilia , Martin Pohl , David Pooley , Chanda Prescod-Weinstein , Dimitrios Psaltis , Geert Raaijmakers , Chris Reynolds , Thomas E. Riley , Greg Salvesen , Andrea Santangelo , Simone Scaringi , Stephane Schanne , Jeremy Schnittman , David Smith , Krista Lynne Smith , Bradford Snios , Andrew Steiner , Jack Steiner , Luigi Stella , Tod Strohmayer , Ming Sun , Thomas Tauris , Corbin Taylor , Aaron Tohuvavohu , Andrea Vacchi , Georgios Vasilopoulos , Alexandra Veledina , Jonelle Walsh , Nevin Weinberg , Dan Wilkins , Richard Willingale , Joern Wilms , Lisa Winter , Michael Wolff , Jean in 't Zand , Andreas Zezas , Bing Zhang , Abdu Zoghbi

A high-resolution beam telescope is essential for the precise characterization of silicon pixel sensors. As part of the CSNS-II upgrade project, a High-Energy Proton Beam Telescope (HEPTel) based on monolithic active pixel sensors (MAPS)…

Instrumentation and Detectors · Physics 2026-02-17 Lan-Kun Li , Ze Gao , Ying-Hao Yu , Liang-Cheng-Long Jin , Ming-Yi Dong , Ren-Hong Liu , Hong-Yu Zhang , Chang Xu , Han-Tao Jing , Yu-Hang Guo , Qun Ou-Yang

In this work, we measure and model tilted x-ray refractive lenses to investigate their effects on an x-ray beam. The modelling is benchmarked against at-wavelength metrology obtained with x-ray speckle vector tracking experiments (XSVT) at…

We present a summary of the in-orbit performance of the soft X-ray imaging telescope Xtend onboard the XRISM mission, based on in-flight observation data, including first-light celestial objects, calibration sources, and results from the…

This project presents the development and implementation of a compact spectrometer, named SPECTRUMMATE, tailored for small telescopes. Small telescopes offer several advantages: they are cost-effective, occupy less space, and are simpler to…

Instrumentation and Methods for Astrophysics · Physics 2025-11-25 Hien Phan-Thanh , Nguyen Nguyen-Duc , Thuy Le-Quang , Tobias C. Hinse , Quang Nguyen-Luong

This paper presents the first-principle design approach for X-ray active optics, using the simulation-modulation cycle in place of the measurement-modulation feedback loops used in traditional active optics. Hence, the new active optics…

Optics · Physics 2024-01-09 Dezhi Diao , Han Dong , Fugui Yang , Ming Li , Weifan Sheng , Xiaowei Zhang

Non-destructive nano-imaging of the internal structure of solid matter is only feasible using hard X-rays due to their high penetration. The highest resolution images are achieved at synchrotron radiation sources (SRF), offering superior…

As one of the latest beamline built at the SOLEIL synchrotron source, ANTARES beamline offers a spectroscopic non-destructive nano-probe to study advanced materials. This innovative scanning photoemission microscopy combines linear and…

Instrumentation and Detectors · Physics 2015-06-12 Jose Avila , Ivy Razado , Stehane Lorcy , Bruno Lagarde , Jean-Luc Giorgetta , François Polack , Maria C. Asensio

In astrophysics, several key questions in the hard X soft Gamma-ray range (above 100 keV) require sensitivity and angular resolution that are hardly achievable with current technologies. Therefore, a new kind of instrument able to focus…

In the context of the LAUE project devoted to build a long focal-length focusing optics for soft $\gamma$-ray astronomy (80 - 600 keV), we present the results of reflectivity measurements of bent crystals in different configurations,…

Instrumentation and Methods for Astrophysics · Physics 2015-06-12 V. Liccardo , E. Virgilli , F. Frontera , V. Valsan

The Beam Dump Facility (BDF) is a planned fixed-target installation in CERN's North Area, set to start operating in 2031. A proton beam of 400 GeV/c will be delivered in 1 s pulses of 4e13 protons every 7.2 s, amounting to 4e19 protons on…

The Astro2020 decadal survey recommended an infrared, optical, ultra-violet (IR/O/UV) telescope with a $\sim$6~m inscribed diameter and equipped with a coronagraph instrument to directly image exoEarths in the habitable zone of their host…