activity
20132025
most citedFirst light of BEaTriX, the new testing facility for the modular X-ray optics of the ATHENA mission

18 citations · 63 across the 11 of their papers we have counts for

collaborators

11 papers

physics.ins-det2025

Effect of chromatic dispersion on image size and lattice plane curvature measurements with Rocking Curve Imaging

Elena Ferrari, Claudio Ferrari, Josè Baruchel +6

ADP crystals of large dimensions (80x80x20 mm3), to be used as a X-ray beam expanders in the BEaTriX facility at INAF-OABrera, have been characterised at BM05 beamline at ESRF sync…

astro-ph.IM2022★ 18 cited

First light of BEaTriX, the new testing facility for the modular X-ray optics of the ATHENA mission

S. Basso, B. Salmaso, D. Spiga +35

The Beam Expander Testing X-ray facility (BEaTriX) is a unique X-ray apparatus now operated at the Istituto Nazionale di Astrofisica (INAF), Osservatorio Astronomico di Brera (OAB)…

astro-ph.IM2019

Thin glass shells for active optics for future space telescopes

Gabriele Vecchi, Stefano Basso, Marta Civitani +3

We present a method for the manufacturing of thin shells of glass, which appears promising for the development of active optics for future space telescopes. The method exploits the…

astro-ph.IM2016★ 12 cited

Design and advancement status of the Beam Expander Testing X-ray facility (BEaTriX)

D. Spiga, C. Pelliciari, B. Salmaso +10

The BEaTriX (Beam Expander Testing X-ray facility) project is an X-ray apparatus under construction at INAF/OAB to generate a broad (200 x 60 mm2), uniform and low-divergent X-ray…

astro-ph.IM2016

Manufacturing and testing a thin glass mirror shell with piezoelectric active control

D. Spiga, M. Barbera, A. Collura +12

Optics for future X-ray telescopes will be characterized by very large aperture and focal length, and will be made of lightweight materials like glass or silicon in order to keep t…

astro-ph.IM2015★ 5 cited

Active shape correction of a thin glass/plastic X-ray mirror

D. Spiga, M. Barbera, S. Basso +9

Optics for future X-ray telescopes will be characterized by very large aperture and focal length, and will be made of lightweight materials like glass or plastic in order to keep t…

astro-ph.IM2015★ 15 cited

LAMP: a micro-satellite based soft X-ray polarimeter for astrophysics

Rui She, Hua Feng, Fabio Muleri +19

The Lightweight Asymmetry and Magnetism Probe (LAMP) is a micro-satellite mission concept dedicated for astronomical X-ray polarimetry and is currently under early phase study. It…

astro-ph.IM2015★ 3 cited

Profile reconstruction of grazing-incidence X-ray mirrors from intra-focal X-ray full imaging

D. Spiga, S. Basso, M. Bavdaz +11

The optics of a number of future X-ray telescopes will have very long focal lengths (10 - 20 m), and will consist of a number of nested/stacked thin, grazing-incidence mirrors. The…

astro-ph.IM2015★ 4 cited

Development of mirrors made of chemically tempered glass foils for future X-ray telescopes

B. Salmaso, M. Civitani, B. Brizzolari +6

Thin slumped glass foils are considered good candidates for the realization of future X-ray telescopes with large effective area and high spatial resolution. However, the hot slump…

astro-ph.IM2014★ 5 cited

Evaluation of the surface strength of glass plates shaped by hot slumping process

L. Proserpio, S. Basso, F. Borsa +15

The Hot Slumping Technology is under development by several research groups in the world for the realization of grazing-incidence segmented mirrors for X-ray astronomy, based on th…

physics.optics2013★ 1 cited

X-ray scattering of periodic and graded multilayers: comparison of experiments to simulations from surface microroughness characterization

B. Salmaso, D. Spiga, R. Canestrari +1

To enhance the reflectivity of X-ray mirrors beyond the critical angle, multilayer coatings are required. Interface imperfections in the multilayer growth process are known to caus…