Proceedings ArticleDOI
Carbon overcoatings for soft x-ray reflectivity enhancement
Vincenzo Cotroneo,Daniele Spiga,Marco Barbera,R. Bruni,K. Chen,C. Marcelli,G. Pareschi,Suzanne Romaine,Y. D. Zhao,L. Zheng,Z. Y. Wu +10 more
TLDR
In this article, the first results concerning the effect of high-density materials on the reflectivity of X-ray observations were presented at the photon energies of 200 eV (i.e. below the carbon K absorption edge).Abstract:
In X-ray astronomical telescopes, the focalization of the radiation is achieved by means of grazing incidence Wolter I
(parabola + hyperbola) optics in total reflection regime. In general, high density materials (e.g. Au, Pt, Ir, W) are used as
reflecting coatings, in order to increase as much as possible the cut-off angles and energies for total reflection. However
these materials present an important reduction of the reflectivity between 0.2 and 5 keV, due to the photoabsorption, and
this phenomenon is particularly enhanced in correspondence of the M absorption edges (between 2 and 3.5 keV). In
general, this determines a strong decrease of the telescope effective area. To overcome the problem we suggested in
previous works the coating of the mirror surface by a low-density material such as carbon. Mirror samples with different
coatings made by high density materials: Au, Ir, Pt, and W with a carbon overcoating were manufactured and reflectivity
data in the soft X-ray band (100-2000 eV), performed both at the XACT facility in Palermo (Italy) and at BSRF
synchrotron in Beijing (China), are showed. In this paper we present some of the first results concerning the
measurements carried out at the photon energies of 200 eV (i.e. below the carbon K absorption edge) and 1280 eV (i.e.
the region just below the heavy material M absorption edge).read more
Citations
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Journal ArticleDOI
Voyage through the Hidden Physics of the Cosmic Web.
Aurora Simionescu,Stefano Ettori,Norbert Werner,Daisuke Nagai,Franco Vazza,H. Akamatsu,Ciro Pinto,J. de Plaa,Nastasha Wijers,Dylan Nelson,E. Pointecouteau,G. W. Pratt,Daniele Spiga,Erwin T. Lau,M. Rossetti,F. Gastaldello,V. Biffi,Esra Bulbul,J. W. den Herder,D. Eckert,Filippo Fraternali,Beatriz Mingo,G. Pareschi,Gabriele Pezzulli,Thomas H. Reiprich,Joop Schaye,Stephen Walker,Jessica K. Werk +27 more
TL;DR: In this paper, the authors proposed a next-generation "Cosmic Web Explorer" that can reach the accretion shocks located several times farther than the virial radii of galaxy clusters and reveal the out-of-equilibrium parts of the intra-cluster medium which are live witnesses to the physics of cosmic accretion.
Proceedings ArticleDOI
New developments in light material overcoating for soft x-ray reflectivity enhancement
Vincenzo Cotroneo,Daniele Spiga,R. Bruni,Wolfgang Burkert,Michael Freyberg,Gisela Hartner,G. Pareschi,Suzanne Romaine +7 more
TL;DR: In this paper, the authors have shown how a thin layer of a light material, like carbon, on top of a traditional reflecting coating, can enhance the reflectivity in the soft x-ray spectral region (below 5 keV) without degrading the performances for higher energies.
Proceedings ArticleDOI
BEaTriX (Beam Expander Testing X-ray facility) for testing ATHENA's SPO modules: advancement status
Bianca Salmaso,Stefano Basso,Mauro Ghigo,Enrico Giro,G. Pareschi,Daniele Spiga,G. Tagliaferri,G. Vecchi,Carlo Pelliciari,Vadim Burwitz,M. Sanchez del Rio,Claudio Ferrari,Andrea Zappettini,Michela Uslenghi,M. Fiorini,Giancarlo Parodi,Mark Ayre,Marcos Bavdaz,Ivo Ferreira,Eric Wille +19 more
TL;DR: In this paper, the Beam Expander Testing X-ray facility (BEaTriX) is proposed to test the Silicon Pore Optics (SPO) modules of the ATHENA Xray observatory.
Proceedings ArticleDOI
Progress in the realization of the beam expander testing x-ray facility (BEaTriX) for testing ATHENA's SPO modules
Bianca Salmaso,Daniele Spiga,Stefano Basso,Mauro Ghigo,Enrico Giro,G. Pareschi,G. Tagliaferri,G. Vecchi,Carlo Pelliciari,Vadim Burwitz,M. Sanchez del Rio,Claudio Ferrari,Andrea Zappettini,Michela Uslenghi,M. Fiorini,Giancarlo Parodi,Ivo Ferreira,Marcos Bavdaz +17 more
TL;DR: The BEaTriX (Beam Expander Testing X-ray) facility is ongoing at INAF/Osservatorio astronomico di Brera as mentioned in this paper, which is designed to operate at 1.49 keV and 4.51 keV by using two fixed beam lines, equipped with the necessary optical elements.
Proceedings ArticleDOI
Soft x-ray reflectivity-enhancement in astronomical telescopes via overcoatings: alternative materials and deposition methods
G. Pareschi,Marta Civitani,Giorgia Sironi,Yang Yang,V. Cotroneo,Giuseppe Valsecchi,Luca Magagnin,Thorsten Döhring,Miranda Bradshaw,Vadim Burwitz,Carlo Pelliciari +10 more
TL;DR: In this article, a novel approach based on the use of thin layer of a Carbon-like materials deposited using a dip coating method is discussed, which can further enhance the soft X-ray effective area of future Xray telescopes.
References
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Proceedings ArticleDOI
Astronomical soft x-ray mirrors reflectivity enhancement by multilayer coatings with carbon overcoating
Giovanni Pareschi,Vincenzo Cotroneo,Daniele Spiga,Dervis Vernani,Marco Barbera,Maria Antonella Artale,Alfonso Collura,Salvatore Varisco,Gabriele Grisoni,Giuseppe Valsecchi,Barbara Negri +10 more
TL;DR: In this paper, the impact of using soft X-ray multilayer mirrors in future Xray telescopes is discussed, and soft Xray reflectivity tests performed on prototype samples presented.
Journal ArticleDOI
The SIMBOL-X hard X-ray mission
TL;DR: SIMBOL-X as mentioned in this paper is a hard X-ray mission based on a formation flight architecture, operating in the 0.5-80 keV energy range, which has been selected for a comprehensive Phase A study, being jointly carried out by CNES and ASI.
Proceedings ArticleDOI
SIMBOL-X: a formation-flying mission for hard-x-ray astrophysics
P. Ferrando,Andrea Goldwurm,Philippe Laurent,Olivier Limousin,J. Martignac,F. Pinsard,Y. Rio,Jean-Pierre Roques,Oberto Citterio,G. Pareschi,G. Tagliaferri,Fabrizio Fiore,Giuseppe Malaguti,Ulrich G. Briel,Günther Hasinger,Lothar Strüder +15 more
TL;DR: SIMBOL-X as mentioned in this paper is a hard X-ray mission, operating in the ~ 0.5-70 keV range, which is proposed by a consortium of European laboratories in response to the 2004 call for ideas of CNES for a scientific mission to be flown on a formation flying demonstrator.
Proceedings ArticleDOI
Soft (0.1 - 10 keV) and hard (>10 keV) x-ray multilayer mirrors for the XEUS astronomical mission
TL;DR: In this paper, a global optimization approach based on an Iteraded Simplex Procedure was applied to optimize the sequence of bi-layers of depth-graded multilayer films, in order to get the best achievable response by the XEUS-I mirrors in the hard X-ray region.
Proceedings ArticleDOI
Silicon pore optics for astrophysical X-ray missions
Maximilien J. Collon,Ramses Günther,Stefan Kraft,Marco W. Beijersbergen,Marcos Bavdaz,Kotska Wallace,Michael Krumrey,Michael Freyberg +7 more
TL;DR: In this paper, the characteristics of the latest generation of very light, stiff and modular X-ray optics, termed high-performance pore optics (HPO), are discussed in detail.
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