English

Re-testing the JET-X Flight Module No. 2 at the PANTER facility

Instrumentation and Methods for Astrophysics 2014-02-20 v4

Abstract

The Joint European X-ray Telescope (JET-X) was the core instrument of the Russian Spectrum-X-gamma space observatory. It consisted of two identical soft X-ray (0.3 - 10 keV) telescopes with focusing optical modules having a measured angular resolution of nearly 15 arcsec. Soon after the payload completion, the mission was cancelled and the two optical flight modules (FM) were brought to the Brera Astronomical Observatory where they had been manufactured. After 16 years of storage, we have utilized the JET-X FM2 to test at the PANTER X-ray facility a prototype of a novel X-ray polarimetric telescope, using a Gas Pixel Detector (GPD) with polarimetric capabilities in the focal plane of the FM2. The GPD was developed by a collaboration between INFN-Pisa and INAF-IAPS. In the first phase of the test campaign, we have re-tested the FM2 at PANTER to have an up-to-date characterization in terms of angular resolution and effective area, while in the second part of the test the GPD has been placed in the focal plane of the FM2. In this paper we report the results of the tests of the sole FM2, using an unpolarized X-ray source, comparing the results with the calibration done in 1996.

Cite

@article{arxiv.1311.2220,
  title  = {Re-testing the JET-X Flight Module No. 2 at the PANTER facility},
  author = {Daniele Spiga and Gianpiero Tagliaferri and Paolo Soffitta and Oberto Citterio and Stefano Basso and Ronaldo Bellazzini and Alessandro Brez and Wolfgang Burkert and Vadim Burwitz and Enrico Costa and Luca de Ruvo and Ettore Del Monte and Sergio Fabiani and Gisela Hartner and Benedikt Menz and Massimo Minuti and Fabio Muleri and Giovanni Pareschi and Michele Pinchera and Alda Rubini and Carmelo Sgrò and Gloria Spandre},
  journal= {arXiv preprint arXiv:1311.2220},
  year   = {2014}
}

Comments

Author's accepted manuscript posted to arXiv.org as permitted by Springer's Self-Archiving Policy. The final publication is available at http://rd.springer.com/article/10.1007%2Fs10686-013-9365-y

R2 v1 2026-06-22T02:04:24.221Z