Skip to main content
archive
Search Submit Donate Log in
Press Enter to search · Advanced search

Astrophysics > Instrumentation and Methods for Astrophysics

arXiv:2107.05496 (astro-ph)
[Submitted on 12 Jul 2021]

Title:Design, Construction, and Test of the Gas Pixel Detectors for the IXPE Mission

Authors:L. Baldini, M. Barbanera, R. Bellazzini, R. Bonino, F. Borotto, A. Brez, C. Caporale, C. Cardelli, S. Castellano, M. Ceccanti, S. Citraro, N. Di Lalla, L. Latronico, L. Lucchesi, C. Magazzù, G. Magazzù, S. Maldera, A. Manfreda, M. Marengo, A. Marrocchesi, P. Mereu, M. Minuti, F. Mosti, H. Nasimi, A. Nuti, C. Oppedisano, L. Orsini, M. Pesce-Rollins, M. Pinchera, A. Profeti, C. Sgrò, G. Spandre, M. Tardiola, D. Zanetti, F. Amici, H. Andersson, P. Attinà, M. Bachetti, W. Baumgartner, D. Brienza, R. Carpentiero, M. Castronuovo, L. Cavalli, E. Cavazzuti, M. Centrone, E. Costa, E. D'Alba, F. D'Amico, E. Del Monte, S. Di Cosimo, A. Di Marco, G. Di Persio, I. Donnarumma, Y. Evangelista, S. Fabiani, R. Ferrazzoli, T. Kitaguchi, F. La Monaca, C. Lefevre, P. Loffredo, P. Lorenzi, E. Mangraviti, G. Matt, T. Meilahti, A. Morbidini, F. Muleri, T. Nakano, B. Negri, S. Nenonen, S. L. O'Dell, M. Perri, R. Piazzolla, S. Pieraccini, M. Pilia, S. Puccetti, B. D. Ramsey, J. Rankin, A. Ratheesh, A. Rubini, F. Santoli, P. Sarra, E. Scalise, A. Sciortino, P. Soffitta, T. Tamagawa, A. F. Tennant, A. Tobia, A. Trois, K. Uchiyama, M. Vimercati, M. C. Weisskopf, F. Xie, F. Zanetti, Y. Zhou
View a PDF of the paper titled Design, Construction, and Test of the Gas Pixel Detectors for the IXPE Mission, by L. Baldini and 93 other authors
View PDF HTML (experimental)
Abstract:Due to be launched in late 2021, the Imaging X-Ray Polarimetry Explorer (IXPE) is a NASA Small Explorer mission designed to perform polarization measurements in the 2-8 keV band, complemented with imaging, spectroscopy and timing capabilities. At the heart of the focal plane is a set of three polarization-sensitive Gas Pixel Detectors (GPD), each based on a custom ASIC acting as a charge-collecting anode. In this paper we shall review the design, manufacturing, and test of the IXPE focal-plane detectors, with particular emphasis on the connection between the science drivers, the performance metrics and the operational aspects. We shall present a thorough characterization of the GPDs in terms of effective noise, trigger efficiency, dead time, uniformity of response, and spectral and polarimetric performance. In addition, we shall discuss in detail a number of instrumental effects that are relevant for high-level science analysis -- particularly as far as the response to unpolarized radiation and the stability in time are concerned.
Comments: To be published in Astroparticle Physics
Subjects: Instrumentation and Methods for Astrophysics (astro-ph.IM); High Energy Astrophysical Phenomena (astro-ph.HE); Instrumentation and Detectors (physics.ins-det)
Cite as: arXiv:2107.05496 [astro-ph.IM]
  (or arXiv:2107.05496v1 [astro-ph.IM] for this version)
  https://doi.org/10.48550/arXiv.2107.05496
arXiv-issued DOI via DataCite
Related DOI: https://doi.org/10.1016/j.astropartphys.2021.102628
DOI(s) linking to related resources

Submission history

From: Carmelo Sgrò [view email]
[v1] Mon, 12 Jul 2021 15:28:42 UTC (5,222 KB)
Full-text links:

Access Paper:

    View a PDF of the paper titled Design, Construction, and Test of the Gas Pixel Detectors for the IXPE Mission, by L. Baldini and 93 other authors
  • View PDF
  • HTML (experimental)
  • TeX Source
license icon view license

Current browse context:

astro-ph.IM
< prev   |   next >
new | recent | 2021-07
Change to browse by:
astro-ph
astro-ph.HE
physics
physics.ins-det

References & Citations

  • INSPIRE HEP
  • NASA ADS
  • Google Scholar
  • Semantic Scholar
Loading...

BibTeX formatted citation

Data provided by:

Bookmark

BibSonomy Reddit

Bibliographic and Citation Tools

Bibliographic Explorer (What is the Explorer?)
Connected Papers (What is Connected Papers?)
Litmaps (What is Litmaps?)
scite Smart Citations (What are Smart Citations?)

Code, Data and Media Associated with this Article

alphaXiv (What is alphaXiv?)
CatalyzeX Code Finder for Papers (What is CatalyzeX?)
DagsHub (What is DagsHub?)
Gotit.pub (What is GotitPub?)
Hugging Face (What is Huggingface?)
ScienceCast (What is ScienceCast?)

Demos

Replicate (What is Replicate?)
Hugging Face Spaces (What is Spaces?)
TXYZ.AI (What is TXYZ.AI?)

Recommenders and Search Tools

Influence Flower (What are Influence Flowers?)
CORE Recommender (What is CORE?)
IArxiv Recommender (What is IArxiv?)
  • Author
  • Venue
  • Institution
  • Topic

arXivLabs: experimental projects with community collaborators

arXivLabs is a framework that allows collaborators to develop and share new arXiv features directly on our website.

Both individuals and organizations that work with arXivLabs have embraced and accepted our values of openness, community, excellence, and user data privacy. arXiv is committed to these values and only works with partners that adhere to them.

Have an idea for a project that will add value for arXiv's community? Learn more about arXivLabs.

Which authors of this paper are endorsers? | Disable MathJax (What is MathJax?)
We gratefully acknowledge support from our major funders, member institutions, , and all contributors.
About · Help · Contact · Subscribe · Copyright · Privacy · Accessibility · Operational Status (opens in new tab)
Major funding support from
Simons Foundation Simons Foundation International Schmidt Sciences