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Temperature stability in the sub-milliHertz band with LISA Pathfinder

Author
Armano, M.; Audley, H.; Baird, J.; Binetruy, P.; Born, M.; Bortoluzzi, D.; Ramos, J.
Type of activity
Journal article
Journal
Monthly notices of the Royal Astronomical Society
Date of publication
2019-07-01
Volume
486
Number
3
First page
3368
Last page
3379
DOI
10.1093/mnras/stz1017
Repository
http://hdl.handle.net/2117/167199 Open in new window
URL
https://academic.oup.com/mnras/article-abstract/486/3/3368/5449024 Open in new window
Abstract
LISA Pathfinder (LPF) was a technology pioneering mission designed to test key technologies required for gravitational wave detection in space. In the low frequency regime (milliHertz and below), where space-based gravitational wave observatories will operate, temperature fluctuations play a crucial role since they can couple into the interferometric measurement and the test masses’ free-fall accuracy in many ways. A dedicated temperature measurement subsystem, with noise levels in 10¿µK¿Hz...
Citation
Armano, M. [et al.]. Temperature stability in the sub-milliHertz band with LISA Pathfinder. "Monthly notices of the Royal Astronomical Society", 1 Juliol 2019, vol. 486, núm. 3, p. 3368-3379.
Keywords
Gravitational waves, Space vehicles: Instruments
Group of research
CREB - Biomedical Engineering Research Centre
GCEM - Electromagnetic Compatibility Group

Participants

  • Armano, M.  (author)
  • Audley, H.  (author)
  • Baird, J.  (author)
  • Binetruy, P.  (author)
  • Born, M.  (author)
  • Bortoluzzi, D.  (author)
  • Ramos Castro, Juan Jose  (author)

Attachments