Details
| Original language | English |
|---|---|
| Title of host publication | International Conference on Space Optics, ICSO 2016 |
| Subtitle of host publication | ICSO 2016 |
| Editors | Bruno Cugny, Nikos Karafolas, Zoran Sodnik |
| Publisher | SPIE |
| ISBN (electronic) | 9781510616134 |
| Publication status | Published - 26 Sept 2017 |
| Event | International Conference on Space Optics 2016 - Biarritz, France Duration: 18 Oct 2016 → 21 Oct 2016 |
Publication series
| Name | Proceedings of SPIE - The International Society for Optical Engineering |
|---|---|
| Volume | 10562 |
| ISSN (Print) | 0277-786X |
| ISSN (electronic) | 1996-756X |
Abstract
Angular misalignment of one of the interfering beams in laser interferometers can couple into the interferometric length measurement and is called tilt-to-length (TTL) coupling in the following. In the noise budget of the planned space-based gravitational-wave detector evolved Laser Interferometer Space Antenna (eLISA) [1, 2] TTL coupling is the second largest noise source after shot noise [3].
ASJC Scopus subject areas
- Materials Science(all)
- Electronic, Optical and Magnetic Materials
- Physics and Astronomy(all)
- Condensed Matter Physics
- Mathematics(all)
- Applied Mathematics
- Engineering(all)
- Electrical and Electronic Engineering
- Computer Science(all)
- Computer Science Applications
Cite this
- Standard
- Harvard
- Apa
- Vancouver
- BibTeX
- RIS
International Conference on Space Optics, ICSO 2016: ICSO 2016. ed. / Bruno Cugny; Nikos Karafolas; Zoran Sodnik. SPIE, 2017. 1056245 (Proceedings of SPIE - The International Society for Optical Engineering; Vol. 10562).
Research output: Chapter in book/report/conference proceeding › Conference contribution › Research
}
TY - GEN
T1 - Experimental demonstration of reduced tilt-to-length coupling by using imaging systems in precision interferometers
AU - Tröbs, M.
AU - Chwalla, M.
AU - Danzmann, K.
AU - Fernández Barránco, G.
AU - Fitzsimons, E.
AU - Gerberding, O.
AU - Heinzel, G.
AU - Killow, C. J.
AU - Lieser, M.
AU - Perreur-lloyd, M.
AU - Robertson, D. I.
AU - Schuster, S.
AU - Schwarze, T. S.
AU - Ward, H.
AU - Zwetz, M.
N1 - Funding Information: We acknowledge funding by the European Space Agency within the project “Optical Bench Development for LISA” (22331/09/NL/HB), support from UK Space Agency, University of Glasgow, Scottish Universities Physics Alliance (SUPA), and support by Deutsches Zentrum für Luft und Raumfahrt (DLR) with funding from the Bundesministerium für Wirtschaft und Technologie (DLR project reference 50 OQ 0601). We thank the German Research Foundation for funding the cluster of Excellence QUEST - Centre for Quantum Engineering and Space-Time Research.
PY - 2017/9/26
Y1 - 2017/9/26
N2 - Angular misalignment of one of the interfering beams in laser interferometers can couple into the interferometric length measurement and is called tilt-to-length (TTL) coupling in the following. In the noise budget of the planned space-based gravitational-wave detector evolved Laser Interferometer Space Antenna (eLISA) [1, 2] TTL coupling is the second largest noise source after shot noise [3].
AB - Angular misalignment of one of the interfering beams in laser interferometers can couple into the interferometric length measurement and is called tilt-to-length (TTL) coupling in the following. In the noise budget of the planned space-based gravitational-wave detector evolved Laser Interferometer Space Antenna (eLISA) [1, 2] TTL coupling is the second largest noise source after shot noise [3].
UR - http://www.scopus.com/inward/record.url?scp=85037695400&partnerID=8YFLogxK
U2 - 10.1117/12.2296137
DO - 10.1117/12.2296137
M3 - Conference contribution
T3 - Proceedings of SPIE - The International Society for Optical Engineering
BT - International Conference on Space Optics, ICSO 2016
A2 - Cugny, Bruno
A2 - Karafolas, Nikos
A2 - Sodnik, Zoran
PB - SPIE
T2 - International Conference on Space Optics 2016
Y2 - 18 October 2016 through 21 October 2016
ER -