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Fabian Meylahn and Benno Willke
The continuous improvement of current gravitational wave detectors (GWDs) and the preparations for next generation GWDs place high demands on their stabilized laser sources. Some of the laser sources need to operate at laser wavelengths between 1.5 &...
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Florian Amann, Francesca Badaracco, Riccardo DeSalvo, Luca Naticchioni, Andrea Paoli, Luca Paoli, Paolo Ruggi and Stefano Selleri
The Einstein Telescope will be a gravitational wave observatory comprising six nested detectors, three optimized to collect low-frequency signals, and three for high frequency. It will be built a few hundred meters under Earth?s surface to reduce direct ...
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Michele Bignotto, Michele Bonaldi, Massimo Cerdonio, Livia Conti, Francesco Penasa, Giovanni A. Prodi, Gabriele Soranzo, Luca Taffarello, and Jean-Pierre Zendri
Pág. -
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Gossler, S. Casey, M. M. Freise, A. Grant, A. Grote, H. Heinzel, G. Heurs, M. Husman, M. E. Kotter, K. Leonhardt, V.
Pág. 3787 - 3795
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Nagano, S. Kawamura, S. Ando, M. Takahashi, R. Arai, K. Musha, M. Telada, S. Fujimoto, M.-K. Fukushima, M. Kozai, Y.
Pág. 4176 - 4183
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Hewitson, M. Grote, H. Heinzel, G. Strain, K. A. Ward, H. Weiland, U.
Pág. 4184 - 4190
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Giaime, J. A. Daw, E. J. Weitz, M. Adhikari, R. Fritschel, P. Abbott, R. Bork, R. Heefner, J.
Pág. 218 - 224
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Beauville, F. Buskulic, D. Flaminio, R. Marion, F. Masserot, A. Massonnet, L. Mours, B. Ramonet, J. Tournefier, E. Verkindt, D.
Pág. 2564 - 2569
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Somiya, K. Tariq, H. Miyakawa, O. Heinzel, G. Mio, N. Kawamura, S.
Pág. 3942 - 3945
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Takahashi, R. Kuwahara, F. Majorana, E. Barton, M. A. Uchiyama, T. Kuroda, K. Araya, A. Arai, K. Takamori, A. Ando, M.
Pág. 2428 - 2433
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