Advanced LIGO Laser Systems for O3 and Future Observation Runs von Bode, Nina, Briggs, Joseph, Chen, Xu, Frede, Maik, Fritschel, Peter, Fyffe, Michael, Gustafson, Eric, Heintze, Matthew, King, Peter, Liu, Jian, Oberling, Jason, Savage, Richard L., Spencer, Andrew, Willke, Benno

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Sequential high power laser amplifiers for gravitational wave detection von Bode, Nina, Meylahn, Fabian, Willke, Benno

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High power, single-frequency, monolithic fiber amplifier for the next generation of gravitational wave detectors von Wellmann, Felix, Steinke, Michael, Meylahn, Fabian, Bode, Nina, Willke, Benno, Overmeyer, Ludger, Neumann, Jörg, Kracht, Dietmar

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Low noise 400 W coherently combined single frequency laser beam for next generation gravitational wave detectors von Wellmann, Felix, Bode, Nina, Wessels, Peter, Overmeyer, Ludger, Neumann, Jörg, Willke, Benno, Kracht, Dietmar

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High-power laser beam in higher-order Hermite–Gaussian modes von Behren, B. von, Heinze, Joscha, Bode, Nina, Willke, Benno

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Conversion of 30 W laser light at 1064 nm to 20 W at 2128 nm and comparison of relative power noise von Gurs, Julian, Bode, Nina, Darsow-Fromm, Christian, Vahlbruch, Henning, Gewecke, Pascal, Steinlechner, Sebastian, Willke, Benno, Schnabel, Roman

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Nd:YVO 4 high-power master oscillator power amplifier laser system for second-generation gravitational wave detectors von Thies, Fabian, Bode, Nina, Oppermann, Patrick, Frede, Maik, Schulz, Bastian, Willke, Benno

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Multiple beam coherent combination via an optical ring resonator von Bode, Nina, Holmes, Zachary, Ng, Sebastian, vonBehren, Benjamin, Ottaway, David, Willke, Benno

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Nd:YVO4 high-power master oscillator power amplifier laser system for second-generation gravitational wave detectors von Thies, Fabian, Bode, Nina, Oppermann, Patrick, Frede, Maik, Schulz, Bastian, Willke, Benno

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Performance study of a high-power single-frequency fiber amplifier architecture for gravitational wave detectors von Wellmann, Felix, Steinke, Michael, Wessels, Peter, Bode, Nina, Meylahn, Fabian, Willke, Benno, Overmeyer, Ludger, Neumann, Jörg, Kracht, Dietmar

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Nd:YVO^sub 4^ high-power master oscillator power amplifier laser system for second-generation gravitational wave detectors von Thies, Fabian, Bode, Nina, Oppermann, Patrick, Frede, Maik, Schulz, Bastian, Willke, Benno

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Quasi Monolithic Fiber Collimators von Carter, Jonathan Joseph, Böhme, Steffen, Weber, Kevin, Bode, Nina, Jorke, Karina, Grobecker, Anja, Koch, Tobias, Fabia, Simone, Koehlenbeck, Sina Maria

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30 W ultra-stable laser light at 2128 nm for future gravitational-wave observatories von Gurs, Julian, Bode, Nina, Darsow-Fromm, Christian, Vahlbruch, Henning, Gewecke, Pascal, Steinlechner, Sebastian, Willke, Benno, Schnabel, Roman

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Conversion of 30 W laser light at 1064 nm to 20 W at 2128 nm and comparison of relative power noise von Gurs, Julian, Bode, Nina, Darsow-Fromm, Christian, Vahlbruch, Henning, Gewecke, Pascal, Steinlechner, Sebastian, Willke, Benno, Schnabel, Roman

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Conversion of 30 W laser light at 1064 nm to 20 W at 2128 nm and comparison of relative power noise von Gurs, Julian, Bode, Nina, Darsow-Fromm, Christian, Vahlbruch, Henning, Gewecke, Pascal, Steinlechner, Sebastian, Willke, Benno, Schnabel, Roman

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Squeezing the quantum noise of a gravitational-wave detector below the standard quantum limit von Jia, Wenxuan, Xu, Victoria, Kuns, Kevin, Evans, Matthew, Abbott, Rich, Ananyeva, Alena, Appert, Stephen, Aritomi, Naoki, Ballmer, Stefan, Barker, David, Betzwieser, Joseph, Bhattacharjee, Dripta, Bonilla, Edgard, Bossilkov, Vladimir, Branch, Adam, Brooks, Aidan, Brown, Daniel, Cao, Huy-tuong, Compton, Camilla, Cottingham, Robert, Csizmazia, Janos, Driggers, Jenne, Etzel, Todd, Feicht, Jon, Frey, Raymond, Frischhertz, William, Fritschel, Peter, Frolov, Valery, Fulda, Paul, Fyffe, Michael, Ganapathy, Dhruva, Gateley, Bubba, Giaime, Joe, Giardina, Dwayne, Guidry, Tyler, Hanks, Jonathan, Hanson, Joe, Heintze, Matthew, Hsiang-yu, Huang, James, Alasdair, Karat, Srinath, Kawabe, Keita, Kissel, Jeffrey, Kumar, Rahul, Lesovsky, Madeline, Llamas, Francisco, Lormand, Marc, Macas, Ronaldas, Macinnis, Myron, Makarem, Camille, Mannix, Benjaminrobert, Martin, Rodica, Mccarthy, Richard, Mcclelland, David, Mccormick, Scott, Mcculler, Lee, Meylahn, Fabian, Mittleman, Richard, Moraru, Dan, Moreno, Gerardo, Mould, Matthew, Nelson, Timothy, Osthelder, Charles, Ottaway, David, Parker, William, Pele, Arnaud, Pham, Huyen, Pirello, Marc, Quetschke, Volker, Ramirez, Karla, Richardson, Jonathan, Robinson, Mitchell, Romie, Janeen, Ross, Michael, Sadecki, Travis, Sanchez, Anthony, Sanchez, Eduardo, Sanchez, Luis, Savage, Richard, Schaetzl, Dean, Mitchell Schiworski, Schnabel, Roman, Schwartz, Eyal, Sellers, Danny, Slagmolen, Bram, Soni, Siddharth, Sun, Ling, Thomas, Patrick, Torrie, Calum, Vajente, Gabriele, Jordan Vanosky, Vecchio, Alberto, Veitch, Peter, Vibhute, Ajay, Warner, Jim, Weaver, Betsy, Weiss, Rainer, Wipf, Christopher, Yu, Haocun, Zucker, Michael

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Quasi Monolithic Fiber Collimators von Carter, Jonathan Joseph, Böhme, Steffen, Weber, Kevin, Bode, Nina, Jorke, Karina, Grobecker, Anja, Koch, Tobias, Fabia, Simone, Koehlenbeck, Sina Maria

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ZUR BEDEUTUNG DES LINKEN VORGESTELLTEN BEINES BEIM ARCHAISCHEN KUROS von Bode, Nina

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Die Statue von Mozia: Hamilkar als Heros (Taf. 27) von Bode, Nina

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DIE STATUE VON MOZIA: HAMILKAR ALS HEROS von BODE, NINA

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