These tools will no longer be maintained as of December 31, 2024. Archived website can be found here. PubMed4Hh GitHub repository can be found here. Contact NLM Customer Service if you have questions.
3. Thermal effects in the Input Optics of the Enhanced Laser Interferometer Gravitational-Wave Observatory interferometers. Dooley KL; Arain MA; Feldbaum D; Frolov VV; Heintze M; Hoak D; Khazanov EA; Lucianetti A; Martin RM; Mueller G; Palashov O; Quetschke V; Reitze DH; Savage RL; Tanner DB; Williams LF; Wu W Rev Sci Instrum; 2012 Mar; 83(3):033109. PubMed ID: 22462908 [TBL] [Abstract][Full Text] [Related]
4. Mirror-orientation noise in a Fabry-Perot interferometer gravitational wave detector. Kawamura S; Zucker ME Appl Opt; 1994 Jun; 33(18):3912-8. PubMed ID: 20935736 [TBL] [Abstract][Full Text] [Related]
5. Implications of Dedicated Seismometer Measurements on Newtonian-Noise Cancellation for Advanced LIGO. Coughlin MW; Harms J; Driggers J; McManus DJ; Mukund N; Ross MP; Slagmolen BJJ; Venkateswara K Phys Rev Lett; 2018 Nov; 121(22):221104. PubMed ID: 30547651 [TBL] [Abstract][Full Text] [Related]
6. Twin mirrors for laser interferometric gravitational-wave detectors. Sassolas B; Benoît Q; Flaminio R; Forest D; Franc J; Galimberti M; Lacoudre A; Michel C; Montorio JL; Morgado N; Pinard L Appl Opt; 2011 May; 50(13):1894-9. PubMed ID: 21532671 [TBL] [Abstract][Full Text] [Related]
7. Analysis of light noise sources in a recycled Michelson interferometer with Fabry-Perot arms. Camp JB; Yamamoto H; Whitcomb SE; McClelland DE J Opt Soc Am A Opt Image Sci Vis; 2000 Jan; 17(1):120-8. PubMed ID: 10641846 [TBL] [Abstract][Full Text] [Related]
8. Experimental demonstration of a classical analog to quantum noise cancellation for use in gravitational wave detection. Mow-Lowry CM; Sheard BS; Gray MB; McClelland DE; Whitcomb SE Phys Rev Lett; 2004 Apr; 92(16):161102. PubMed ID: 15169214 [TBL] [Abstract][Full Text] [Related]