LIGO Detector Characterization in the first half of the fourth Observing run

Soni, S.; Berger, B. K.; Davis, D.; Renzo, F. Di.; Effler, A.; Ferreira, T. A.; Glanzer, J.; Goetz, E.; González, G.; Helmling-Cornell, A.; Hughey, B.; Huxford, R.; Mannix, B.; Mo, G.; Nandi, D.; Neunzert, A.; Nichols, S.; Pham, K.; Renzini, A. I.; Schofield, R. M. S.; Stuver, A; Trevor, M.; Álvarez-López, S.; Beda, R.; Berry, C. P. L.; Bhuiyan, S.; Bruntz, R.; Christensen, N.; Blagg, L.; Chan, M.; Charlton, P.; Connolly, G.; Dhatri, R.; Ding, J.; Garg, V.; Holley-Bockelmann, K.; Hourihane, S.; Jani, K.; Janssens, K.; Jarov, S.; Knee, A. M.; Lattal, A.; Lecoeuche, Y.; Littenberg, T.; Liyanage, A.; Lott, B.; Macas, R.; Malakar, D.; McGowan, K.; McIver, J.; Millhouse, M.; Nuttall, L.; Nykamp, D.; Ota, I.; Rawcliffe, C.; Scully, B.; Tasson, J.; Tejera, A.; Thiele, S.; Udall, R.; Winborn, C.; Yarbrough, Z.; Zhang, Z.; Abbott, R.; Abouelfettouh, I.; Adhikari, R. X.; Ananyeva, A.; Appert, S.; Arai, K.; Aritomi, N.; Aston, S. M.; Ball, M.; Ballmer, S. W.; Barker, D.; Barsotti, L.; Betzwieser, J.; Billingsley, G.; Biscans, S.; Bode, N.; Bonilla, E.; Bossilkov, V.; Branch, A.; Brooks, A. F.; Brown, D. D.; Bryant, J.; Cahillane, C.; Cao, H.; Capote, E.; Clara, F.; Collins, J.; Compton, C. M.; Cottingham, R.; Coyne, D. C.; Crouch, R.; Csizmazia, J.; Cullen, T. J.; Dartez, L. P.; Demos, N.; Dohmen, E.; Driggers, J. C.; Dwyer, S. E.; Ejlli, A.; Etzel, T.; Evans, M.; Feicht, J.; Frey, R.; Frischhertz, W.; Fritschel, P.; Frolov, V. V.; Fulda, P.; Fyffe, M.; Ganapathy, D.; Gateley, B.; Giaime, J. A.; Giardina, K. D.; Goetz, R.; Goodwin-Jones, A. W.; Gras, S.; Gray, C.; Griffith, D.; Grote, H.; Guidry, T.; Hall, E. D.; Hanks, J.; Hanson, J.; Heintze, M. C.; Holland, N. A.; Hoyland, D.; Huang, H. Y.; Inoue, Y.; James, A. L.; Jennings, A.; Jia, W.; Karat, S.; Karki, S.; Kasprzack, M.; Kawabe, K.; Kijbunchoo, N.; King, P. J.; Kissel, J. S.; Komori, K.; Kontos, A.; Kumar, Rahul; Kuns, K.; Landry, M.; Lantz, B.; Laxen, M.; Lee, K.; Lesovsky, M.; Llamas, F.; Lormand, M.; Loughlin, H. A.; Macas, R.; MacInnis, M.; Makarem, C. N.; Mansell, G. L.; Martin, R. M.; Mason, K.; Matichard, F.; Mavalvala, N.; Maxwell, N.; McCarrol, G.; McCarthy, R.; McClelland, D. E.; McCormick, S.; McCuller, L.; McRae, T.; Mera, F.; Merilh, E. L.; Meylahn, F.; Mittleman, R.; Moraru, D.; Moreno, G.; Mullavey, A.; Nakano, M.; Nelson, T. J. N.; Notte, J.; Oberling, J.; O'Hanlon, T.; Osthelder, C.; Ottaway, D. J.; Overmier, H.; Parker, W.; Pele, A.; Pham, H.; Pirello, M.; Quetschke, V.; Ramirez, K. E.; Reyes, J.; Richardson, J. W.; Robinson, M.; Rollins, J. G.; Romel, C. L.; Romie, J. H.; Ross, M. P.; Ryan, K.; Sadecki, T.; Sanchez, A.; Sanchez, E. J.; Sanchez, L. E.; Savage, R. L.; Schaetzl, D.; Schiworski, M. G.; Schnabel, R.; Schwartz, E.; Sellers, D.; Shaffer, T.; Short, R. W.; Sigg, D.; Slagmolen, B. J. J.; Soike, C.; Srivastava, V.; Sun, L.; Tanner, D. B.; Thomas, M.; Thomas, P.; Thorne, K. A.; Torrie, C. I.; Traylor, G.; Ubhi, A. S.; Vajente, G.; Vanosky, J.; Vecchio, A.; Veitch, P. J.; Vibhute, A. M.; von Reis, E. R. G.; Warner, J.; Weaver, B.; Weiss, R.; Whittle, C.; Willke, B.; Wipf, C. C.; Xu, V. A.; Yamamoto, H.; Zhang, L.; Zucker, M. E.

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LIGO Detector Characterization in the first half of the fourth Observing run

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Bode, N.
Laser Interferometry & Gravitational Wave Astronomy, AEI-Hannover, MPI for Gravitational Physics, Max Planck Society;

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Willke, B.
Laser Interferometry & Gravitational Wave Astronomy, AEI-Hannover, MPI for Gravitational Physics, Max Planck Society;

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Zitation

Soni, S., Berger, B. K., Davis, D., Renzo, F. D., Effler, A., Ferreira, T. A., et al. (in preparation). LIGO Detector Characterization in the first half of the fourth Observing run.

Zitierlink: https://hdl.handle.net/21.11116/0000-000F-DC49-8

Zusammenfassung

Progress in gravitational-wave astronomy depends upon having sensitive
detectors with good data quality. Since the end of the LIGO-Virgo-KAGRA third
Observing run in March 2020, detector-characterization efforts have lead to
increased sensitivity of the detectors, swifter validation of
gravitational-wave candidates and improved tools used for data-quality
products. In this article, we discuss these efforts in detail and their impact
on our ability to detect and study gravitational-waves. These include the
multiple instrumental investigations that led to reduction in transient noise,
along with the work to improve software tools used to examine the detectors
data-quality. We end with a brief discussion on the role and requirements of
detector characterization as the sensitivity of our detectors further improves
in the future Observing runs.