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dc.contributor.authorVitale, Salvatore
dc.contributor.authorEvans, M.
dc.contributor.authorFritschel, Peter K.
dc.contributor.authorBarsotti, Lisa
dc.contributor.authorBiscans, Sebastien
dc.contributor.authorFernandez-Galiana, A.
dc.contributor.authorGras, Slawomir
dc.contributor.authorHall, Evan D.
dc.contributor.authorMacInnis, Myron E
dc.contributor.authorMartynov, Denis
dc.contributor.authorMason, Kenneth R
dc.contributor.authorMatichard, Fabrice
dc.contributor.authorMavalvala, Nergis
dc.contributor.authorMcCuller, Lee P
dc.contributor.authorMittleman, Richard K
dc.contributor.authorShoemaker, David H
dc.contributor.authorTse, Maggie
dc.contributor.authorWeiss, Rainer
dc.contributor.authorYu, Hang
dc.contributor.authorYu, Haocun
dc.contributor.authorZucker, Michael E
dc.date.accessioned2019-06-10T20:11:33Z
dc.date.available2019-06-10T20:11:33Z
dc.date.issued2019-02
dc.date.submitted2018-07
dc.identifier.issn2470-0010
dc.identifier.issn2470-0029
dc.identifier.urihttps://hdl.handle.net/1721.1/121242
dc.description.abstractThe Advanced LIGO detectors have recently completed their second observation run successfully. The run lasted for approximately 10 months and led to multiple new discoveries. The sensitivity to gravitational waves was partially limited by laser noise. Here, we utilize auxiliary sensors that witness these correlated noise sources, and use them for noise subtraction in the time domain data. This noise and line removal is particularly significant for the LIGO Hanford Observatory, where the improvement in sensitivity is greater than 20%. Consequently, we were also able to improve the astrophysical estimation for the location, masses, spins, and orbital parameters of the gravitational wave progenitors.en_US
dc.publisherAmerican Physical Societyen_US
dc.relation.isversionofhttp://dx.doi.org/10.1103/PhysRevD.99.042001en_US
dc.rightsArticle is made available in accordance with the publisher's policy and may be subject to US copyright law. Please refer to the publisher's site for terms of use.en_US
dc.sourceAPSen_US
dc.titleImproving astrophysical parameter estimation via offline noise subtraction for Advanced LIGOen_US
dc.typeArticleen_US
dc.identifier.citationDriggers, J. C. et al. “Improving Astrophysical Parameter Estimation via Offline Noise Subtraction for Advanced LIGO.” Physical Review D 99, 4 (February 2019): 042001 © 2019 American Physical Societyen_US
dc.contributor.departmentMassachusetts Institute of Technology. Department of Physicsen_US
dc.contributor.departmentMassachusetts Institute of Technology. Laboratory for Nuclear Scienceen_US
dc.contributor.departmentLIGO (Observatory : Massachusetts Institute of Technology)en_US
dc.relation.journalPhysical Review Den_US
dc.eprint.versionFinal published versionen_US
dc.type.urihttp://purl.org/eprint/type/JournalArticleen_US
eprint.statushttp://purl.org/eprint/status/PeerRevieweden_US
dc.date.updated2019-03-20T18:29:54Z
dspace.orderedauthorsDriggers, J. C.; Vitale, S.; Lundgren, A. P.; Evans, M.; Kawabe, K.; Dwyer, S. E.; Izumi, K.; Schofield, R. M. S.; Effler, A.; Sigg, D.; Fritschel, P.; Drago, M.; Nitz, A.; Abbott, B. P.; Abbott, R.; Abbott, T. D.; Adams, C.; Adhikari, R. X.; Adya, V. B.; Ananyeva, A.; Appert, S.; Arai, K.; Aston, S. M.; Austin, C.; Ballmer, S. W.; Barker, D.; Barr, B.; Barsotti, L.; Bartlett, J.; Bartos, I.; Batch, J. C.; Bell, A. S.; Betzwieser, J.; Billingsley, G.; Birch, J.; Biscans, S.; Blair, C. D.; Blair, R. M.; Bork, R.; Brooks, A. F.; Cao, H.; Ciani, G.; Clara, F.; Cooper, S. J.; Corban, P.; Countryman, S. T.; Covas, P. B.; Cowart, M. J.; Coyne, D. C.; Cumming, A.; Cunningham, L.; Danzmann, K.; Da Silva Costa, C. F.; Daw, E. J.; DeBra, D.; DeSalvo, R.; Dooley, K. L.; Doravari, S.; Edo, T. B.; Etzel, T.; Evans, T. M.; Fair, H.; Fernandez-Galiana, A.; Ferreira, E. C.; Fisher, R. P.; Fong, H.; Frey, R.; Frolov, V. V.; Fulda, P.; Fyffe, M.; Gateley, B.; Giaime, J. A.; Giardina, K. D.; Goetz, E.; Goetz, R.; Gras, S.; Gray, C.; Grote, H.; Gushwa, K. E.; Gustafson, E. K.; Gustafson, R.; Hall, E. D.; Hammond, G.; Hanks, J.; Hanson, J.; Hardwick, T.; Harry, G. M.; Heintze, M. C.; Heptonstall, A. W.; Hough, J.; Jones, R.; Kandhasamy, S.; Karki, S.; Kasprzack, M.; Kaufer, S.; Kennedy, R.; Kijbunchoo, N.; Kim, W.; King, E. J.; King, P. J.; Kissel, J. S.; Korth, W. Z.; Kuehn, G.; Landry, M.; Lantz, B.; Laxen, M.; Liu, J.; Lockerbie, N. A.; Lormand, M.; MacInnis, M.; Macleod, D. M.; Márka, S.; Márka, Z.; Markosyan, A. S.; Maros, E.; Marsh, P.; Martin, I. W.; Martynov, D. V.; Mason, K.; Massinger, T. J.; Matichard, F.; Mavalvala, N.; McCarthy, R.; McClelland, D. E.; McCormick, S.; McCuller, L.; McIver, J.; McManus, D. J.; McRae, T.; Mendell, G.; Merilh, E. L.; Meyers, P. M.; Mittleman, R.; Mogushi, K.; Moraru, D.; Moreno, G.; Mow-Lowry, C. M.; Mueller, G.; Mukund, N.; Mullavey, A.; Munch, J.; Nelson, T. J. N.; Nguyen, P.; Nuttall, L. K.; Oberling, J.; Oliver, M.; Oppermann, P.; Oram, Richard J.; O’Reilly, B.; Ottaway, D. J.; Overmier, H.; Palamos, J. R.; Parker, W.; Pele, A.; Penn, S.; Perez, C. J.; Phelps, M.; Pierro, V.; Pinto, I. M.; Pirello, M.; Principe, M.; Prokhorov, L. G.; Puncken, O.; Quetschke, V.; Quintero, E. A.; Radkins, H.; Raffai, P.; Ramirez, K. E.; Reid, S.; Reitze, D. H.; Robertson, N. A.; Rollins, J. G.; Roma, V. J.; Romel, C. L.; Romie, J. H.; Ross, M. P.; Rowan, S.; Ryan, K.; Sadecki, T.; Sanchez, E. J.; Sanchez, L. E.; Sandberg, V.; Savage, R. L.; Sellers, D.; Shaddock, D. A.; Shaffer, T. J.; Shapiro, B.; Shoemaker, D. H.; Slagmolen, B. J. J.; Smith, B.; Smith, J. R.; Sorazu, B.; Spencer, A. P.; Strain, K. A.; Tanner, D. B.; Taylor, R.; Thomas, M.; Thomas, P.; Thorne, K. A.; Thrane, E.; Toland, K.; Torrie, C. I.; Traylor, G.; Tse, M.; Tuyenbayev, D.; Vajente, G.; Valdes, G.; van Veggel, A. A.; Vass, S.; Vecchio, A.; Veitch, P. J.; Venkateswara, K.; Venugopalan, G.; Vo, T.; Vorvick, C.; Walker, M.; Ward, R. L.; Warner, J.; Weaver, B.; Weiss, R.; Weßels, P.; Willke, B.; Wipf, C. C.; Worden, J.; Yamamoto, H.; Yancey, C. C.; Yu, Hang; Yu, Haocun; Zhang, L.; Zucker, M. E.; Zweizig, J.en_US
dspace.embargo.termsNen_US
dspace.date.submission2019-04-04T10:36:22Z
mit.journal.volume99en_US
mit.journal.issue4en_US
mit.licensePUBLISHER_POLICYen_US


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