Zobrazeno 1 - 10
of 1 619
pro vyhledávání: '"Michael L. Katz"'
Autor:
Lorenzo Speri, Michael L. Katz, Alvin J. K. Chua, Scott A. Hughes, Niels Warburton, Jonathan E. Thompson, Christian E. A. Chapman-Bird, Jonathan R. Gair
Publikováno v:
Frontiers in Applied Mathematics and Statistics, Vol 9 (2024)
Extreme Mass Ratio Inspirals (EMRIs) are one of the key sources for future space-based gravitational wave interferometers. Measurements of EMRI gravitational waves are expected to determine the characteristics of their sources with sub-percent precis
Externí odkaz:
https://doaj.org/article/4f9ebcb5db56477595b18fff41f2e8d1
Autor:
Lorenzo Speri, Andrea Antonelli, Laura Sberna, Stanislav Babak, Enrico Barausse, Jonathan R. Gair, Michael L. Katz
Publikováno v:
Physical Review X, Vol 13, Iss 2, p 021035 (2023)
Gravitational-wave observations of extreme mass ratio inspirals (EMRIs) offer the opportunity to probe the environments of active galactic nuclei (AGN) through the torques that accretion disks induce on the binary. Within a Bayesian framework, we stu
Externí odkaz:
https://doaj.org/article/6cd45c4f3f19412c8bfc236a205fefc4
Autor:
Katz, Michael L.1
Publikováno v:
Federal Communications Law Journal. Feb2016, Vol. 68 Issue 1, p29-30. 2p.
Publikováno v:
Monthly Notices of the Royal Astronomical Society
Supermassive black holes (SMBHs) merging in dwarf galaxies will be detectable by the Laser Interferometer Space Antenna (LISA) in the mid-2030s. Previous cosmological hydrodynamic simulations have shown the prediction of massive black holes merging i
Publikováno v:
Physical Review D. 107
Publikováno v:
Physical Review D
The analysis of gravitational wave (GW) datasets is based on the comparison of measured time series with theoretical templates of the detector's response to a variety of source parameters. For LISA, the main scientific observables will be the so-call
Autor:
Michael L Katz, Camilla Danielski, Nikolaos Karnesis, Valeriya Korol, Nicola Tamanini, Neil J Cornish, Tyson B Littenberg
The Laser Interferometer Space Antenna (LISA) will detect and characterize ∼104 Galactic Binaries, consisting predominantly of two white dwarfs (WDs). An interesting prospect within this population is a third object – another WD star, a circumbin
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::99f2d80debf72ac86e14ad07d848f9d2
http://hdl.handle.net/10261/288642
http://hdl.handle.net/10261/288642
Autor:
Jan van Roestel, Thomas Kupfer, Ashish Mahabal, Kevin B. Burdge, Ben Rusholme, Yuhan Yao, Eric C. Bellm, Rick Burruss, Thomas A. Prince, Lynne A. Hillenbrand, Reed Riddle, Michael L. Katz, David L. Kaplan, Dmitry A. Duev, Andrew J. Drake, Przemek Mróz, Matthew J. Graham, Amruta Jaodand, Hector Rodriguez, Frank J. Masci, M. Rigault, Michael W. Coughlin, Richard Dekany, Jeffry Zolkower, Russ R. Laher
Publikováno v:
Mon.Not.Roy.Astron.Soc.
Mon.Not.Roy.Astron.Soc., 2021, 505 (2), pp.2954-2965. ⟨10.1093/mnras/stab1502⟩
Mon.Not.Roy.Astron.Soc., 2021, 505 (2), pp.2954-2965. ⟨10.1093/mnras/stab1502⟩
The current generation of all-sky surveys is rapidly expanding our ability to study variable and transient sources. These surveys, with a variety of sensitivities, cadences, and fields of view, probe many ranges of time-scale and magnitude. Data from
Autor:
Richard Gilbert, Michael L. Katz
Publikováno v:
SSRN Electronic Journal.
Publikováno v:
Physical Review D
We present the fastemriwaveforms (FEW) package, a collection of tools to build and analyze extreme mass ratio inspiral (EMRI) waveforms. Here, we expand on [A. J. K. Chua et al., Phys. Rev. Lett. 126, 051102 (2021).] that introduced the first fast an
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::20f14ee3bfb2b58bfe47b8345ef1fa86
https://resolver.caltech.edu/CaltechAUTHORS:20210927-213255697
https://resolver.caltech.edu/CaltechAUTHORS:20210927-213255697