Author: "Klein, Sr" / Topic: astronomical and space sciences - Searchworks@Jio Institute Digital Library Search Results

38 results on '"Klein, Sr"'

1. Triboelectric backgrounds to radio-based polar ultra-high energy neutrino (UHEN) experiments

Author: Aguilar, JA, Anker, A, Allison, P, Archambault, S, Baldi, P, Barwick, SW, Beatty, JJ, Beise, J, Besson, D, Bishop, A, Bondarev, E, Botner, O, Bouma, S, Buitink, S, Cataldo, M, Chen, CC, Chen, CH, Chen, P, Chen, YC, Choi, T, Clark, BA, Clay, W, Curtis-Ginsberg, Z, Connolly, A, Cremonesi, L, Dasgupta, P, Davies, J, de Kockere, S, de Vries, KD, Deaconu, C, DuVernois, MA, Flaherty, J, Friedman, E, Gaior, R, Gaswint, G, Glaser, C, Hallgren, A, Hallmann, S, Ham, Y-B, Hanson, JC, Harty, N, Hendricks, B, Hoffman, KD, Hong, E, Hornhuber, C, Hsu, SY, Hu, L, Huang, JJ, Huang, M-H, Hughes, K, Ishihara, A, Jee, G, Jung, J, Karle, A, Kelley, JL, Klein, SR, Kleinfelder, SA, Kim, J, Kim, K-C, Kim, M-C, Kravchenko, I, Krebs, R, Ku, Y, Kuo, CY, Kurusu, K, Kwon, Hyuck-Jin, Lahmann, R, Landsman, H, Latif, U, Lee, C, Leung, C-H, Li, C-J, Liu, J, Liu, T-C, Lu, M-Y, Madison, K, Mammo, J, Mase, K, McAleer, S, Meures, T, Meyers, ZS, Michaels, K, Mikhailova, M, Mulrey, K, Nam, J, Nichol, RJ, Nir, G, Nelles, A, Novikov, A, Nozdrina, A, Oberla, E, Oeyen, B, Osborn, J, Pan, Y, Pandya, H, Paul, MP, Persichilli, C, Pfendner, C, Plaisier, I, and Punsuebsay, N
Subjects: Particle and High Energy Physics, Physical Sciences, Neutrino, Ultra-high energy cosmic rays, Background rejection, Triboelectric effect, Astronomical and Space Sciences, Atomic, Molecular, Nuclear, Particle and Plasma Physics, Nuclear & Particles Physics, Astronomical sciences, Particle and high energy physics
Abstract: In the hopes of observing the highest-energy neutrinos (E>1 EeV) populating the Universe, both past (RICE, AURA, ANITA) and current (RNO-G, ARIANNA, ARA and TAROGE-M) polar-sited experiments exploit the impulsive radio emission produced by neutrino interactions. In such experiments, rare single event candidates must be unambiguously identified above backgrounds. Background rejection strategies to date primarily target thermal noise fluctuations and also impulsive radio-frequency signals of anthropogenic origin. In this paper, we consider the possibility that ‘fake’ neutrino signals may also be generated naturally via the ‘triboelectric effect.’ This broadly describes any process in which force applied at a boundary layer results in displacement of surface charge, leading to the production of an electrostatic potential difference ΔV. Wind blowing over granular surfaces such as snow can induce such a potential difference, with subsequent coronal discharge. Discharges over timescales as short as nanoseconds can then lead to radio-frequency emissions at characteristic MHz–GHz frequencies. Using data from various past (RICE, AURA, SATRA, ANITA) and current (RNO-G, ARIANNA and ARA) neutrino experiments, we find evidence for such backgrounds, which are generally characterized by: (a) a threshold wind velocity which likely depends on the experimental trigger criteria and layout; for the experiments considered herein, this value is typically O(10 m/s), (b) frequency spectra generally shifted to the low-end of the frequency regime to which current radio experiments are typically sensitive (100–200 MHz), (c) for the strongest background signals, an apparent preference for discharges from above-surface structures, although the presence of more isotropic, lower amplitude triboelectric discharges cannot be excluded.
Published: 2023

2. Measuring the polarization reconstruction resolution of the ARIANNA neutrino detector with cosmic rays

Author: collaboration, The ARIANNA, Anker, A, Baldi, P, Barwick, SW, Beise, J, Besson, DZ, Bouma, S, Cataldo, M, Chen, P, Gaswint, G, Glaser, C, Hallgren, A, Hallmann, S, Hanson, JC, Klein, SR, Kleinfelder, SA, Lahmann, R, Liu, J, Magnuson, M, McAleer, S, Meyers, ZS, Nam, J, Nelles, A, Novikov, A, Paul, MP, Persichilli, C, Plaisier, I, Pyras, L, Rice-Smith, R, Tatar, J, Wang, S-H, Welling, C, and Zhao, L
Subjects: cosmological neutrinos, neutrino astronomy, neutrino detectors, ultra high energy photons and neutrinos, Astronomical and Space Sciences, Atomic, Molecular, Nuclear, Particle and Plasma Physics, Nuclear & Particles Physics
Abstract: The ARIANNA detector is designed to detect neutrinos with energies above 1017 eV. Due to the similarities in generated radio signals, cosmic rays are often used as test beams for neutrino detectors. Some ARIANNA detector stations are equipped with antennas capable of detecting air showers. Since the radio emission properties of air showers are well understood, and the polarization of the radio signal can be predicted from the arrival direction, cosmic rays can be used as a proxy to assess the reconstruction capabilities of the ARIANNA neutrino detector. We report on dedicated efforts of reconstructing the polarization of cosmic-ray radio pulses. After correcting for difference in hardware, the two stations used in this study showed similar performance in terms of event rate and agreed with simulation. Subselecting high quality cosmic rays, the polarizations of these cosmic rays were reconstructed with a resolution of 2.5° (68% containment), which agrees with the expected value obtained from simulation. A large fraction of this resolution originates from uncertainties in the predicted polarization because of the contribution of the subdominant Askaryan effect in addition to the dominant geomagnetic emission. Subselecting events with a zenith angle greater than 70° removes most influence of the Askaryan emission, and, with limited statistics, we found the polarization uncertainty is reduced to 1.3° (68% containment).
Published: 2022

3. A search for cosmogenic neutrinos with the ARIANNA test bed using 4.5 years of data

Author: Anker, A, Barwick, SW, Bernhoff, H, Besson, DZ, Bingefors, N, García-Fernández, D, Gaswint, G, Glaser, C, Hallgren, A, Hanson, JC, Klein, SR, Kleinfelder, SA, Lahmann, R, Latif, U, Nam, J, Novikov, A, Nelles, A, Paul, MP, Persichilli, C, Plaisier, I, Prakash, T, Shively, SR, Tatar, J, Unger, E, Wang, S-H, and Welling, C
Subjects: Nuclear and Plasma Physics, Particle and High Energy Physics, Physical Sciences, Affordable and Clean Energy, cosmological neutrinos, neutrino astronomy, neutrino experiments, ultra high energy photons and neutrinos, astro-ph.IM, astro-ph.HE, Astronomical and Space Sciences, Atomic, Molecular, Nuclear, Particle and Plasma Physics, Nuclear & Particles Physics, Astronomical sciences, Particle and high energy physics
Abstract: The primary mission of the ARIANNA ultra-high energy neutrino telescope is to uncover astrophysical sources of neutrinos with energies greater than 1016 eV. A pilot array, consisting of seven ARIANNA stations located on the surface of the Ross Ice Shelf in Antarctica, was commissioned in November 2014. We report on the search for astrophysical neutrinos using data collected between November 2014 and February 2019. A straight-forward template matching analysis yielded no neutrino candidates, with a signal efficiency of 79%. We find a 90% confidence upper limit on the diffuse neutrino flux of E2Φ=1.7× 10-6 GeV cm-2s-1sr-1 for a decade wide logarithmic bin centered at a neutrino energy of 1018,eV, which is an order of magnitude improvement compared to the previous limit reported by the ARIANNA collaboration. The ARIANNA stations, including purpose built cosmic-ray stations at the Moore's Bay site and demonstrator stations at the South Pole, have operated reliably. Sustained operation at two distinct sites confirms that the flexible and adaptable architecture can be deployed in any deep ice, radio quiet environment. We show that the scientific capabilities, technical innovations, and logistical requirements of ARIANNA are sufficiently well understood to serve as the basis for large area radio-based neutrino telescope with a wide field-of-view.
Published: 2020

4. Targeting ultra-high energy neutrinos with the ARIANNA experiment

Author: Anker, A, Barwick, SW, Bernhoff, H, Besson, DZ, Bingefors, N, Gaswint, G, Glaser, C, Hallgren, A, Hanson, JC, Lahmann, R, Latif, U, Nam, J, Novikov, A, Klein, SR, Kleinfelder, SA, Nelles, A, Paul, MP, Persichilli, C, Shively, SR, Tatar, J, Unger, E, Wang, SH, and Yodh, G
Subjects: Neutrino, Radio, Antarctica, Cosmic ray, Askaryan radiation, ARIANNA, astro-ph.IM, astro-ph.HE, 85-06, Aerospace & Aeronautics, Astronomical and Space Sciences, Aerospace Engineering, Mechanical Engineering
Abstract: The measurement of ultra-high energy (UHE) neutrinos (E > 1016 eV) opens a new field of astronomy with the potential to reveal the sources of ultra-high energy cosmic rays especially if combined with observations in the electromagnetic spectrum and gravitational waves. The ARIANNA pilot detector explores the detection of UHE neutrinos with a surface array of independent radio detector stations in Antarctica which allows for a cost-effective instrumentation of large volumes. Twelve stations are currently operating successfully at the Moore's Bay site (Ross Ice Shelf) in Antarctica and at the South Pole. We will review the current state of ARIANNA and its main results. We report on a newly developed wind generator that successfully operates in the harsh Antarctic conditions and powers the station for a substantial time during the dark winter months. The robust ARIANNA surface architecture, combined with environmentally friendly solar and wind power generators, can be installed at any deep ice location on the planet and operated autonomously. We report on the detector capabilities to determine the neutrino direction by reconstructing the signal arrival direction of a 800 m deep calibration pulser, and the reconstruction of the signal polarization using the more abundant cosmic-ray air showers. Finally, we describe a large-scale design – ARIA – that capitalizes on the successful experience of the ARIANNA operation and is designed sensitive enough to discover the first UHE neutrino.
Published: 2019

5. Neutrino vertex reconstruction with in-ice radio detectors using surface reflections and implications for the neutrino energy resolution

Author: Anker, A, Barwick, SW, Bernhoff, H, Besson, DZ, Bingefors, N, García-Fernández, D, Gaswint, G, Glaser, C, Hallgren, A, Hanson, JC, Klein, SR, Kleinfelder, SA, Lahmann, R, Latif, U, Nam, J, Novikov, A, Nelles, A, Paul, MP, Persichilli, C, Plaisier, I, Prakash, T, Shively, SR, Tatar, J, Unger, E, Wang, S-H, Welling, C, and Zierke, S
Subjects: Nuclear and Plasma Physics, Particle and High Energy Physics, Physical Sciences, neutrino astronomy, neutrino detectors, neutrino experiments, ultra high energy photons and neutrinos, astro-ph.IM, Astronomical and Space Sciences, Atomic, Molecular, Nuclear, Particle and Plasma Physics, Nuclear & Particles Physics, Astronomical sciences, Particle and high energy physics
Abstract: Ultra high energy neutrinos (Eν > 1016.5eV) are efficiently measured via radio signals following a neutrino interaction in ice. An antenna placed1(15 m) below the ice surface will measure two signals for the vast majority of events (90% at Eν=1018 eV): a direct pulse and a second delayed pulse from a reflection off the ice surface. This allows for a unique identification of neutrinos against backgrounds arriving from above. Furthermore, the time delay between the direct and reflected signal (D'n'R) correlates with the distance to the neutrino interaction vertex, a crucial quantity to determine the neutrino energy. In a simulation study, we derive the relation between time delay and distance and study the corresponding experimental uncertainties in estimating neutrino energies. We find that the resulting contribution to the energy resolution is well below the natural limit set by the unknown inelasticity in the initial neutrino interaction. We present an in-situ measurement that proves the experimental feasibility of this technique. Continuous monitoring of the local snow accumulation in the vicinity of the transmit and receive antennas using this technique provide a precision of (1 mm) in surface elevation, which is much better than that needed to apply the D'n'R technique to neutrinos.
Published: 2019

6. Observation of classically 'forbidden' electromagnetic wave propagation and implications for neutrino detection.

Author: Barwick, SW, Berg, EC, Besson, DZ, Gaswint, G, Glaser, C, Hallgren, A, Hanson, JC, Klein, SR, Kleinfelder, S, Köpke, L, Kravchenko, I, Lahmann, R, Latif, U, Nam, J, Nelles, A, Persichilli, C, Sandstrom, P, Tatar, J, and Unger, E
Subjects: cosmic ray experiments, ultra high energy photons and neutrinos, Nuclear & Particles Physics, Astronomical and Space Sciences, Atomic, Molecular, Nuclear, Particle and Plasma Physics, Atomic, Molecular, Nuclear, Particle and Plasma Physics
Abstract: Ongoing experimental efforts in Antarctica seek to detect ultra-high energy neutrinos by measurement of radio-frequency (RF) Askaryan radiation generated by the collision of a neutrino with an ice molecule. An array of RF antennas, deployed either in-ice or in-air, is used to infer the properties of the neutrino. To evaluate their experimental sensitivity, such experiments require a refractive index model for ray tracing radio-wave trajectories from a putative in-ice neutrino interaction point to the receiving antennas; this gives the degree of signal absorption or ray bending from source to receiver. The gradient in the density profile over the upper 200 meters of Antarctic ice, coupled with Fermat's least-time principle, implies ray "bending" and the existence of "forbidden" zones for predominantly horizontal signal propagation at shallow depths. After re-deriving the formulas describing such shadowing, we report on experimental results that, somewhat unexpectedly, demonstrate the existence of electromagnetic wave transport modes from nominally shadowed regions. The fact that this shadow-signal propagation is observed both at South Pole and the Ross Ice Shelf in Antarctica suggests that the effect may be a generic property of polar ice, with potentially important implications for experiments seeking to detect neutrinos.
Published: 2018

7. Observation of classically `forbidden' electromagnetic wave propagation and implications for neutrino detection.

Author: Barwick, SW, Berg, EC, Besson, DZ, Gaswint, G, Glaser, C, Hallgren, A, Hanson, JC, Klein, SR, Kleinfelder, S, Köpke, L, Kravchenko, I, Lahmann, R, Latif, U, Nam, J, Nelles, A, Persichilli, C, Sandstrom, P, Tatar, J, and Unger, E
Subjects: Particle and High Energy Physics, Astronomical Sciences, Physical Sciences, cosmic ray experiments, ultra high energy photons and neutrinos, Astronomical and Space Sciences, Atomic, Molecular, Nuclear, Particle and Plasma Physics, Nuclear & Particles Physics, Astronomical sciences, Particle and high energy physics
Abstract: Ongoing experimental efforts in Antarctica seek to detect ultra-high energy neutrinos by measurement of radio-frequency (RF) Askaryan radiation generated by the collision of a neutrino with an ice molecule. An array of RF antennas, deployed either in-ice or in-air, is used to infer the properties of the neutrino. To evaluate their experimental sensitivity, such experiments require a refractive index model for ray tracing radio-wave trajectories from a putative in-ice neutrino interaction point to the receiving antennas; this gives the degree of signal absorption or ray bending from source to receiver. The gradient in the density profile over the upper 200 meters of Antarctic ice, coupled with Fermat's least-time principle, implies ray "bending" and the existence of "forbidden" zones for predominantly horizontal signal propagation at shallow depths. After re-deriving the formulas describing such shadowing, we report on experimental results that, somewhat unexpectedly, demonstrate the existence of electromagnetic wave transport modes from nominally shadowed regions. The fact that this shadow-signal propagation is observed both at South Pole and the Ross Ice Shelf in Antarctica suggests that the effect may be a generic property of polar ice, with potentially important implications for experiments seeking to detect neutrinos.
Published: 2018

8. Ultra-peripheral collisions and hadronic structure

Author: Klein, SR
Subjects: ultra-peripheral collisions, photoproduction, quarkonium, nuclear structure, RHIC, LHC, Nuclear & Particles Physics, Astronomical and Space Sciences, Atomic, Molecular, Nuclear, Particle and Plasma Physics, Quantum Physics
Abstract: Ultra-peripheral collisions are the energy frontier for photon-mediated interactions, reaching, at the Large Hadron Collider (LHC), γ−p center of mass energies five to ten times higher than at HERA and reaching γγ energies higher than at LEP. Photoproduction of heavy quarkonium and dijets in pp and pA collisions probes the gluon distribution in protons at Bjorken-x values down to 3×10−6, far smaller than can be otherwise studied. In AA collisions, these reactions probe the gluon distributions in heavy ions, down to x values of a few 10−5. Although more theoretical work is needed to nail down all of the uncertainties, inclusion of these data in current parton distribution function fits would greatly improve the accuracy of the gluon distributions at low Bjorken-x and low/moderate Q2. High-statistics ρ0 data probe the spatial distribution of the interaction sites; the site distribution is given by the Fourier transform of dσ/dt. After introducing UPCs, this review presents recent measurements of dilepton production and light-by-light scattering and recent data on proton and heavy nuclei structure, emphasizing results presented at Quark Matter 2017 (QM2017).
Published: 2017

9. Radio detection of air showers with the ARIANNA experiment on the Ross Ice Shelf

Author: Barwick, SW, Besson, DZ, Burgman, A, Chiem, E, Hallgren, A, Hanson, JC, Klein, SR, Kleinfelder, SA, Nelles, A, Persichilli, C, Phillips, S, Prakash, T, Reed, C, Shively, SR, Tatar, J, Unger, E, Walker, J, and Yodh, G
Subjects: Nuclear and Plasma Physics, Particle and High Energy Physics, Physical Sciences, Cosmic rays, Neutrinos, Radio emission, 98.70.Sa, 95.85.Ry, 95.55.Vj, 95.55.Jz, Astronomical and Space Sciences, Atomic, Molecular, Nuclear, Particle and Plasma Physics, Nuclear & Particles Physics, Astronomical sciences, Particle and high energy physics
Abstract: The ARIANNA hexagonal radio array (HRA) is an experiment in its pilot phase designed to detect cosmogenic neutrinos of energies above 1016 eV. The most neutrino-like background stems from the radio emission of air showers. This article reports on dedicated efforts of simulating and detecting the signals of cosmic rays. A description of the fully radio self-triggered data-set, the properties of the detected air shower signals in the frequency range of 100–500 MHz and the consequences for neutrino detection are given. 38 air shower signals are identified by their distinct waveform characteristics, are in good agreement with simulations and their signals provide evidence that neutrino-induced radio signals will be distinguishable with high efficiency in ARIANNA. The cosmic ray flux at a mean energy of 6.5−1.0+1.2×1017 eV is measured to be 1.1−0.7+1.0×10−16 eV−1 km−2 sr−1 yr−1 and one five-fold coincident event is used to illustrate the capabilities of the ARIANNA detector to reconstruct arrival direction and energy of air showers.
Published: 2017

10. Characteristics of Cherenkov radiation in naturally occurring ice

Author: Mikkelsen, RE, Poulsen, T, Uggerhøj, UI, and Klein, SR
Subjects: Nuclear and Plasma Physics, Physical Sciences, Astronomical and Space Sciences, Atomic, Molecular, Nuclear, Particle and Plasma Physics, Quantum Physics, Nuclear & Particles Physics, Mathematical physics, Astronomical sciences, Particle and high energy physics
Abstract: We revisit the theory of Cherenkov radiation in uniaxial crystals. Historically, a number of flawed attempts have been made at explaining this radiation phenomenon, and a consistent error-free description is nowhere available. We apply our calculation to a large modern day telescope - IceCube. Located in Antarctica, this detector makes use of the naturally occurring ice as a medium to generate Cherenkov radiation. However, due to the high pressure at the depth of the detector site, large volumes of hexagonal ice crystals are formed. We calculate how this affects the Cherenkov radiation yield and angular dependence. We conclude that the effect is small, at most about a percent, and would only be relevant in future high-precision instruments like e.g. Precision IceCube Next Generation Upgrade (PINGU). For radio-Cherenkov experiments which use the presence of a clear Cherenkov cone to determine the arrival direction, any variation in emission angle will directly and linearly translate into a change in apparent neutrino direction. In closing, we also describe a simple experiment to test this formalism and calculate the impact of anisotropy on light yields from lead tungstate crystals as used, for example, in the CMS calorimeter at the CERN LHC.
Published: 2016

11. A first search for cosmogenic neutrinos with the ARIANNA Hexagonal Radio Array

Author: Barwick, SW, Berg, EC, Besson, DZ, Binder, G, Binns, WR, Boersma, DJ, Bose, RG, Braun, DL, Buckley, JH, Bugaev, V, Buitink, S, Dookayka, K, Dowkontt, PF, Duffin, T, Euler, S, Gerhardt, L, Gustafsson, L, Hallgren, A, Hanson, JC, Israel, MH, Kiryluk, J, Klein, SR, Kleinfelder, S, Niederhausen, H, Olevitch, MA, Persichelli, C, Ratzlaff, K, Rauch, BF, Reed, C, Roumi, M, Samanta, A, Simburger, GE, Stezelberger, T, Tatar, J, Uggerhoj, UI, Walker, J, Yodh, G, Young, R, and Collaboration, ARIANNA
Subjects: Radio, Antarctica, Neutrino, Cosmogenic, GZK, High energy, astro-ph.HE, astro-ph.IM, Astronomical and Space Sciences, Atomic, Molecular, Nuclear, Particle and Plasma Physics, Nuclear & Particles Physics
Abstract: The ARIANNA experiment seeks to observe the diffuse flux of neutrinos in the 108-1010 GeV energy range using a grid of radio detectors at the surface of the Ross Ice Shelf of Antarctica. The detector measures the coherent Cherenkov radiation produced at radio frequencies, from about 100 MHz-1 GHz, by charged particle showers generated by neutrino interactions in the ice. The ARIANNA Hexagonal Radio Array (HRA) is being constructed as a prototype for the full array. During the 2013-14 austral summer, three HRA stations collected radio data which was wirelessly transmitted off site in nearly real-time. The performance of these stations is described and a simple analysis to search for neutrino signals is presented. The analysis employs a set of three cuts that reject background triggers while preserving 90% of simulated cosmogenic neutrino triggers. No neutrino candidates are found in the data and a model-independent 90% confidence level Neyman upper limit is placed on the all flavor ν+ν¯ flux in a sliding decade-wide energy bin. The limit reaches a minimum of 1.9×10-23GeV-1cm-2s-1sr-1 in the 108.5-109.5 GeV energy bin. Simulations of the performance of the full detector are also described. The sensitivity of the full ARIANNA experiment is presented and compared with current neutrino flux models.
Published: 2015

12. Time-domain response of the ARIANNA detector

Author: Barwick, SW, Berg, EC, Besson, DZ, Duffin, T, Hanson, JC, Klein, SR, Kleinfelder, SA, Piasecki, M, Ratzlaff, K, Reed, C, Roumi, M, Stezelberger, T, Tatar, J, Walker, J, Young, R, and Zou, L
Subjects: GZK neutrinos, Askaryan effect, Radio detector, astro-ph.IM, astro-ph.HE, Astronomical and Space Sciences, Atomic, Molecular, Nuclear, Particle and Plasma Physics, Nuclear & Particles Physics
Abstract: The Antarctic Ross Ice Shelf Antenna Neutrino Array (ARIANNA) is a high-energy neutrino detector designed to record the Askaryan electric field signature of cosmogenic neutrino interactions in ice. To understand the inherent radio-frequency (RF) neutrino signature, the time-domain response of the ARIANNA RF receiver must be measured. ARIANNA uses Create CLP5130-2N log-periodic dipole arrays (LPDAs). The associated effective height operator converts incident electric fields to voltage waveforms at the LDPA terminals. The effective height versus time and incident angle was measured, along with the associated response of the ARIANNA RF amplifier. The results are verified by correlating to field measurements in air and ice, using oscilloscopes. Finally, theoretical models for the Askaryan electric field are combined with the detector response to predict the neutrino signature.
Published: 2015

13. Review of Particle Physics: Particle data group

Author: Hagiwara, K, Hikasa, K, Nakamura, K, Tanabashi, M, Aguilar-Benitez, M, Amsler, C, Barnett, RM, Burchat, PR, Carone, CD, Caso, C, Conforto, G, Dahl, O, Doser, M, Eidelman, S, Feng, JL, Gibbons, L, Goodman, M, Grab, C, Groom, DE, Gurtu, A, Hayes, KG, Hernández-Rey, JJ, Honscheid, K, Kolda, C, Mangano, ML, Manley, DM, Manohar, AV, March-Russell, J, Masoni, A, Miquel, R, Mönig, K, Murayama, H, Navas, S, Olive, KA, Pape, L, Patrignani, C, Piepke, A, Roos, M, Terning, J, Törnqvist, NA, Trippe, TG, Vogel, P, Wohl, CG, Workman, RL, Yao, WM, Armstrong, B, Gee, PS, Lugovsky, KS, Lugovsky, SB, Lugovsky, VS, Artuso, M, Asner, D, Babu, KS, Barberio, E, Battaglia, M, Bichsel, H, Biebel, O, Bloch, P, Cahn, RN, Cattai, A, Chivukula, RS, Cousins, RD, Cowan, G, Damour, T, Desler, K, Donahue, RJ, Edwards, DA, Elvira, VD, Erler, J, Ezhela, VV, Fassó, A, Fetscher, W, Fields, BD, Foster, B, Froidevaux, D, Fukugita, M, Gaisser, TK, Garren, L, Gerber, HJ, Gilman, FJ, Haber, HE, Hagmann, C, Hewett, J, Hinchliffe, I, Hogan, CJ, Höhler, G, Igo-Kemenes, P, Jackson, JD, Johnson, KF, Karlen, D, Kayser, B, Klein, SR, Kleinknecht, K, Knowles, IG, Kreitz, P, Kuyanov, YV, Landua, R, Langacker, P, Littenberg, L, and Martin, AD
Subjects: Nuclear & Particles Physics, Astronomical and Space Sciences, Atomic, Molecular, Nuclear, Particle and Plasma Physics, Quantum Physics, Atomic, Molecular, Nuclear, Particle and Plasma Physics
Abstract: This biennial Review summarizes much of Particle Physics. Using data from previous editions, plus 2205 new measurements from 667 papers, we list, evaluate, and average measured properties of gauge bosons, leptons, quarks, mesons, and baryons. We also summarize searches for hypothetical particles such as Higgs bosons, heavy neutrinos, and supersymmetric particles. All the particle properties and search limits are listed in Summary Tables. We also give numerous tables, figures, formulae, and reviews of topics such as the Standard Model, particle detectors, probability, and statistics. This edition features expanded coverage of CP violation in B mesons and of neutrino oscillations. For the first time we cover searches for evidence of extra dimensions (both in the particle listings and in a new review). Another new review is on Grand Unified Theories. A booklet is available containing the Summary Tables and abbreviated versions of some of the other sections of this full Review. All tables, listings, and reviews (and errata) are also available on the Particle Data Group website: http://pdg.lbl.gov.
Published: 2002

14. Measurement of the total hadronic cross section in e+e- annihilation at s=29 GeV

Author: von Zanthier, C, de Boer, W, Grindhammer, G, Hylen, J, Harral, B, Hearty, C, Labarga, L, Matthews, J, Schaad, M, Abrams, G, Adolphsen, CE, Akerlof, C, Alexander, JP, Alvarez, M, Baden, AR, Ballam, J, Barish, BC, Barklow, T, Barnett, BA, Bartelt, J, Blockus, D, Bonvicini, G, Boyarski, A, Boyer, J, Brabson, B, Breakstone, A, Brom, JM, Bulos, F, Burchat, PR, Burke, DL, Butler, F, Calvino, F, Cence, RJ, Chapman, J, Cords, D, Coupal, DP, DeStaebler, HC, Dorfan, DE, Dorfan, JM, Drell, PS, Feldman, GJ, Fernandez, E, Field, RC, Ford, WT, Fordham, C, Frey, R, Fujino, D, Gan, KK, Gidal, G, Glanzman, T, Goldhaber, G, Green, A, Grosse-Wiesmann, P, Haggerty, J, Hanson, G, Harr, R, Harris, FA, Hawkes, CM, Hayes, K, Herrup, D, Heusch, CA, Himel, T, Hoenk, M, Hutchinson, D, Innes, WR, Jaffre, M, Jaros, JA, Juricic, I, Kadyk, JA, Karlen, D, Kent, J, Klein, SR, Koska, W, Kozanecki, W, Lankford, AJ, Larsen, RR, Levi, ME, Li, Z, Litke, AM, Lüth, V, Meyer, DI, Milliken, BD, Moffeit, KC, Müller, L, Nash, J, Nelson, ME, Nitz, D, Ogren, H, O'Shaughnessy, KF, Parker, SI, Peck, C, Perl, ML, Petersen, A, Petradza, M, Porter, FC, Rankin, P, Riles, K, Rust, DR, Sadrozinski, HFW, and Schalk, TL
Subjects: Nuclear and Plasma Physics, Particle and High Energy Physics, Mathematical Physics, Mathematical Sciences, Physical Sciences, Astronomical and Space Sciences, Atomic, Molecular, Nuclear, Particle and Plasma Physics, Quantum Physics, Nuclear & Particles Physics, Mathematical physics, Astronomical sciences, Particle and high energy physics
Abstract: A precise measurement of the ratio R of the total cross section e+e-hadrons to the pointlike cross section e+e-+- at a center-of-mass energy of 29.0 GeV is presented. The data were taken with the upgraded Mark II detector at the SLAC storage ring PEP. The result is R=3.920.050.09. The luminosity has been determined with three independent luminosity monitors measuring Bhabha scattering at different angular intervals. Recent calculations of higher-order QED radiative corrections are used to estimate the systematic error due to missing higher-order radiative corrections in the Monte Carlo event generators. © 1991 The American Physical Society.
Published: 1991

15. Test of QED to fourth order by study of four-lepton final states in e+e- interactions at 29 GeV with the Mark II detector

Author: Petradza, M, Thun, R, Abrams, G, Amidei, D, Baden, AR, Barklow, T, Boyarski, A, Boyer, J, Burchat, PR, Burke, DL, Butler, F, Dorfan, JM, Feldman, GJ, Gidal, G, Gladney, L, Gold, MS, Goldhaber, G, Haggerty, J, Hanson, G, Hayes, K, Herrup, D, Himel, T, Hollebeek, RJ, Innes, WR, Jaros, JA, Kadyk, JA, Karlen, D, Klein, SR, Lankford, AJ, Larsen, RR, LeClaire, BW, Levi, ME, Lockyer, NS, Lüth, V, Nelson, ME, Ong, RA, Perl, ML, Richter, B, Riles, K, Rowson, PC, Schaad, T, Schellman, H, Schmidke, WB, Sheldon, PD, Trilling, GH, Wood, DR, and Yelton, JM
Subjects: Astronomical and Space Sciences, Atomic, Molecular, Nuclear, Particle and Plasma Physics, Quantum Physics, Nuclear & Particles Physics
Abstract: We have tested QED to fourth order in the coupling constant in the large-Q2 region by studying four-lepton final states in e+e- interactions with the Mark II detector at the SLAC storage ring PEP (s=29 GeV). All four final-state particles were detected at large angles with respect to the beam axis. For an integrated luminosity of 205 pb-1, we observed ten e+e-e+e-, ten e+e-+-, and one events with opposite-charge pair masses greater than 1 GeV/c2. These events show good agreement with the complete 4 QED calculation. © 1990 The American Physical Society.
Published: 1990

16. Measurement of the two-photon width of the eta '(958).

Author: Butler, F, Boyer, J, Gidal, G, Abrams, G, Amidei, D, Baden, AR, Gold, MS, Goldhaber, G, Golding, L, Haggerty, J, Herrup, D, Juricic, I, Kadyk, JA, Levi, ME, Nelson, ME, Rowson, PC, Schellman, H, Schmidke, WB, Sheldon, PD, Trilling, GH, Wood, DR, Riles, K, Perl, ML, Barklow, T, Boyarski, A, Burchat, PR, Burke, DL, Dorfan, JM, Feldman, GJ, Gladney, L, Hanson, G, Hayes, K, Hollebeek, RJ, Innes, WR, Jaros, JA, Karlen, D, Klein, SR, Lankford, AJ, Larsen, RR, LeClaire, BW, Lockyer, NS, Lüth, V, Ong, RA, Richter, B, Yelton, JM, and Schaad, T
Subjects: Nuclear & Particles Physics, Astronomical and Space Sciences, Atomic, Molecular, Nuclear, Particle and Plasma Physics, Quantum Physics
Abstract: Using 203 pb-1 of data collected by the Mark II detector at the SLAC storage ring PEP, we have measured the radiative width of the for quasireal photons. The width is separately measured in the three reactions e+e-e+e-0+-,0; e+e-e+e-0+-; 0+-(0,), and e+e-e+e-0, giving a statistically weighted average two-photon width of=4.57±0.25±0.44 keV. As a byproduct of the study of the decay mode, we also measured the two-photon decay width of the a2(1320) as a2(1320)=1.03±0.13±0.21 keV. © 1990 The American Physical Society.
Published: 1990

17. Measurement of the two-photon width of the η′(958)

Author: Butler, F, Boyer, J, Gidal, G, Abrams, G, Amidei, D, Baden, AR, Gold, MS, Goldhaber, G, Golding, L, Haggerty, J, Herrup, D, Juricic, I, Kadyk, JA, Levi, ME, Nelson, ME, Rowson, PC, Schellman, H, Schmidke, WB, Sheldon, PD, Trilling, GH, Wood, DR, Riles, K, Perl, ML, Barklow, T, Boyarski, A, Burchat, PR, Burke, DL, Dorfan, JM, Feldman, GJ, Gladney, L, Hanson, G, Hayes, K, Hollebeek, RJ, Innes, WR, Jaros, JA, Karlen, D, Klein, SR, Lankford, AJ, Larsen, RR, LeClaire, BW, Lockyer, NS, Lüth, V, Ong, RA, Richter, B, Yelton, JM, and Schaad, T
Subjects: Astronomical and Space Sciences, Atomic, Molecular, Nuclear, Particle and Plasma Physics, Quantum Physics, Nuclear & Particles Physics
Abstract: Using 203 pb-1 of data collected by the Mark II detector at the SLAC storage ring PEP, we have measured the radiative width of the for quasireal photons. The width is separately measured in the three reactions e+e-e+e-0+-,0; e+e-e+e-0+-; 0+-(0,), and e+e-e+e-0, giving a statistically weighted average two-photon width of=4.57±0.25±0.44 keV. As a byproduct of the study of the decay mode, we also measured the two-photon decay width of the a2(1320) as a2(1320)=1.03±0.13±0.21 keV. © 1990 The American Physical Society.
Published: 1990

18. Search for a nearly degenerate lepton doublet (L-,L0).

Author: Riles, K, Perl, ML, Barklow, T, Boyarski, A, Burchat, PR, Burke, DL, Dorfan, JM, Feldman, GJ, Gladney, L, Hanson, G, Hayes, K, Hollebeek, RJ, Innes, WR, Jaros, JA, Karlen, D, Klein, SR, Lankford, AJ, Larsen, RR, LeClaire, BW, Lockyer, NS, Lüth, V, Ong, RA, Richter, B, Yelton, JM, Abrams, G, Amidei, D, Baden, AR, Boyer, J, Butler, F, Gidal, G, Gold, MS, Goldhaber, G, Golding, L, Haggerty, J, Herrup, D, Juricic, I, Kadyk, JA, Levi, ME, Nelson, ME, Rowson, PC, Schellman, H, Schmidke, WB, Sheldon, PD, Trilling, GH, Wood, DR, and Schaad, T
Subjects: Nuclear & Particles Physics, Astronomical and Space Sciences, Atomic, Molecular, Nuclear, Particle and Plasma Physics, Quantum Physics
Abstract: We have searched for a heavy charged lepton with an associated neutrino of nearly the same mass in e+e- annihilation data taken with the Mark II detector at a center-of-mass energy of 29 GeV. In order to suppress contamination from conventional two-photon reactions, this analysis uses a novel, radiative-tagging technique. Requiring the presence of an isolated, energetic photon allows a search for lepton doublets with mass splittings smaller than that previously accessible to experiment. No evidence for such a new lepton doublet has been found, enabling limits to be placed on allowed mass combinations. Mass splittings as low as 250-400 MeV/c2 are excluded for charged-lepton masses between 500 MeV/c2 and 10 GeV/c2. © 1990 The American Physical Society.
Published: 1990

19. Search for decays of the Z to unstable neutral leptons with mass between 2.5 and 22 GeV

Author: Burchat, PR, King, M, Abrams, GS, Adolphsen, CE, Averill, D, Ballam, J, Barish, BC, Barklow, T, Barnett, BA, Bartelt, J, Bethke, S, Blockus, D, Bonvicini, G, Boyarski, A, Brabson, B, Breakstone, A, Bulos, F, Burke, DL, Cence, RJ, Chapman, J, Chmeissani, M, Cords, D, Coupal, DP, Dauncey, P, DeStaebler, HC, Dorfan, DE, Dorfan, JM, Drewer, DC, Elia, R, Feldman, GJ, Fernandes, D, Field, RC, Ford, WT, Fordham, C, Frey, R, Fujino, D, Gan, KK, Gatto, C, Gero, E, Gidal, G, Glanzman, T, Goldhaber, G, Cadenas, JJ Gomez, Gratta, G, Grindhammer, G, Grosse-Wiesmann, P, Hanson, G, Harr, R, Harral, B, Harris, FA, Hawkes, CM, Hayes, K, Hearty, C, Heusch, CA, Hildreth, MD, Himel, T, Hinshaw, DA, Hong, SJ, Hutchinson, D, Hylen, J, Innes, WR, Jacobsen, RG, Jaros, JA, Jung, CK, Kadyk, JA, Kent, J, Klein, SR, Koetke, DS, Komamiya, S, Koska, W, Kowalski, LA, Kozanecki, W, Kral, JF, Kuhlen, M, Labarga, L, Lankford, AJ, Larsen, RR, Le Diberder, F, Levi, ME, Litke, AM, Lou, XC, Lüth, V, McKenna, JA, Matthews, JAJ, Mattison, T, Milliken, BD, Moffeit, KC, Munger, CT, Murray, WN, Nash, J, Ogren, H, O'Shaughnessy, KF, Parker, SI, Peck, C, Perl, ML, Perrier, F, Petradza, M, Pitthan, R, Porter, FC, and Rankin, P
Subjects: Nuclear and Plasma Physics, Particle and High Energy Physics, Physical Sciences, Astronomical and Space Sciences, Atomic, Molecular, Nuclear, Particle and Plasma Physics, Quantum Physics, Nuclear & Particles Physics, Mathematical physics, Astronomical sciences, Particle and high energy physics
Abstract: Using the sample of neutral vector bosons (Z's) produced at the SLAC Linear Collider and detected with the Mark II detector, we search for the decay of the Z to a pair of particles, one of which decays to two charged particles. The observed number of Z decays with this signature excludes, at a confidence level greater than 95%, the decay of the Z to a pair of fourth-generation Dirac neutrinos with mass between 2.5 and 22 GeV, a decay length less than about 1 cm, and coupling to any of the first three generations of charged leptons. This is the first time the existence of such a lepton coupling to the ± has been excluded by a direct search. © 1990 The American Physical Society.
Published: 1990

20. A reanalysis of B0-B̄0 mixing in e+e- annihilation at 29 GeV

Author: Weir, AJ, Abrams, G, Adolphsen, CE, Alexander, JP, Alvarez, M, Amidei, D, Baden, AR, Barish, BC, Barklow, T, Barnett, BA, Bartelt, I, Blockus, D, Bonvicini, G, Boyarski, A, Boyer, J, Brabson, B, Breakstone, A, Brom, JM, Bulos, F, Burchat, PR, Burke, DL, Butler, F, Calvino, F, Cence, RJ, Chapman, J, Cords, D, Coupal, DP, Destaebler, HC, Dorfan, DE, Dorfan, JM, Drell, PS, Feldman, GJ, Fernandez, E, Field, RC, Ford, WT, Fordham, C, Frey, R, Fujino, D, Gan, KK, Gidal, G, Gladney, L, Glanzman, T, Gold, MS, Goldhaber, G, Green, A, Grosse-Wiesmann, P, Haggerty, J, Hanson, G, Harr, R, Harris, FA, Hawkes, CM, Hayes, K, Herrup, D, Heusch, CA, Himel, T, Hollebeek, RJ, Hutchinson, D, Hylef, J, Innes, WR, Jaffre, M, Jaros, JA, Juricic, I, Kadyk, JA, Karlen, D, Kent, J, Klein, SR, Koska, W, Kozanecki, W, Lankford, AJ, Larsen, RR, LeClaire, BW, Levi, ME, Litke, AM, Lockyer, NS, Lüth, V, Matthews, JAJ, Meyer, DI, Milliken, BD, Moffeit, KC, Müller, L, Nash, J, Nelson, ME, Nitz, D, Ogren, H, Ong, RA, O'Shaughnessy, KF, Parker, SI, Peck, C, Perl, ML, Petersen, A, Petradza, M, Porter, FC, Rankin, P, Richter, B, Riles, K, Rowson, PC, Rust, DR, Sadrozinski, HFW, Schaad, T, and Schalk, TL
Subjects: Nuclear & Particles Physics, Atomic, Molecular, Nuclear, Particle and Plasma Physics, Astronomical and Space Sciences, Mathematical Physics, Atomic, Molecular, Nuclear, Particle and Plasma Physics
Abstract: Data taken by the Mark II detector at the PEP storage ring was used to measure the rate of dilepton production in multihadronic events produced by e+e- annihilation at √s=29 GeV. We determine the probability that a hadron initially containing a b (b̄) quark decays to a positive (negative) lepton to be 0.17-0.08+0.15, with 90% confidence level limits of 0.06 and 0.38. © 1990.
Published: 1990

21. Radiative tau production and decay.

Author: Wu, DY, Hayes, K, Perl, ML, Barklow, T, Boyarski, A, Burchat, PR, Burke, DL, Dorfan, JM, Feldman, GJ, Gladney, L, Hanson, G, Hollebeek, RJ, Innes, WR, Jaros, JA, Karlen, D, Klein, SR, Lankford, AJ, Larsen, RR, LeClaire, BW, Lockyer, NS, Lüth, V, Ong, RA, Richter, B, Riles, K, Yelton, JM, Abrams, G, Amidei, D, Baden, AR, Boyer, J, Butler, F, Gidal, G, Gold, MS, Goldhaber, G, Golding, L, Haggerty, J, Herrup, D, Juricic, I, Kadyk, JA, Levi, ME, Nelson, ME, Rowson, PC, Schellman, H, Schmidke, WB, Sheldon, PD, Trilling, GH, Wood, DR, and Schaad, T
Subjects: Nuclear & Particles Physics, Astronomical and Space Sciences, Atomic, Molecular, Nuclear, Particle and Plasma Physics, Quantum Physics
Abstract: We have studied the muon decay channel of the lepton with the presence of a photon in e+e- annihilation data at Ec.m.=29 GeV from the Mark II detector. Included in this study is the first direct measurement of radiative decay. We find the ratio of the measured branching fraction to the expected value from QED to be 1.03±0.42. © 1990 The American Physical Society.
Published: 1990

22. Radiative τ production and decay

Author: Wu, DY, Hayes, K, Perl, ML, Barklow, T, Boyarski, A, Burchat, PR, Burke, DL, Dorfan, JM, Feldman, GJ, Gladney, L, Hanson, G, Hollebeek, RJ, Innes, WR, Jaros, JA, Karlen, D, Klein, SR, Lankford, AJ, Larsen, RR, LeClaire, BW, Lockyer, NS, Lüth, V, Ong, RA, Richter, B, Riles, K, Yelton, JM, Abrams, G, Amidei, D, Baden, AR, Boyer, J, Butler, F, Gidal, G, Gold, MS, Goldhaber, G, Golding, L, Haggerty, J, Herrup, D, Juricic, I, Kadyk, JA, Levi, ME, Nelson, ME, Rowson, PC, Schellman, H, Schmidke, WB, Sheldon, PD, Trilling, GH, Wood, DR, and Schaad, T
Subjects: Astronomical and Space Sciences, Atomic, Molecular, Nuclear, Particle and Plasma Physics, Quantum Physics, Nuclear & Particles Physics
Abstract: We have studied the muon decay channel of the lepton with the presence of a photon in e+e- annihilation data at Ec.m.=29 GeV from the Mark II detector. Included in this study is the first direct measurement of radiative decay. We find the ratio of the measured branching fraction to the expected value from QED to be 1.03±0.42. © 1990 The American Physical Society.
Published: 1990

23. Upper limits on D+/- and B+/- decays to two leptons plus pi +/- or K+/-

Author: Weir, AJ, Klein, SR, Abrams, G, Adolphsen, CE, Akerlof, C, Alexander, JP, Alvarez, M, Amidei, D, Baden, AR, Ballam, J, Barish, BC, Barklow, T, Barnett, BA, Bartelt, J, Blockus, D, Bonvicini, G, Boyarski, A, Boyer, J, Brabson, B, Breakstone, A, Brom, JM, Bulos, F, Burchat, PR, Burke, DL, Butler, F, Calvino, F, Cence, RJ, Chapman, J, Cords, D, Coupal, DP, DeStaebler, HC, Dorfan, DE, Dorfan, JM, Drell, PS, Feldman, GJ, Fernandez, E, Field, RC, Ford, WT, Fordham, C, Frey, R, Fujino, D, Gan, KK, Gidal, G, Gladney, L, Glanzman, T, Gold, MS, Goldhaber, G, Green, A, Grosse-Wiesmann, P, Haggerty, J, Hanson, G, Harr, R, Harris, FA, Hawkes, CM, Hayes, K, Herrup, D, Heusch, CA, Himel, T, Hollebeek, RJ, Hutchinson, D, Hylen, J, Innes, WR, Jaffre, M, and Jaros, JA
Subjects: Nuclear & Particles Physics, Astronomical and Space Sciences, Atomic, Molecular, Nuclear, Particle and Plasma Physics, Quantum Physics
Abstract: Data taken by the Mark II detector at the SLAC e+e- storage ring PEP was used to search for exclusive decays of D and B mesons into two charged leptons plus a charged pion or kaon. All possible charge and lepton combinations consistent with charge conservation were considered and no evidence for any signals was found. We obtain upper limits for the various branching ratios ranging from 2.5×10-3 to 9.2×10-3, at a 90% confidence level. Some of these limits can be used to constrain leptoquark masses in various models. © 1990 The American Physical Society.
Published: 1990

24. Upper limits on D± and B± decays to two leptons plus π± or K±

Author: Weir, AJ, Klein, SR, Abrams, G, Adolphsen, CE, Akerlof, C, Alexander, JP, Alvarez, M, Amidei, D, Baden, AR, Ballam, J, Barish, BC, Barklow, T, Barnett, BA, Bartelt, J, Blockus, D, Bonvicini, G, Boyarski, A, Boyer, J, Brabson, B, Breakstone, A, Brom, JM, Bulos, F, Burchat, PR, Burke, DL, Butler, F, Calvino, F, Cence, RJ, Chapman, J, Cords, D, Coupal, DP, DeStaebler, HC, Dorfan, DE, Dorfan, JM, Drell, PS, Feldman, GJ, Fernandez, E, Field, RC, Ford, WT, Fordham, C, Frey, R, Fujino, D, Gan, KK, Gidal, G, Gladney, L, Glanzman, T, Gold, MS, Goldhaber, G, Green, A, Grosse-Wiesmann, P, Haggerty, J, Hanson, G, Harr, R, Harris, FA, Hawkes, CM, Hayes, K, Herrup, D, Heusch, CA, Himel, T, Hollebeek, RJ, Hutchinson, D, Hylen, J, Innes, WR, Jaffre, M, Jaros, JA, Juricic, I, Kadyk, JA, Karlen, D, Kent, J, Koska, W, Kozanecki, W, Lankford, AJ, Larsen, RR, LeClaire, BW, Levi, ME, Litke, AM, Lockyer, NS, Lüth, V, Matthews, JAJ, Meyer, DI, Milliken, BD, Moffeit, KC, Müller, L, Nash, J, Nelson, ME, Nitz, D, Ogren, H, Ong, RA, O'Shaughnessy, KF, Parker, SI, Peck, C, Petersen, A, Petradza, M, Porter, FC, Rankin, P, Richter, B, Riles, K, Rowson, PC, Rust, DR, Sadrozinski, HFW, and Schaad, T
Subjects: Nuclear and Plasma Physics, Particle and High Energy Physics, Physical Sciences, Astronomical and Space Sciences, Atomic, Molecular, Nuclear, Particle and Plasma Physics, Quantum Physics, Nuclear & Particles Physics, Mathematical physics, Astronomical sciences, Particle and high energy physics
Abstract: Data taken by the Mark II detector at the SLAC e+e- storage ring PEP was used to search for exclusive decays of D and B mesons into two charged leptons plus a charged pion or kaon. All possible charge and lepton combinations consistent with charge conservation were considered and no evidence for any signals was found. We obtain upper limits for the various branching ratios ranging from 2.5×10-3 to 9.2×10-3, at a 90% confidence level. Some of these limits can be used to constrain leptoquark masses in various models. © 1990 The American Physical Society.
Published: 1990

25. Measurement of the tau lifetime

Author: Amidei, D, Trilling, GH, Abrams, GS, Baden, AR, Boyer, J, Butler, F, Gidal, G, Gold, MK, Goldhaber, G, Golding, L, Haggerty, J, Herrup, D, Juricic, I, Kadyk, JA, Nelson, ME, Rowson, PC, Schellman, H, Schmidke, WB, Sheldon, PD, de la Vaissiere, C, Wood, DR, Jaros, JA, Barklow, T, Boyarski, AM, Burchat, P, Burke, DL, Dorfan, JM, Feldman, GJ, Gladney, L, Hanson, G, Hayes, K, Hollebeek, RJ, Innes, WR, Karlen, D, Klein, SR, Lankford, AJ, Larsen, RR, LeClaire, BW, Levi, ME, Lockyer, NS, Lüth, V, Matteuzzi, C, Ong, RA, Perl, ML, Richter, B, Riles, K, Yelton, JM, and Schaad, T
Subjects: Astronomical and Space Sciences, Atomic, Molecular, Nuclear, Particle and Plasma Physics, Quantum Physics, Nuclear & Particles Physics
Abstract: We have used a high-resolution drift chamber in the Mark II detector at the SLAC storage ring PEP to measure the lifetime of leptons produced in e+e- annihilations at 29 GeV. Based on the flight-path distribution of 807 three-prong decays, the lifetime is found to be (2.880.16 0.17)×10-13 sec, in agreement with expectations for e - universality. © 1988 The American Physical Society.
Published: 1988

26. Limit on the decay D0→eμ∓

Author: Riles, K, Dorfan, JM, Abrams, GS, Amidei, D, Baden, AR, Barklow, T, Boyarski, AM, Boyer, J, Burchat, PR, Burke, DL, Butler, F, Feldman, GJ, Gidal, G, Gladney, L, Gold, MS, Goldhaber, G, Golding, LJ, Haggerty, J, Hanson, G, Hayes, K, Herrup, D, Himel, T, Hollebeek, RJ, Innes, WR, Jaros, JA, Juricic, I, Kadyk, JA, Karlen, D, Klein, SR, Lankford, AJ, Larsen, RR, LeClaire, BW, Levi, ME, Lockyer, NS, Lüth, V, Matteuzzi, C, Nelson, ME, Ong, RA, Perl, ML, Richter, B, Rowson, PC, Schaad, T, Schellman, H, Schmidke, WB, Sheldon, PD, Trilling, GH, de la Vaissiere, C, Wood, DR, and Yelton, JM
Subjects: Astronomical and Space Sciences, Atomic, Molecular, Nuclear, Particle and Plasma Physics, Quantum Physics, Nuclear & Particles Physics
Abstract: We have searched for the lepton-flavor-violating decay D0e in 204 pb-1 of e+e- annihilation data at Ec.m.=29 GeV from the Mark II detector. No candidates were found; we estimate an upper limit on the cross section times branching ratio of (e+e-D0,D0; inclusive)B(D0e)
Published: 1987

27. Search for B-decay to Higgs bosons for Higgs boson masses between 50 and 210 MeV/c2

Author: Snyder, A, Murray, WN, Abrams, G, Adolphsen, CE, Akerlof, C, Alexander, JP, Alvarez, M, Amidel, D, Baden, AR, Barish, BC, Barklow, T, Barnett, BA, Bartelt, J, Blockus, D, Bonvicini, G, Boyarski, A, Boyer, J, Brabson, B, Breakstone, A, Brom, JM, Bulos, F, Burchat, PR, Burke, DL, Butler, F, Calvino, F, Cence, RJ, Chapman, J, Cords, D, Coupal, DP, Destaebler, HC, Dorfan, DE, Dorfan, JM, Drell, PS, Feldman, GJ, Fernandez, E, Field, RC, Ford, WT, Fordham, C, Frey, R, Fujino, D, Gan, KK, Gidal, G, Gladney, L, Glanzman, T, Gold, MS, Goldhaber, G, Grosse-Wiesmann, P, Haggerty, J, Hanson, G, Harr, R, Harris, FA, Hawkes, CM, Hayes, K, Herrup, D, Heusch, CA, Himel, T, Hollebeek, RJ, Hutchinson, D, Hylen, J, Innes, WR, Jaffre, M, Jaros, JA, Juricic, I, Kadyk, JA, Karlen, D, Kent, J, Klein, SR, Koska, W, Kozanecki, W, Lankford, AJ, Larsen, RR, Leclaire, BW, Levi, ME, Litke, AM, Lockyer, NS, Lüth, V, Matthews, JAJ, Meyer, DI, Milliken, BD, Moffeit, KC, Müller, L, Nash, J, Nelson, ME, Nitz, D, Ogren, H, Ong, RA, O'Shaughnessy, KF, Parker, SI, Peck, C, Perl, ML, Petersen, A, Petradza, M, Porter, FC, Rankin, P, Richter, B, Riles, K, Rowson, PC, Rust, DR, Sadrozinski, HFW, and Schaad, T
Subjects: Mathematical Physics, Astronomical and Space Sciences, Atomic, Molecular, Nuclear, Particle and Plasma Physics, Nuclear & Particles Physics
Abstract: We use data from the Mark II experiment at PEP to search for the process B→h0X for mh0 between 50 and 210 MeV/c2. No evidence for the Higgs boson is seen in this mass range. The limit obtained rules out the standard Higgs boson for masses between 70 and 210 MeV/c2 and significantly constrains extensions of the Higgs sector. © 1989.
Published: 1989

28. The Mark II detector for the SLC

Author: Abrams, G, Adolphsen, CE, Akerlof, C, Alexander, JP, Alvarez, M, Averill, D, Baden, AR, Ballam, J, Barish, BC, Barklow, T, Barnett, BA, Bartelt, J, Blockus, D, De Boer, W, Bonvicini, G, Boswell, C, Boyarski, A, Boyer, J, Brabson, B, Braune, K, Breakstone, A, Brom, JM, Bulos, F, Burchat, PR, Burke, DL, Butler, F, Calvino, F, Cence, RJ, Chapman, J, Chmeissani, M, Cords, D, Coupal, DP, Dauncey, P, Destaebler, HC, Dorfan, DE, Dorfan, JM, Drell, PS, Drewer, DC, Fay, J, Feldman, GJ, Fernandes, D, Fernandez, E, Field, RC, Ford, WT, Fordham, C, Frey, R, Fujino, D, Gan, KK, Gatto, C, Gero, E, Gidal, G, Glanzman, T, Goldhaber, G, Cadenas, JJ Gomez, Gong, X, Gratta, G, Green, A, Grosse-Wiesmann, P, Haggerty, J, Hanson, G, Harr, R, Harral, B, Harris, FA, Hawkes, CM, Hayes, K, Hearty, C, Herrup, D, Heusch, CA, Himel, T, Hinshaw, DA, Hoenk, M, Holmgren, S-O, Hong, SJ, Hutchinson, D, Hylen, J, Innes, WR, Jacobsen, RG, Jaffre, M, Jaros, JA, Jung, CK, Juricic, I, Kadyk, JA, Karlen, D, Kent, J, King, M, Klein, SR, Koepke, L, Koetke, D, Koide, A, Komamiya, S, Koska, W, Kowalski, LA, Kozanecki, W, Kral, JF, Kuhlen, M, Labarga, L, Lankford, AJ, Larsen, RR, Levi, ME, and Li, Z
Subjects: Astronomical and Space Sciences, Atomic, Molecular, Nuclear, Particle and Plasma Physics, Other Physical Sciences, Nuclear & Particles Physics
Abstract: The Mark II detector has been upgraded in preparation for its role as the first detector to take data at the Stanford Linear Collider. The new detector components include the central drift chamber, the time-of-flight system, the coil, the endcap electromagnetic calorimeters and the beam energy and luminosity measuring devices. There have also been improvements in detector hermeticity. All of the major components were installed for a test run at the PEP storage ring (√s = 29 GeV) in 1985. This paper describes the upgraded detector, including its trigger and data acquisition systems, and gives performance figures for its components. Future improvements are also discussed. © 1989.
Published: 1989

29. Bose-Einstein correlations in e+e- collisions.

Author: Juricic, I, Goldhaber, G, Gidal, G, Abrams, G, Amidei, D, Baden, AR, Boyer, J, Butler, F, Carithers, WC, Gold, MS, Golding, L, Haggerty, J, Herrup, D, Kadyk, JA, Levi, ME, Nelson, ME, Rowson, PC, Schellman, H, Schmidke, WB, Sheldon, PD, Trilling, GH, Wood, DR, Barklow, T, Boyarski, A, Breidenbach, M, Burchat, P, Burke, DL, Cords, D, Dorfan, JM, Feldman, GJ, Gladney, L, Hanson, G, Hayes, K, Hitlin, DG, Hollebeek, RJ, Innes, WR, Jaros, JA, Karlen, D, Klein, SR, Lankford, AJ, Larsen, RR, LeClaire, BW, Lockyer, NS, Lüth, V, Ong, RA, Perl, ML, Richter, B, Riles, K, Ross, MC, Schindler, RH, Yelton, JM, Schaad, T, and Schwitters, RF
Subjects: Nuclear & Particles Physics, Astronomical and Space Sciences, Atomic, Molecular, Nuclear, Particle and Plasma Physics, Quantum Physics, Atomic, Molecular, Nuclear, Particle and Plasma Physics
Abstract: Four data sets collected with the Mark II detector during its operation at the SPEAR and PEP e+e- storage rings at SLAC are used to study the Bose-Einstein correlation between pairs and triplets of like-sign charged pions. The data sets represent four different regions of energy available for hadron production: the J at s =3.095 GeV, typical hadronic energy of 5 GeV in two-photon events, and annihilation in the energy regions s =47 GeV above the J, and s =29 GeV. The Bose-Einstein correlation is studied as a function of Q2, the four-momentum difference squared of the pair, and of Q32, an analogous quantity defined for triplets. After corrections for Coulomb effects and pion misidentification, pair analyses indicate a nearly full Bose-Einstein enhancement (1) in the J and the two-photon data, and about half the maximum value in the two higher-energy data sets. The pair analysis parameter r lies within a band of ±0.1 fm around 0.7 fm and is essentially the same for all four data sets. Pion triplet analyses give consistent results for the triplet parameters 3 and r3. In an attempt to investigate the shape of the pion source, we also study the Bose-Einstein correlation in pion pairs using two-dimensional distributions in components of Q2. © 1989 The American Physical Society.
Published: 1989

30. Multihadronic events at Ec.m.=29 GeV and predictions of QCD models from Ec.m.=29 GeV to Ec.m.=93 GeV

Author: Petersen, A, Abrams, G, Adolphsen, CE, Akerlof, C, Alexander, JP, Alvarez, M, Amidei, D, Baden, AR, Ballam, J, Barish, BC, Barklow, T, Barnett, BA, Bartelt, J, Blockus, D, Bonvicini, G, Boyarski, A, Boyer, J, Brabson, B, Breakstone, A, Brom, JM, Bulos, F, Burchat, PR, Burke, DL, Butler, F, Calvino, F, Cence, RJ, Chapman, J, Cords, D, Coupal, DP, DeStaebler, HC, Dorfan, DE, Dorfan, JM, Drell, PS, Feldman, GJ, Fernandez, E, Field, RC, Ford, WT, Fordham, C, Frey, R, Fujino, D, Gan, KK, Gidal, G, Gladney, L, Glanzman, T, Gold, MS, Goldhaber, G, Golding, L, Green, A, Grosse-Wiesmann, P, Haggerty, J, Hanson, G, Harr, R, Harris, FA, Hawkes, CM, Hayes, K, Herrup, D, Heusch, CA, Himel, T, Hoenk, M, Hollebeek, RJ, Hutchinson, D, Hylen, J, Innes, WR, Jaffre, M, Jaros, JA, Juricic, I, Kadyk, JA, Karlen, D, Kent, J, Klein, SR, Koide, A, Koska, W, Kozanecki, W, Lankford, AJ, Larsen, RR, LeClaire, BW, Levi, ME, Li, Z, Litke, AM, Lockyer, NS, Matteuzzi, C, Matthews, JAJ, Meyer, DI, Milliken, BD, Moffeit, KC, Müller, L, Nash, J, Nelson, ME, Nitz, D, Ogren, H, Ong, RA, O’Shaughnessy, KF, Parker, SI, Peck, C, Perl, ML, Petradza, M, Porter, FC, Rankin, P, Richter, B, and Riles, K
Subjects: Astronomical and Space Sciences, Atomic, Molecular, Nuclear, Particle and Plasma Physics, Quantum Physics, Nuclear & Particles Physics
Abstract: Multihadronic e+e- annihilation events at a center-of-mass energy of 29 GeV have been studied with both the original (PEP 5) Mark II and the upgraded Mark II detectors. Detector-corrected distributions from global shape analyses such as aplanarity, Q2-Q1, sphericity, thrust, minor value, oblateness, and jet masses, and inclusive charged-particle distributions including x, rapidity, p, and particle flow are presented. These distributions are compared with predictions from various multihadron event models which use leading-logarithmic shower evolution or QCD matrix elements at the parton level and string or cluster fragmentation for hadronization. The new generation of parton-shower models gives, on the average, a better description of the data than the previous parton-shower models. The energy behavior of these models is compared to existing e+e- data. The predictions of the models at a center-of-mass energy of 93 GeV, roughly the expected mass of the Z0, are also presented. © 1988 The American Physical Society.
Published: 1988

31. Determination of αs from energy-energy correlations in e+e- annihilation at 29 GeV

Author: Wood, DR, Petersen, A, Abrams, G, Adolphsen, CE, Akerlof, C, Alexander, JP, Alvarez, M, Amidei, D, Baden, AR, Ballam, J, Barish, BC, Barklow, T, Barnett, BA, Bartelt, J, Blockus, D, Bonvicini, G, Boyarski, A, Boyer, J, Brabson, B, Breakstone, A, Brom, JM, Bulos, F, Burchat, PR, Burke, DL, Butler, F, Calvino, F, Cence, RJ, Chapman, J, Cords, D, Coupal, DP, DeStaebler, HC, Dorfan, DE, Dorfan, JM, Drell, PS, Feldman, GJ, Fernandez, E, Field, RC, Ford, WT, Fordham, C, Frey, R, Fujino, D, Gan, KK, Gidal, G, Gladney, L, Glanzman, T, Gold, MS, Goldhaber, G, Golding, L, Green, A, Grosse-Wiesmann, P, Haggerty, J, Hanson, G, Harr, R, Harris, FA, Hawkes, CM, Hayes, K, Herrup, D, Heusch, CA, Himel, T, Hoenk, M, Hollebeek, RJ, Hutchinson, D, Hylen, J, Innes, WR, Jaffre, M, Jaros, JA, Juricic, I, Kadyk, JA, Karlen, D, Kent, J, Klein, SR, Koide, A, Koska, W, Kozanecki, W, Lankford, AJ, Larsen, RR, LeClaire, BW, Levi, ME, Li, Z, Litke, AM, Lockyer, NS, Lüth, V, Matteuzzi, C, Matthews, JAJ, Meyer, DI, Milliken, BD, Moffeit, KC, Müller, L, Nash, J, Nelson, ME, Nitz, D, Ogren, H, Ong, RA, O’Shaughnessy, KF, Parker, SI, Peck, C, Perl, ML, Petradza, M, Porter, FC, and Rankin, P
Subjects: Nuclear and Plasma Physics, Particle and High Energy Physics, Physical Sciences, Affordable and Clean Energy, Astronomical and Space Sciences, Atomic, Molecular, Nuclear, Particle and Plasma Physics, Quantum Physics, Nuclear & Particles Physics, Mathematical physics, Astronomical sciences, Particle and high energy physics
Abstract: We have studied the energy-energy correlation in e+e- annihilation into hadrons at s =29 GeV using the Mark II detector at the SLAC storage ring PEP. We find to O(s2) that s=0.1580.0030.008 if hadronization is described by string fragmentation. Independent fragmentation schemes give s=0.100.14, and give poor agreement with the data. A leading-log shower fragmentation model is found to describe the data well. © 1988 The American Physical Society.
Published: 1988

32. Measurement of single and double radiative low-Q2 Bhabha scattering at Ec.m.

Author: Karlen, D, Abrams, G, Amidei, D, Baden, AR, Barklow, T, Boyarski, AM, Boyer, J, Burchat, PR, Burke, DL, Butler, F, Dorfan, JM, Feldman, GJ, Gidal, G, Gladney, L, Gold, MS, Goldhaber, G, Golding, L, Haggerty, J, Hanson, G, Hayes, K, Herrup, D, Hollebeek, RJ, Innes, WR, Jaros, JA, Juricic, I, Kadyk, JA, Klein, SR, Lankford, AJ, Larsen, RR, LeClaire, BW, Levi, M, Lockyer, NS, Lüth, V, Nelson, ME, Ong, RA, Perl, ML, Richter, B, Riles, K, Rowson, PC, Schaad, T, Schellman, H, Schmidke, WB, Sheldon, PD, Trilling, GH, Wood, DR, and Yelton, JM
Subjects: Nuclear & Particles Physics, Astronomical and Space Sciences, Atomic, Molecular, Nuclear, Particle and Plasma Physics, Quantum Physics
Abstract: The process e+e-e+e-(), where one electron scatters at a small angle, is studied with data from the Mark II detector at the SLAC storage ring PEP. The data are in excellent agreement with a Monte Carlo calculation and include a large contribution from order 4. The ratio of measured to calculated cross sections is R=0.9930.0170.015, where the first error is statistical and the second systematic. This is a sensitive test of the calculation of the dominant background for neutrino-counting experiments. © 1989 The American Physical Society.
Published: 1989

33. Limits on new-lepton pairs (L-,L0) with arbitrary neutrino mass.

Author: Stoker, DP, Perl, ML, Abrams, G, Baden, AR, Barklow, T, Barnett, BA, Boyarski, AM, Boyer, J, Burchat, PR, Butler, F, Dorfan, JM, Feldman, GJ, Gidal, G, Hanson, G, Harral, BD, Hayes, K, Herrup, D, Hylen, JE, Innes, WR, Jaros, JA, Kadyk, JA, Karlen, D, Klein, SR, Lankford, AJ, LeClaire, BW, Levi, M, Lüth, V, Matthews, JA, Ong, RA, Riles, K, Rowson, PC, and Wood, DR
Subjects: Nuclear & Particles Physics, Astronomical and Space Sciences, Atomic, Molecular, Nuclear, Particle and Plasma Physics, Quantum Physics
Abstract: We have searched 205 pb-1 of s =29 GeV data from the Mark II detector at the SLAC e+e- storage ring PEP for events which may signify the existence of a new lepton pair (L-,L0) where the L0 may be massive, but does not exceed the L- mass. Three event signatures for L+L- decay are examined: (i) e, (ii) (e or)(+4), and (iii) (e or )(3+0). The numbers of signature events are found to be in good agreement with Monte Carlo simulations of known background sources. The ranges of L- and L0 masses for which new lepton pairs are excluded are obtained using a likelihood-ratio method to compare the number of observed signature events to the expected background, and to the expected background plus Monte Carlo predictions of (L-,L0) signals. © 1989 The American Physical Society.
Published: 1989

34. Upper limit on B0B0 mixing in e+e- annihilation at 29 GeV

Author: Schaad, T, Nelson, ME, Abrams, G, Amidei, D, Baden, AR, Barklow, T, Boyarski, AM, Boyer, J, Breidenbach, M, Burchat, PR, Burke, DL, Butler, F, Dorfan, JM, Feldman, GJ, Gidal, G, Gladney, L, Gold, MS, Goldhaber, G, Golding, L, Haggerty, J, Hanson, G, Hayes, K, Herrup, D, Hollebeek, RJ, Innes, WR, Jaros, JA, Juricic, I, Kadyk, JA, Karlen, D, Klein, SR, Lankford, AJ, Larsen, RR, Leclaire, BW, Levi, M, Lockyer, NS, Lüth, V, Matteuzi, C, Ong, RA, Perl, ML, Richter, B, Riles, K, Ross, MC, Rowson, PC, Schellman, H, Schmidke, WB, Schwitters, R, Sheldon, PD, trilling, GH, De La Vaissiere, C, Wood, DR, Yelton, JM, and Zaiser, C
Subjects: Nuclear & Particles Physics, Mathematical Physics, Astronomical and Space Sciences, Atomic, Molecular, Nuclear, Particle and Plasma Physics
Published: 1985

35. Upper limit on the branching ratio for the decay τ-→Π-ηvτ

Author: Gan, KK, Abrams, GS, Amidei, D, Baden, AR, Barklow, T, Boyarski, AM, Boyer, J, Burchat, PR, Burke, DL, Butler, F, Dorfan, JM, Feldman, GJ, Gidal, G, Gladney, L, Gold, MS, Goldhaber, G, Golding, L, Haggerty, J, Hanson, G, Hayes, K, Herrup, D, Hollebeek, RJ, Innes, WR, Jaros, JA, Juricic, I, Kadyk, JA, Karlen, D, Klein, SR, Lankford, AJ, Larsen, RR, Leclaire, BW, Levi, ME, Lockyer, NS, Lüth, V, Matteuzzi, C, Nelson, ME, Ong, RA, Perl, ML, Richter, B, Riles, K, Rowson, PC, Schaad, T, Schellman, H, Schmidke, WB, Sheldon, PD, Trilling, GH, de la Vaissiere, C, Wood, DR, and Yelton, JM
Subjects: Mathematical Physics, Astronomical and Space Sciences, Atomic, Molecular, Nuclear, Particle and Plasma Physics, Nuclear & Particles Physics
Abstract: We have searched for the decay τ-→Π-ηvτ using the MARK II detector at the PEP e+e- storage ring. No evidence for the decay is found; the upper limit for the branching ratio is B(τ-→Π-ηvτ)
Published: 1987

36. Observation of ψ production in e+e- annihilation at 29 GeV

Author: Wormser, G, Ong, RA, Abrams, G, Amidei, D, Baden, AR, Barklow, T, Boyarski, AM, Boyer, J, Burchat, PR, Burke, DL, Butler, F, Dorfan, JM, Feldman, GJ, Gidal, G, Gladney, L, Gold, MS, Goldhaber, G, Golding, L, Haggerty, J, Hanson, G, Hayes, K, Herrup, D, Hollebeek, RJ, Innes, WR, Jaros, JA, Juricic, I, Kadyk, JA, Karlen, D, Klein, SR, Lankford, AJ, Larsen, RR, LeClaire, BW, Levi, M, Lockyer, NS, Lüth, V, Matteuzzi, C, Nelson, ME, Richter, B, Riles, K, Rowson, PC, Schaad, T, Schellman, H, Schmidke, WB, Sheldon, PD, Trilling, GH, de la Vaissiere, C, Wood, DR, and Yelton, JM
Subjects: Astronomical and Space Sciences, Atomic, Molecular, Nuclear, Particle and Plasma Physics, Quantum Physics, Nuclear & Particles Physics
Abstract: Inclusive production in e+e- annihilation at 29 GeV has been measured with the Mark II detector. The cross section is found to be 1.10.50.4 pb. After subtraction of the expected contribution from B decay, an upper limit of 0.02 is obtained for other sources of production. © 1988 The American Physical Society.
Published: 1988

37. Observation of psi production in e+e- annihilation at 29 GeV.

Author: Wormser, G, Ong, RA, Abrams, G, Amidei, D, Baden, AR, Barklow, T, Boyarski, AM, Boyer, J, Burchat, PR, Burke, DL, Butler, F, Dorfan, JM, Feldman, GJ, Gidal, G, Gladney, L, Gold, MS, Goldhaber, G, Golding, L, Haggerty, J, Hanson, G, Hayes, K, Herrup, D, Hollebeek, RJ, Innes, WR, Jaros, JA, Juricic, I, Kadyk, JA, Karlen, D, Klein, SR, Lankford, AJ, Larsen, RR, LeClaire, BW, Levi, M, Lockyer, NS, Lüth, V, Matteuzzi, C, Nelson, ME, Richter, B, Riles, K, Rowson, PC, Schaad, T, Schellman, H, Schmidke, WB, Sheldon, PD, Trilling, GH, de la Vaissiere C, Wood, DR, and Yelton, JM
Subjects: Nuclear & Particles Physics, Astronomical and Space Sciences, Atomic, Molecular, Nuclear, Particle and Plasma Physics, Quantum Physics
Abstract: Inclusive production in e+e- annihilation at 29 GeV has been measured with the Mark II detector. The cross section is found to be 1.10.50.4 pb. After subtraction of the expected contribution from B decay, an upper limit of 0.02 is obtained for other sources of production. © 1988 The American Physical Society.
Published: 1988

38. Search for Multimessenger Sources of Gravitational Waves and High-energy Neutrinos with Advanced LIGO during Its First Observing Run, ANTARES, and IceCube

Author: Albert, A, Andre, M, Anghinolfi, M, Ardid, M, Aubert, J-J and Aublin, J, Avgitas, T, Baret, B, Barrios-Marti, J, Basa, S, Belhorma, B, Bertin, V and Biagi, S, Bormuth, R, Boumaaza, J, Bourret, S, Bouwhuis, M. C, Branzas, H, Bruijn, R, Brunner, J, Busto, J, Capone, A, Caramete, L, Carr, J, Celli, S, Chabab, M, Moursli, El, Cherkaoui and Chiarusi, R., T, Circella, M, Coelho, J. A. B, Coleiro, A, Colomer, M, Coniglione, R, Costantini, H, Coyle, P, Creusot, A, Diaz, A. F, Deschamps, A, Distefano, C, Palma, Di, I and Domi, A, Dona, R, Donzaud, C, Dornic, D, Drouhin, D, Eberl, T, Bojaddaini, El, I and El Khayati, N, Elsaesser, D, Enzenhoefer, A, Ettahiri, A, Fassi, F, Felis, I and Fermani, P, Ferrara, G, Fusco, L, Gay, P, Glotin, H, Gregoire, T, Ruiz, Gracia and Graf, R., K, Hallmann, S, van Haren, H, Heijboer, A. J, Hello, Y, Hernandez-Rey, J. J, Hoessl, J, Hofestaedt, J, Illuminati, G, de Jong, M, Jongen, M, Kadler, M, Kalekin, O, Katz, U, Khan-Chowdhury, N. R, Kouchner, A, Kreter, M, Kreykenbohm, I and Kulikovskiy, V and Lachaud, C, Lahmann, R, Lefevre, D, Leonora, E, Levi, G, Lotze, M, Loucatos, S, Maggi, G, Marcelin, M, Margiotta, A, Marinelli, A, Martinez-Mora, J. A, Mele, R, Melis, K, Migliozzi, P, Moussa, A, Navas, S, Nezri, E, Nunez, A, Organokov, M, Pavalas, G. E, Pellegrino, C, Piattelli, P, Popa, V and Pradier, Quinn, L, Racca, C, Randazzo, N, Riccobene, G, Sanchez-Losa, A, Saldana, M, Salvadori, I and Samtleben, D. F. E., Sanguineti, M, Sapienza, P, Schussler, F, Spurio, M, Stolarczyk, Th and Taiuti, M, Tayalati, Y, Trovato, A, Vallage, B, Van Elewyck, V, Versari, F, Vivolo, D, Wilms, J, Zaborov, D, Zornoza, J. D, Zuniga, J, Aartsen, M. G, Ackermann, M, Adams, J, Aguilar, J. A, Ahlers, M, Ahrens, M, Altmann, D, Andeen, K, Anderson, T, Ansseau, I and Anton, G, Arguelles, C, Auffenberg, J, Axani, S, Backes, P, Bagherpour, H, Bai, X, Barbano, A, Barron, J. P, Barwick, S. W, Baum, V and Bay, R, Beatty, J. J, Tjus, Becker and Becker, J., K-H and BenZvi, Berley, D, Bernardini, E, Besson, D. Z, Binder, G, Bindig, D, Blaufuss, E, Blot, S, Bohm, C, Boerner, M, Bos, F, Boeser, S, Botner, O, Bourbeau, E, Bourbeau, J, Bradascio, F, Braun, J, Brenzke, M, Bretz, H-P and Bron, Brostean-Kaiser, J, Burgman, A, Busse, R. S, Carver, T, Cheung, E, Chirkin, D, Clark, K, Classen, L, Collin, G. H, Conrad, J. M, Coppin, P, Correa, P, Cowen, D. F, Cross, R, Dave, P, Day, M, de Andre, J. P. A. M, De Clercq, C, Delaunay, J. J, Dembinski, H, Deoskar, K, De Ridder, S, Desiati, P, de Vries, K. D, de Wasseige, G, de With, M, Deyoung, T, Diaz-Velez, J. C, Lorenzo, Di, V and Dujmovic, H, Dumm, J. P, Dunkman, M, Dvorak, E, Eberhardt, B, Ehrhardt, T, Eichmann, B, Eller, P, Evenson, P. A, Fahey, S, Fazely, A. R, Felde, J, Filimonov, K, Finley, C, Franckowiak, A, Friedman, E, Fritz, A, Gaisser, T. K, Gallagher, J, Ganster, E, Garrappa, S, Gerhardt, L, Ghorbani, K, Giang, W, Glauch, T, Gluesenkamp, T, Goldschmidt, A, Gonzalez, J. G, Grant, D, Griffith, Z, Haack, C, Hallgren, A, Halve, L, Halzen, F, Hanson, K, Hebecker, D, Heereman, D, Helbing, K, Hellauer, R, Hickford, S, Hignight, J, Hill, G. C, Hoffman, K. D, Hoffmann, R, Hoinka, T, Hokanson-Fasig, B, Hoshina, K, Huang, F, Huber, M, Hultqvist, K, Huennefeld, M, Hussain, R, In, S, Iovine, N, Ishihara, A, Jacobi, E, Japaridze, G. S, Jeong, M, Jero, K, Jones, B. J. P, Kalaczynski, P, Kang, W, Kappes, A, Kappesser, D, Karg, T, Karle, A, Kauer, M, Keivani, A, Kelley, J. L, Kheirandish, A, Kim, J, Kintscher, T, Kiryluk, J, Kittler, T, Klein, S. R, Koirala, R, Kolanoski, H, Koepke, L, Kopper, C, Kopper, S, Koschinsky, J. P, Koskinen, D. J, Kowalski, M, Krings, K, Kroll, M, Krueckl, G, Kunwar, S, Kurahashi, N, Kyriacou, A, Labare, M, Lanfranchi, J. L, Larson, M. J, Lauber, F, Leonard, K, Leuermann, M, Liu, Q. R, Lohfink, E, Mariscal, Lozano and Lu, C. J., L, Lunemann, J, Luszczak, W, Madsen, J, Mahn, K. B. M, Makino, Y, Mancina, S, Maris, I. C, Maruyama, R, Mase, K, Maunu, R, Meagher, K, Medici, M, Meier, M, Menne, T, Merino, G, Meures, T, Miarecki, S, Micallef, J, Momente, G, Montaruli, T, Moore, R. W, Moulai, M, Nagai, R, Nahnhauer, R, Nakarmi, P, Naumann, U, Neer, G, Niederhausen, H, Nowicki, S. C, Nygren, D. R, Pollmann, Obertacke and Olivas, A., O'Murchadha, A, O'Sullivan, E, Palczewski, T, Pandya, H, Pankova, V, D, Peiffer, P, Pepper, J. A, de los Heros, Perez and Pieloth, C., Pinat, E, Pizzuto, A, Plum, M, Price, P. B, Przybylski, G. T, Raab, C, Rameez, M, Rauch, L, Rawlins, K, Rea, I. C, Reimann, R, Relethford, B, Renzi, G, Resconi, E, Rhode, W, Richman, M, Robertson, S, Rongen, M, Rott, C, Ruhe, T, Ryckbosch, D, Rysewyk, D, Safa, I and Herrera, Sanchez and Sandrock, S. E., Sandroos, J, Santander, M, Sarkar, S, Satalecka, K, Schaufel, M, Schlunder, P, Schmidt, T, Schneider, A, Schneider, J, Schoeneberg, S, Schumacher, L, Sclafani, S, Seckel, D, Seunarine, S, Soedingrekso, J, Soldin, D, Song, M, Spiczak, G. M, Spiering, C, Stachurska, J, Stamatikos, M, Stanev, T, Stasik, A, Stein, R, Stettner, J, Steuer, A, Stezelberger, T, Stokstad, R. G, Stossl, A, Strotjohann, N. L, Stuttard, T, Sullivan, G. W, Sutherland, M, Taboada, I and Tenholt, F, Ter-Antonyan, S, Terliuk, A, Tilav, S, Toale, P. A, Tobin, M. N, Tonnis, C, Toscano, S, Tosi, D, Tselengidou, M, Tung, C. F, Turcati, A, Turcotte, R, Turley, C. F, Ty, B, Unger, E, Elorrieta, Unland and Usner, M. A., Vandenbroucke, J, Van Driessche, W, van Eijk, D, van Eijndhoven, N, Vanheule, S, van Santen, J, Vraeghe, M, Walck, C, Wallace, A, Wallraff, M, Wandler, F. D, Wandkowsky, N, Watson, T. B, Waza, A, Weaver, C, Weiss, M. J, Wendt, C, Werthebach, J, Westerhoff, S, Whelan, B. J, Whitehorn, N, Wiebe, K, Wiebusch, C. H, Wille, L, Williams, D. R, Wills, L, Wolf, M, Wood, J, Wood, T. R, Woolsey, E, Woschnagg, K, Wrede, G, D. L, Xu, X. W, Xu, Xu, Y, Yanez, J. P, Yodh, G, Yoshida, S, Yuan, T, Abbott, B. P, Abbott, R, Abbott, T. D, Abraham, S, Acernese, F, Ackley, K, Adams, C, Adya, V. B, Affeldt, C, Agathos, M, Agatsuma, K, Aggarwal, N, Aguiar, O. D, Aiello, L, Ain, A, Ajith, P, Allen, G, Allocca, A, Aloy, M. A, Altin, P. A, Amato, A, Ananyeva, A, Anderson, S. B, Anderson, W. G, Angelova, Antier, S, Appert, S, Arai, K, Araya, M. C, Areeda, J. S, Arene, M, Arnaud, N, Arun, K. G, Ascenzi, S, Ashton, G, Aston, S. M, Astone, P, Aubin, F, Aufmuth, P, Aultoneal, K, Austin, C, Avendano, V and Avila-Alvarez, Babak, S, Bacon, P, Badaracco, F, Bader, M. K. M, Bae, S, Baker, P. T, Baldaccini, F, Ballardin, G, Ballmer, S. W, Banagiri, S, Barayoga, J. C, Barclay, S. E, Barish, B. C, Barker, D, Barkett, K, Barnum, S, Barone, F, Barr, B, Barsotti, L, Barsuglia, M, Barta, D, Bartlett, J, Bartos, I and Bassiri, Basti, A, Bawaj, M, Bayley, J. C, Bazzan, M, Becsy, B, Bejger, M, Belahcene, I and Bell, A. S., Beniwal, D, Berger, B. K, Bergmann, G, Bernuzzi, S, Bero, J. J, Berry, C. P. L, Bersanetti, D, Bertolini, A, Betzwieser, J, Bhandare, R, Bidler, J, Bilenko, I. A, Bilgili, S. A, Billingsley, G, Birch, J, Birney, R, Birnholtz, O, Biscans, S, Biscoveanu, S, Bisht, A, Bitossi, M, Bizouard, M. A, Blackburn, J. K, Blair, C. D, Blair, D. G, Blair, R. M, Bloemen, S, Bode, N, Boer, M, Boetzel, Y, Bogaert, G, Bondu, F, Bonilla, E, Bonnand, R, Booker, P, Boom, B. A, Booth, C. D, Bork, R, Boschi, V and Bose, Bossie, K, Bossilkov, V and Bosveld, Bouffanais, Y, Bozzi, A, Bradaschia, C, Brady, P. R, Bramley, A, Branchesi, M, Brau, J. E, Briant, T, Briggs, J. H, Brighenti, F, Brillet, A, Brinkmann, M, Brisson, V and Brockill, Brooks, A. F, Brown, D. D, Brunett, S, Buikema, A, Bulik, T, Bulten, H. J, Buonanno, A, Buskulic, D, Buy, C, Byer, R. L, Cabero, M, Cadonati, L, Cagnoli, G, Cahillane, C, Bustillo, Calderon and Callister, J., T. A., Calloni, E, Camp, J. B, Campbell, W. A, Cannon, K. C, Cao, H, Cao, J, Capocasa, E, Carbognani, F, Caride, S, Carney, M. F, Carullo, G, Diaz, Casanueva and Casentini, J., Caudill, S, Cavaglia, M, Cavalier, F, Cavalieri, R, Cella, G, Cerda-Duran, P, Cerretani, G, Cesarini, E, Chaibi, O, Chakravarti, K, Chamberlin, S. J, Chan, M, Chao, S, Charlton, P, Chase, E. A, Chassande-Mottin, E, Chatterjee, D, Chaturvedi, M, Cheeseboro, B. D, Chen, H. Y, Chen, X, Chen, Y, Cheng, H-P and Cheong, C. K., Chia, H. Y, Chincarini, A, Chiummo, A, Cho, G, Cho, H. S, Cho, M, Christensen, N, Chu, Q, Chua, S, Chung, K. W, Chung, S, Ciani, G, Ciobanu, A. A, Ciolfi, R, Cipriano, F, Cirone, A, Clara, F, Clark, J. A, Clearwater, P, Cleva, F, Cocchieri, C, Coccia, E, Cohadon, P-F and Cohen, Colgan, R, Colleoni, M, Collette, C. G, Collins, C, Cominsky, L. R, Constancio Jr, M, Conti, L, Cooper, S. J, Corban, P, Corbitt, T. R, Cordero-Carrion, I and Corley, K. R., Cornish, N, Corsi, A, Cortese, S, Costa, C. A, Cotesta, R, Coughlin, M. W, Coughlin, S. B, Coulon, J-P and Countryman, S. T., Couvares, P, Covas, P. B, Cowan, E. E, Coward, D. M, Cowart, M. J, Coyne, D. C, Coyne, R, Creighton, J. D. E, Creighton, T. D, Cripe, J, Croquette, M, Crowder, S. G, Cullen, T. J, Cumming, A, Cunningham, L, Cuoco, E, Dal Canton, T, Dalya, G, Danilishin, S. L, D'Antonio, S, Danzmann, K, Dasgupta, A, Costa, Da Silva and Datrier, C. F., L. E. H., Dattilo, V and Dave, I and Davier, Davis, D, Daw, E. J, Debra, D, Deenadayalan, M, Degallaix, J, De Laurentis, M, Deleglise, S, Del Pozzo, W, Demarchi, L. M, Demos, N, Dent, T, Denys, M, De Pietri, R, Derby, J, De Rosa, R, De Rossi, C, Desalvo, R, de Varona, O, Dhurandhar, S, Diaz, M. C, Dietrich, T, Di Fiore, L, Di Giovanni, M, Di Girolamo, T, Di Lieto, A, Ding, B, Di Pace, S, Di Renzo, F, Dmitriev, A, Doctor, Z, Donovan, F, Dooley, K. L, Doravari, S, Dorrington, I and Downes, T. P., Drago, M, Driggers, J. C, Du, Z, Ducoin, J-G and Dupej, Dwyer, S. E, Easter, P. J, Edo, T. B, Edwards, M. C, Effler, A, Ehrens, P, Eichholz, J, Eikenberry, S. S, Eisenmann, M, Eisenstein, R. A, Essick, R. C, Estelles, H, Estevez, D, Etienne, Z. B, Etzel, T, Evans, M, Evans, T. M, Fafone, V and Fair, Fairhurst, S, Fan, X, Farinon, S, Farr, B, Farr, W. M, Fauchon-Jones, E. J, Favata, M, Fays, M, Fazio, M, Fee, C, Feicht, J, Fejer, M. M, Feng, F, Fernandez-Galiana, A, Ferrante, I and Ferreira, E. C., Ferreira, T. A, Ferrini, F, Fidecaro, F, Fiori, I and Fiorucci, Fishbach, M, Fisher, R. P, Fishner, J. M, Fitz-Axen, M, Flaminio, R, Fletcher, M, Flynn, E, Fong, H, Font, J. A, Forsyth, P. W. F, Fournier, J-D and Frasca, Frasconi, F, Frei, Z, Freise, A, Frey, R, Frey, V and Fritschel, Frolov, V. V, Fulda, P, Fyffe, M, Gabbard, H. A, Gadre, B. U, Gaebel, S. M, Gair, J. R, Gammaitoni, L, Ganija, M. R, Gaonkar, S. G, Garcia, A, Garcia-Quiros, C, Garufi, F, Gateley, B, Gaudio, S, Gaur, G, Gayathri, V and Gemme, Genin, E, Gennai, A, George, D, George, J, Gergely, L, Germain, V and Ghonge, Ghosh, Abhirup and Ghosh, Archisman and Ghosh, Giacomazzo, B, Giaime, J. A, Giardina, K. D, Giazotto, A, Gill, K, Giordano, G, Glover, L, Godwin, P, Goetz, E, Goetz, R, Goncharov, B, Gonzalez, G, Castro, Gonzalez and Gopakumar, J. M., Gorodetsky, M. L, Gossan, S. E, Gosselin, M, Gouaty, R, Grado, A, Graef, C, Granata, M, Grant, A, Gras, S, Grassia, P, Gray, C, Gray, R, Greco, G, Green, A. C, Green, R, Gretarsson, E. M, Groot, P, Grote, H, Grunewald, S, Gruning, P, Guidi, G. M, Gulati, H. K, Guo, Y, Gupta, A, Gupta, M. K, Gustafson, E. K, Gustafson, R, Haegel, L, Halim, O, Hall, B. R, Hall, E. D, Hamilton, E. Z, Hammond, G, Haney, M, Hanke, M. M, Hanks, J, Hanna, C, Hannuksela, O. A, Hanson, J, Hardwick, T, Haris, K, Harms, J, Harry, G. M, Harry, I. W, Haster, C-J and Haughian, Hayes, F. J, Healy, J, Heidmann, A, Heintze, M. C, Heitmann, H, Hello, P, Hemming, G, Hendry, M, Heng, I. S, Hennig, J, Heptonstall, A. W, Hernandez, F. J, Heurs, M, Hild, S, Hinderer, T, Hoak, D, Hochheim, S, Hofman, D, Holgado, A. M, Holland, N. A, Holt, K, Holz, D. E, Hopkins, P, Horst, C, Hough, J, Howell, E. J, Hoy, C. G, Hreibi, A, Huerta, E. A, Huet, D, Hughey, B, Hulko, M, Husa, S, Huttner, S. H, Huynh-Dinh, T, Idzkowski, B, Iess, A, Ingram, C, Inta, R, Intini, G, Irwin, B, Isa, H. N, Isac, J-M and Isi, Iyer, B. R, Izumi, K, Jacqmin, T, Jadhav, S. J, Jani, K, Janthalur, N. N, Jaranowski, P, Jenkins, A. C, Jiang, J, Johnson, D. S, Jones, A. W, Jones, I, Jones, R, Jonker, R. J. G, Ju, L, Junker, J, Kalaghatgi, Kalogera, V and Kamai, B, Kandhasamy, S, Kang, G, Kanner, J. B, Kapadia, S. J, Karki, S, Karvinen, K. S, Kashyap, R, Kasprzack, M, Katsanevas, S, Katsavounidis, E, Katzman, W, Kaufer, S, Kawabe, K, Keerthana, Kefelian, F, Keitel, D, Kennedy, R, Key, J. S, Khalili, F. Y, Khan, H, Khan, I and Khan, Khan, Z, Khazanov, E. A, Khursheed, M, Kijbunchoo, N, Kim, Chunglee and Kim, J. C., Kim, K, Kim, W, Kim, W. S, Y-M and Kimball, King, E. J, King, P. J, Kinley-Hanlon, M, Kirchhoff, R, Kissel, J. S, Kleybolte, L, Klika, J. H, Klimenko, S, Knowles, T. D, Koch, P, Koehlenbeck, S. M, Koekoek, G, Koley, S, Kondrashov, V and Kontos, Koper, N, Korobko, M, Korth, W. Z, Kowalska, I and Kozak, D. B., Kringel, V and Krishnendu, Krolak, A, Kuehn, G, Kumar, A, Kumar, P, Kumar, R, Kumar, S, Kuo, L, Kutynia, A, Kwang, S, Lackey, B. D, Lai, K. H, Lam, T. L, Landry, M, Lane, B. B, Lang, R. N, Lange, J, Lantz, B, Lanza, R. K, Lartaux-Vollard, A, Lasky, P. D, Laxen, M, Lazzarini, A, Lazzaro, C, Leaci, P, Leavey, S, Lecoeuche, Y. K, Lee, C. H, Lee, H. K, Lee, H. M, Lee, H. W, Lee, J, Lee, K, Lehmann, J, Lenon, A, Leroy, N, Letendre, N, Levin, Y, Li, J, K. J. L, Li, T. G. F, Li, Li, X, Lin, F, Linde, F, Linker, S. D, Littenberg, T. B, Liu, J, Liu, X, R. K. L, Lo, Lockerbie, N. A, London, L. T, Longo, A, Lorenzini, M, Loriette, V and Lormand, Losurdo, G, Lough, J. D, Lousto, C. O, Lovelace, G, Lower, M. E, Lueck, H, Lumaca, D, Lundgren, A. P, Lynch, R, Ma, Y, Macas, R, Macfoy, S, Macinnis, M, Macleod, D. M, Macquet, A, Magana-Sandoval, F, Zertuche, Magana and Magee, L., R. M., Majorana, E, Maksimovic, I and Malik, Man, N, Mandic, V and Mangano, V and Mansell, G. L., Manske, M, Mantovani, M, Marchesoni, F, Marion, F, Marka, S, Marka, Z, Markakis, C, Markosyan, A. S, Markowitz, A, Maros, E, Marquina, A, Marsat, S, Martelli, F, Martin, I. W, Martin, R. M, Martynov, Mason, K, Massera, E, Masserot, A, Massinger, T. 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ENS Paris (FRDPENS), École normale supérieure - Paris (ENS Paris), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-École normale supérieure - Paris (ENS Paris), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Centre National de la Recherche Scientifique (CNRS), Université de Strasbourg (UNISTRA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Albert, A., André, M., Anghinolfi, M., Ardid, M., Aubert, J. -J., Aublin, J., Avgitas, T., Baret, B., Barrios-Martí, J., Basa, S., Belhorma, B., Bertin, V., Biagi, S., Bormuth, R., Boumaaza, J., Bourret, S., Bouwhuis, M. C., Brânzaş, H., Bruijn, R., Brunner, J., Busto, J., Capone, A., Caramete, L., Carr, J., Celli, S., Chabab, M., El Moursli, R. Cherkaoui, Chiarusi, T., Circella, M., Coelho, J. A. B., Coleiro, A., Colomer, M., Coniglione, R., Costantini, H., Coyle, P., Creusot, A., Díaz, A. F., Deschamps, A., Distefano, C., Di Palma, I., Domi, A., Donà, R., Donzaud, C., Dornic, D., Drouhin, D., Eberl, T., El Bojaddaini, I., El Khayati, N., Elsässer, D., Enzenhöfer, A., Ettahiri, A., Fassi, F., Felis, I., Fermani, P., Ferrara, G., Fusco, L., Gay, P., Glotin, H., Grégoire, T., Ruiz, R. Gracia, Graf, K., Hallmann, S., Van Haren, H., Heijboer, A. J., Hello, Y., Hernández-Rey, J. J., Hößl, J., Hofestädt, J., Illuminati, G., De Jong, M., Jongen, M., Kadler, M., Kalekin, O., Katz, U., Khan-Chowdhury, N. R., Kouchner, A., Kreter, M., Kreykenbohm, I., Kulikovskiy, V., Lachaud, C., Lahmann, R., Lefèvre, D., Leonora, E., Levi, G., Lotze, M., Loucatos, S., Maggi, G., Marcelin, M., Margiotta, A., Marinelli, A., Martínez-Mora, J. A., Mele, R., Melis, K., Migliozzi, P., Moussa, A., Navas, S., Nezri, E., Nuñez, A., Organokov, M., Pǎvǎlaş, G. E., Pellegrino, C., Piattelli, P., Popa, V., Pradier, T., Quinn, L., Racca, C., Randazzo, N., Riccobene, G., Sánchez-Losa, A., Saldaña, M., Salvadori, I., Samtleben, D. F. E., Sanguineti, M., Sapienza, P., Schüssler, F., Spurio, M., Stolarczyk, Th., Taiuti, M., Tayalati, Y., Trovato, A., Vallage, B., Van Elewyck, V., Versari, F., Vivolo, D., Wilms, J., Zaborov, D., Zornoza, J. D., Zñiga, J., Aartsen, M. G., Ackermann, M., Adams, J., Aguilar, J. A., Ahlers, M., Ahrens, M., Altmann, D., Andeen, K., Anderson, T., Ansseau, I., Anton, G., Argüelles, C., Auffenberg, J., Axani, S., Backes, P., Bagherpour, H., Bai, X., Barbano, A., Barron, J. P., Barwick, S. W., Baum, V., Bay, R., Beatty, J. J., Tjus, J. Becker, Becker, K. -H., Benzvi, S., Berley, D., Bernardini, E., Besson, D. Z., Binder, G., Bindig, D., Blaufuss, E., Blot, S., Bohm, C., Börner, M., Bos, F., Böser, S., Botner, O., Bourbeau, E., Bourbeau, J., Bradascio, F., Braun, J., Brenzke, M., Bretz, H. -P., Bron, S., Brostean-Kaiser, J., Burgman, A., Busse, R. S., Carver, T., Cheung, E., Chirkin, D., Clark, K., Classen, L., Collin, G. H., Conrad, J. M., Coppin, P., Correa, P., Cowen, D. F., Cross, R., Dave, P., Day, M., De André, J. P. A. M., De Clercq, C., Delaunay, J. J., Dembinski, H., Deoskar, K., De Ridder, S., Desiati, P., De Vries, K. D., De Wasseige, G., De With, M., Deyoung, T., Díaz-Vélez, J. C., Lorenzo, V. Di, Dujmovic, H., Dumm, J. P., Dunkman, M., Dvorak, E., Eberhardt, B., Ehrhardt, T., Eichmann, B., Eller, P., Evenson, P. A., Fahey, S., Fazely, A. R., Felde, J., Filimonov, K., Finley, C., Franckowiak, A., Friedman, E., Fritz, A., Gaisser, T. K., Gallagher, J., Ganster, E., Garrappa, S., Gerhardt, L., Ghorbani, K., Giang, W., Glauch, T., Glüsenkamp, T., Goldschmidt, A., Gonzalez, J. G., Grant, D., Griffith, Z., Haack, C., Hallgren, A., Halve, L., Halzen, F., Hanson, K., Hebecker, D., Heereman, D., Helbing, K., Hellauer, R., Hickford, S., Hignight, J., Hill, G. C., Hoffman, K. D., Hoffmann, R., Hoinka, T., Hokanson-Fasig, B., Hoshina, K., Huang, F., Huber, M., Hultqvist, K., Hünnefeld, M., Hussain, R., In, S., Iovine, N., Ishihara, A., Jacobi, E., Japaridze, G. S., Jeong, M., Jero, K., Jones, B. J. P., Kalaczynski, P., Kang, W., Kappes, A., Kappesser, D., Karg, T., Karle, A., Kauer, M., Keivani, A., Kelley, J. L., Kheirandish, A., Kim, J., Kintscher, T., Kiryluk, J., Kittler, T., Klein, S. R., Koirala, R., Kolanoski, H., Köpke, L., Kopper, C., Kopper, S., Koschinsky, J. P., Koskinen, D. J., Kowalski, M., Krings, K., Kroll, M., Krückl, G., Kunwar, S., Kurahashi, N., Kyriacou, A., Labare, M., Lanfranchi, J. L., Larson, M. J., Lauber, F., Leonard, K., Leuermann, M., Liu, Q. R., Lohfink, E., Mariscal, C. J. Lozano, Lu, L., Lünemann, J., Luszczak, W., Madsen, J., Mahn, K. B. M., Makino, Y., Mancina, S., Mariş, I. C., Maruyama, R., Mase, K., Maunu, R., Meagher, K., Medici, M., Meier, M., Menne, T., Merino, G., Meures, T., Miarecki, S., Micallef, J., Momenté, G., Montaruli, T., Moore, R. W., Moulai, M., Nagai, R., Nahnhauer, R., Nakarmi, P., Naumann, U., Neer, G., Niederhausen, H., Nowicki, S. C., Nygren, D. R., Pollmann, A. Obertacke, Olivas, A., O'Murchadha, A., O'Sullivan, E., Palczewski, T., Pandya, H., Pankova, D. V., Peiffer, P., Pepper, J. A., De Los Heros, C. Pérez, Pieloth, D., Pinat, E., Pizzuto, A., Plum, M., Price, P. B., Przybylski, G. T., Raab, C., Rameez, M., Rauch, L., Rawlins, K., Rea, I. C., Reimann, R., Relethford, B., Renzi, G., Resconi, E., Rhode, W., Richman, M., Robertson, S., Rongen, M., Rott, C., Ruhe, T., Ryckbosch, D., Rysewyk, D., Safa, I., Herrera, S. E. Sanchez, Sandrock, A., Sandroos, J., Santander, M., Sarkar, S., Satalecka, K., Schaufel, M., Schlunder, P., Schmidt, T., Schneider, A., Schneider, J., Schöneberg, S., Schumacher, L., Sclafani, S., Seckel, D., Seunarine, S., Soedingrekso, J., Soldin, D., Song, M., Spiczak, G. M., Spiering, C., Stachurska, J., Stamatikos, M., Stanev, T., Stasik, A., Stein, R., Stettner, J., Steuer, A., Stezelberger, T., Stokstad, R. G., Stößl, A., Strotjohann, N. L., Stuttard, T., Sullivan, G. W., Sutherland, M., Taboada, I., Tenholt, F., Ter-Antonyan, S., Terliuk, A., Tilav, S., Toale, P. A., Tobin, M. N., Tönnis, C., Toscano, S., Tosi, D., Tselengidou, M., Tung, C. F., Turcati, A., Turcotte, R., Turley, C. F., Ty, B., Unger, E., Elorrieta, M. A. Unland, Usner, M., Vandenbroucke, J., Van Driessche, W., Van Eijk, D., Van Eijndhoven, N., Vanheule, S., Van Santen, J., Vraeghe, M., Walck, C., Wallace, A., Wallraff, M., Wandler, F. D., Wandkowsky, N., Watson, T. B., Waza, A., Weaver, C., Weiss, M. 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W., Banagiri, S., Barayoga, J. C., Barclay, S. E., Barish, B. C., Barker, D., Barkett, K., Barnum, S., Barone, F., Barr, B., Barsotti, L., Barsuglia, M., Barta, D., Bartlett, J., Bartos, I., Bassiri, R., Basti, A., Bawaj, M., Bayley, J. C., Bazzan, M., Bécsy, B., Bejger, M., Belahcene, I., Bell, A. S., Beniwal, D., Berger, B. K., Bergmann, G., Bernuzzi, S., Bero, J. J., Berry, C. P. L., Bersanetti, D., Bertolini, A., Betzwieser, J., Bhandare, R., Bidler, J., Bilenko, I. A., Bilgili, S. A., Billingsley, G., Birch, J., Birney, R., Birnholtz, O., Biscans, S., Biscoveanu, S., Bisht, A., Bitossi, M., Bizouard, M. A., Blackburn, J. K., Blair, C. D., Blair, D. G., Blair, R. M., Bloemen, S., Bode, N., Boer, M., Boetzel, Y., Bogaert, G., Bondu, F., Bonilla, E., Bonnand, R., Booker, P., Boom, B. A., Booth, C. D., Bork, R., Boschi, V., Bose, S., Bossie, K., Bossilkov, V., Bosveld, J., Bouffanais, Y., Bozzi, A., Bradaschia, C., Brady, P. R., Bramley, A., Branchesi, M., Brau, J. E., Briant, T., Briggs, J. H., Brighenti, F., Brillet, A., Brinkmann, M., Brisson, V., Brockill, P., Brooks, A. F., Brown, D. D., Brunett, S., Buikema, A., Bulik, T., Bulten, H. J., Buonanno, A., Buskulic, D., Buy, C., Byer, R. L., Cabero, M., Cadonati, L., Cagnoli, G., Cahillane, C., Bustillo, J. Calderón, Callister, T. A., Calloni, E., Camp, J. B., Campbell, W. A., Cannon, K. C., Cao, H., Cao, J., Capocasa, E., Carbognani, F., Caride, S., Carney, M. F., Carullo, G., Diaz, J. Casanueva, Casentini, C., Caudill, S., Cavaglià, M., Cavalier, F., Cavalieri, R., Cella, G., Cerdá-Durán, P., Cerretani, G., Cesarini, E., Chaibi, O., Chakravarti, K., Chamberlin, S. J., Chan, M., Chao, S., Charlton, P., Chase, E. A., Chassande-Mottin, E., Chatterjee, D., Chaturvedi, M., Cheeseboro, B. D., Chen, H. Y., Chen, X., Chen, Y., Cheng, H. -P., Cheong, C. K., Chia, H. Y., Chincarini, A., Chiummo, A., Cho, G., Cho, H. S., Cho, M., Christensen, N., Chu, Q., Chua, S., Chung, K. W., Chung, S., Ciani, G., Ciobanu, A. A., Ciolfi, R., Cipriano, F., Cirone, A., Clara, F., Clark, J. A., Clearwater, P., Cleva, F., Cocchieri, C., Coccia, E., Cohadon, P. -F., Cohen, D., Colgan, R., Colleoni, M., Collette, C. G., Collins, C., Cominsky, L. R., Constancio, M., Conti, L., Cooper, S. J., Corban, P., Corbitt, T. R., Cordero-Carrión, I., Corley, K. R., Cornish, N., Corsi, A., Cortese, S., Costa, C. A., Cotesta, R., Coughlin, M. W., Coughlin, S. B., Coulon, J. -P., Countryman, S. T., Couvares, P., Covas, P. B., Cowan, E. E., Coward, D. M., Cowart, M. J., Coyne, D. C., Coyne, R., Creighton, J. D. E., Creighton, T. D., Cripe, J., Croquette, M., Crowder, S. G., Cullen, T. J., Cumming, A., Cunningham, L., Cuoco, E., Canton, T. Dal, Dálya, G., Danilishin, S. L., D'Antonio, S., Danzmann, K., Dasgupta, A., Costa, C. F. Da Silva, Datrier, L. E. H., Dattilo, V., Dave, I., Davier, M., Davis, D., Daw, E. J., Debra, D., Deenadayalan, M., Degallaix, J., De Laurentis, M., Deléglise, S., Pozzo, W. Del, Demarchi, L. M., Demos, N., Dent, T., Denys, M., De Pietri, R., Derby, J., De Rosa, Rosario., De Rossi, C., Desalvo, R., De Varona, O., Dhurandhar, S., Díaz, M. C., Dietrich, T., Fiore, L. Di., Giovanni, M. Di., Di Girolamo, T., Lieto, A. Di., Ding, B., Pace, S. Di., Renzo, F. Di., Dmitriev, A., Doctor, Z., Donovan, F., Dooley, K. L., Doravari, S., Dorrington, I., Downes, T. P., Drago, M., Driggers, J. C., Du, Z., Ducoin, J. -G., Dupej, P., Dwyer, S. E., Easter, P. J., Edo, T. B., Edwards, M. C., Effler, A., Ehrens, P., Eichholz, J., Eikenberry, S. S., Eisenmann, M., Eisenstein, R. A., Essick, R. C., Estelles, H., Estevez, D., Etienne, Z. B., Etzel, T., Evans, M., Evans, T. M., Fafone, V., Fair, H., Fairhurst, S., Fan, X., Farinon, S., Farr, B., Farr, W. M., Fauchon-Jones, E. J., Favata, M., Fays, M., Fazio, M., Fee, C., Feicht, J., Fejer, M. M., Feng, F., Fernandez-Galiana, A., Ferrante, I., Ferreira, E. C., Ferreira, T. A., Ferrini, F., Fidecaro, F., Fiori, I., Fiorucci, D., Fishbach, M., Fisher, R. P., Fishner, J. M., Fitz-Axen, M., Flaminio, R., Fletcher, M., Flynn, E., Fong, H., Font, J. A., Forsyth, P. W. F., Fournier, J. -D., Frasca, S., Frasconi, F., Frei, Z., Freise, A., Frey, R., Frey, V., Fritschel, P., Frolov, V. V., Fulda, P., Fyffe, M., Gabbard, H. A., Gadre, B. U., Gaebel, S. M., Gair, J. R., Gammaitoni, L., Ganija, M. R., Gaonkar, S. G., Garcia, A., García-Quirós, C., Garufi, F., Gateley, B., Gaudio, S., Gaur, G., Gayathri, V., Gemme, G., Genin, E., Gennai, A., George, D., George, J., Gergely, L., Germain, V., Ghonge, S., Ghosh, Abhirup, Ghosh, Archisman, Ghosh, S., Giacomazzo, B., Giaime, J. A., Giardina, K. D., Giazotto, A., Gill, K., Giordano, G., Glover, L., Godwin, P., Goetz, E., Goetz, R., Goncharov, B., González, G., Castro, J. M. Gonzalez, Gopakumar, A., Gorodetsky, M. L., Gossan, S. 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Perreca, A, Pfeiffer, H, Phelps, M, Phukon, K, Piccinni, O, Pichot, M, Piergiovanni, F, Pillant, G, Pinard, L, Pirello, M, Pitkin, M, Poggiani, R, Pong, D, Ponrathnam, S, Popolizio, P, Porter, E, Powell, J, Prajapati, A, Prasad, J, Prasai, K, Prasanna, R, Pratten, G, Prestegard, T, Privitera, S, Prodi, G, Prokhorov, L, Puncken, O, Punturo, M, Puppo, P, Pürrer, M, Qi, H, Quetschke, V, Quinonez, P, Quintero, E, Quitzow-James, R, Raab, F, Radkins, H, Radulescu, N, Raffai, P, Raja, S, Rajan, C, Rajbhandari, B, Rakhmanov, M, Ramirez, K, Ramos-Buades, A, Rana, J, Rao, K, Rapagnani, P, Raymond, V, Razzano, M, Read, J, Regimbau, T, Rei, L, Reid, S, Reitze, D, Ren, W, Ricci, F, Richardson, C, Richardson, J, Ricker, P, Riles, K, Rizzo, M, Robertson, N, Robie, R, Robinet, F, Rocchi, A, Rolland, L, Rollins, J, Roma, V, Romanelli, M, Romano, R, Romel, C, Romie, J, Rose, K, Rosińska, D, Rosofsky, S, Ross, M, Rowan, S, Rüdiger, A, Ruggi, P, Rutins, G, Ryan, K, Sachdev, S, Sadecki, T, Sakellariadou, 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Stocks, D, Stone, R, Stops, D, Strain, K, Stratta, G, Strigin, S, Strunk, A, Sturani, R, Stuver, A, Sudhir, V, Summerscales, T, Sun, L, Sunil, S, Suresh, J, Sutton, P, Swinkels, B, Szczepańczyk, M, Tacca, M, Tait, S, Talbot, C, Talukder, D, Tanner, D, Tápai, M, Taracchini, A, Tasson, J, Taylor, R, Thies, F, Thomas, M, Thomas, P, Thondapu, S, Thorne, K, Thrane, E, Tiwari, S, Tiwari, V, Toland, K, Tonelli, M, Tornasi, Z, Torres-Forné, A, Torrie, C, Töyrä, D, Travasso, F, Traylor, G, Tringali, M, Trozzo, L, Trudeau, R, Tsang, K, Tse, M, Tso, R, Tsukada, L, Tsuna, D, Tuyenbayev, D, Ueno, K, Ugolini, D, Unnikrishnan, C, Urban, A, Usman, S, Vahlbruch, H, Vajente, G, Valdes, G, Van Bakel, N, Van Beuzekom, M, Van Den Brand, J, Broeck, C, Vander-Hyde, D, Schaaf, L, Van Heijningen, J, Van Veggel, A, Vardaro, M, Varma, V, Vass, S, Vasúth, M, Vecchio, A, Vedovato, G, Veitch, J, Veitch, P, Venkateswara, K, Venugopalan, G, Verkindt, D, Vetrano, F, Viceré, A, Viets, A, Vine, D, Vinet, J, Vitale, S, 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C., Diaz, A. F., Dona, R., Elsasser, D., Enzenhofer, A., Gregoire, T., Ruiz, R. G., Hernandez-Rey, J. J., Hossl, J., Hofestadt, J., Lefevre, D., Martinez-Mora, J. A., Nunez, A., Pavalas, G. E., Sanchez-Losa, A., Saldana, M., Schussler, F., Stolarczyk, T., Zniga, J., Arguelles, C., Tjus, J. B., Borner, M., Boser, S., De Andre, J. P. A. M., Diaz-Velez, J. C., Lorenzo, V. D., Glusenkamp, T., Hunnefeld, M., Kopke, L., Kruckl, G., Mariscal, C. J. L., Lunemann, J., Maris, I. C., Momente, G., Pollmann, A. O., De Los Heros, C. P., Herrera, S. E. S., Schoneberg, S., Stossl, A., Tonnis, C., Elorrieta, M. A. U., Arene, M., Becsy, B., Bustillo, J. C., Diaz, J. C., Cavaglia, M., Cerda-Duran, P., Cordero-Carrion, I., Canton, T. D., Dalya, G., Costa, C. F. D. S., Deleglise, S., Pozzo, W. D., Diaz, M. C., Girolamo, T. Di., Garcia-Quiros, C., Ghosh, A., Gonzalez, G., Castro, J. M. G., Kefelian, F., Kim, C., Krolak, A., Luck, H., Magana-Sandoval, F., Zertuche, L. 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Yeeles, Dw, Yu, Hc, Yuen, Shr, Zadrozny, Ak, Zendri, Jp, Zhu, Xj, Zucker, Me, Physics, Faculty of Sciences and Bioengineering Sciences, Vriendenkring VUB, Elementary Particle Physics, ITA, USA, GBR, FRA, DEU, ESP, Centre Tecnològic de Vilanova i la Geltrú, Universitat Politècnica de Catalunya. LAB - Laboratori d'Aplicacions Bioacústiques, COMUE Université Côte d'Azur (2015 - 2019) (COMUE UCA)-COMUE Université Côte d'Azur (2015 - 2019) (COMUE UCA)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de la Côte d'Azur, Université Côte d'Azur (UCA)-COMUE Université Côte d'Azur (2015 - 2019) (COMUE UCA)-Université Côte d'Azur (UCA)-Centre National de la Recherche Scientifique (CNRS), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7), Institut national des sciences de l'Univers (INSU - CNRS)-Institut de Recherche pour le Développement (IRD [France-Sud])-Centre National de la Recherche Scientifique (CNRS)-Observatoire de la Côte d'Azur, Université Côte d'Azur (UCA)-Université Côte d'Azur (UCA), and Institut de Recherche pour le Développement (IRD)-Aix Marseille Université (AMU)-Université de Toulon (UTLN)-Centre National de la Recherche Scientifique (CNRS)
Subjects: Astrofísica, collapse [supernova], neutron star: binary, EVENTS GW150914, Gravitació, 010504 meteorology & atmospheric sciences, neutrino: energy: high, Astronomy, RAY, Binary number, binary [neutron star], Astrophysics, 7. Clean energy, 01 natural sciences, Physical Chemistry, Atomic, IceCube, neutrino, Particle and Plasma Physics, Astronomi, astrofysik och kosmologi, black hole, Astronomy, Astrophysics and Cosmology, LIGO, 010303 astronomy & astrophysics, gravitational wave, ELECTROMAGNETIC SIGNALS, QC, QB, Settore FIS/01, Physics, High Energy Astrophysical Phenomena (astro-ph.HE), astro-ph.HE, [PHYS]Physics [physics], Astrophysics::Instrumentation and Methods for Astrophysics, neutrinos, gravitational waves, 520 Astronomie und zugeordnete Wissenschaften, ddc, observatory, Supernova, astrophysics: density, Physical Sciences, Neutrino, Astrophysics - High Energy Astrophysical Phenomena, Astronomy and Astrophysics, Space and Planetary Science, Astronomical and Space Sciences, signature, Physical Chemistry (incl. Structural), supernova: collapse, Astrophysics::High Energy Astrophysical Phenomena, FOS: Physical sciences, Astrophysics::Cosmology and Extragalactic Astrophysics, Astronomy & Astrophysics, Gravitational waves, emission [gravitational radiation], Ones gravitacionals, Coincident, 0103 physical sciences, Gravitational Waves, Neutrinos, LIGO, Virgo, Antares, IceCube, Nuclear, ddc:530, Neutrins, energy: high [neutrino], Neutrinos, STFC, Astrophysique, Astrophysics::Galaxy Astrophysics, 0105 earth and related environmental sciences, Science & Technology, ANTARES, Gravitational wave, Virgo, Organic Chemistry, RCUK, Molecular, Astronomie, Astronomy and Astrophysic, 530 Physik, Sciences de l'espace, Black hole, messenger, Neutron star, Antares, Physics and Astronomy, FISICA APLICADA, Física::Astronomia i astrofísica [Àrees temàtiques de la UPC], gravitational radiation: emission, density [astrophysics], ddc:520, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], EMISSION
Abstract: [EN] Astrophysical sources of gravitational waves, such as binary neutron star and black hole mergers or core-collapse supernovae, can drive relativistic outflows, giving rise to non-thermal high-energy emission. High-energy neutrinos are signatures of such outflows. The detection of gravitational waves and high-energy neutrinos from common sources could help establish the connection between the dynamics of the progenitor and the properties of the out¿ow. We searched for associated emission of gravitational waves and high-energy neutrinos from astrophysical transients with minimal assumptions using data from Advanced LIGO from its first observing run O1, and data from the ANTARES and IceCube neutrino observatories from the same time period. We focused on candidate events whose astrophysical origins could not be determined from a single messenger. We found no significant coincident candidate, which we used to constrain the rate density of astrophysical sources dependent on their gravitational-wave and neutrino emission processes., The ANTARES Collaboration acknowledge the financial support of the funding agencies: Centre National de la Recherche Scientifique (CNRS), Commissariat a l'energie atomique et aux energies alternatives (CEA), Commission Europeenne (FEDER fund and Marie Curie Program), Institut Universitaire de France (IUF), IdEx program and UnivEarthS Labex program at Sorbonne Paris Cite (ANR-10-LABX-0023 and ANR-11-IDEX-0005-02), Labex OCEVU (ANR-11-LABX-0060) and the A*MIDEX project (ANR-11-IDEX-0001-02), Region Ile-de-France (DIM-ACAV), Region Alsace (contrat CPER), Region Provence-Alpes-Cote d'Azur, Departement du Var and Ville de La Seyne-sur-Mer, France; Bundesministerium fur Bildung und Forschung (BMBF), Germany; Istituto Nazionale di Fisica Nucleare (INFN), Italy; Nederlandse organisatie voor Wetenschappelijk Onderzoek (NWO), the Netherlands; Council of the President of the Russian Federation for young scientists and leading scientific schools supporting grants, Russia; National Authority for Scientific Research (ANCS), Romania; Ministerio de Economia y Competitividad (MINECO): Plan Estatal de Investigacion (refs. FPA2015-65150-C3-1-P, -2-P and -3-P, (MINECO/FEDER)), Severo Ochoa Centre of Excellence and MultiDark Consolider (MINECO), and Prometeo and Grisolia programs (Generalitat Valenciana), Spain; Ministry of Higher Education, Scientific Research and Professional Training, Morocco. We also acknowledge the technical support of Ifremer, AIM and Foselev Marine for the sea operation and the CC-IN2P3 for the computing facilities. The IceCube Collaboration gratefully acknowledges the following support: USA-U.S. National Science Foundation-Office of Polar Programs, U.S. National Science Foundation-Physics Division, Wisconsin Alumni Research Foundation, Center for High Throughput Computing (CHTC) at the University of Wisconsin-Madison, Open Science Grid (OSG), Extreme Science and Engineering Discovery Environment (XSEDE), U.S. Department of Energy-National Energy Research Scientific Computing Center, Particle astrophysics research computing center at the University of Maryland, Institute for Cyber-Enabled Research at Michigan State University, and Astroparticle physics computational facility at Marquette University; Belgium-Funds for Scientific Research (FRS-FNRS and FWO), FWO Odysseus and Big Science programmes, and Belgian Federal Science Policy Office (Belspo); Germany-Bundesministerium fur Bildung und Forschung (BMBF), Deutsche Forschungsgemeinschaft (DFG), Helmholtz Alliance for Astroparticle Physics (HAP), Initiative and Networking Fund of the Helmholtz Association, Deutsches Elektronen Synchrotron (DESY), and High Performance Computing cluster of the RWTH Aachen; Sweden-Swedish Research Council, Swedish Polar Research Secretariat, Swedish National Infrastructure for Computing (SNIC), and Knut and Alice Wallenberg Foundation; Australia-Australian Research Council; Canada-Natural Sciences and Engineering Research Council of Canada, Calcul Quebec, Compute Ontario, Canada Foundation for Innovation, WestGrid, and Compute Canada; Denmark-Villum Fonden, Danish National Research Foundation (DNRF); New Zealand-Marsden Fund; Japan-Japan Society for Promotion of Science (JSPS) and Institute for Global Prominent Research (IGPR) of Chiba University; Korea-National Research Foundation of Korea (NRF); Switzerland-Swiss National Science Foundation (SNSF). The LIGO Scientific Collaboration and the Virgo Collaboration gratefully acknowledge the support of the United States National Science Foundation (NSF) for the construction and operation of the LIGO Laboratory and Advanced LIGO as well as the Science and Technology Facilities Council (STFC) of the United Kingdom, the Max-Planck-Society (MPS), and the State of Niedersachsen/Germany for support of the construction of Advanced LIGO and construction and operation of the GEO600 detector. Additional support for Advanced LIGO was provided by the Australian Research Council, etc.
Published: 2019
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