Author: "Juan Calderón Bustillo" / Topic: 010306 general physics - Searchworks@Jio Institute Digital Library Search Results

15 results on '"Juan Calderón Bustillo"'

1. Post-merger chirps from binary black holes as probes of the final black-hole horizon

Author: Deirdre Shoemaker, Pablo Laguna, Christopher Evans, Juan Calderón Bustillo, Grace Kim, and James A. Clark
Subjects: Physics::General Physics, Astrophysics::High Energy Astrophysical Phenomena, General Physics and Astronomy, FOS: Physical sciences, lcsh:Astrophysics, Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, General Relativity and Quantum Cosmology (gr-qc), 01 natural sciences, General Relativity and Quantum Cosmology, Binary black hole, 0103 physical sciences, lcsh:QB460-466, 010306 general physics, 010303 astronomy & astrophysics, Physics, Einstein Telescope, Gravitational wave, Horizon, LIGO, lcsh:QC1-999, Black hole, Numerical relativity, Apparent horizon, lcsh:Physics
Abstract: The merger of a binary black hole gives birth to a highly distorted final black hole. The gravitational radiation emitted as this black hole relaxes presents us with the unique opportunity to probe extreme gravity and its connection with the dynamics of the black hole horizon. Using numerical relativity simulations, we demonstrate a connection between a concrete observable feature in the gravitational waves and geometrical features on the dynamical apparent horizon of the final black hole. Specifically, we show how the line-of-sight passage of a "cusp"-like defect on the horizon of the final black hole correlates with "chirp"-like frequency peaks in the post-merger gravitational-waves. These post-merger chirps should be observed and analyzed as the sensitivity of LIGO and Virgo increases and as future generation detectors, such as LISA and the Einstein Telescope, become operational., Comment: Version accepted in Communications Physics. 11 pages, 5 figures in main text, 3 Figures in Supp. Material
Published: 2020
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2. Confusing Head-On Collisions with Precessing Intermediate-Mass Binary Black Hole Mergers

Author: Nicolas Sanchis-Gual, Alejandro Torres-Forné, José A. Font, and Juan Calderón Bustillo
Subjects: Physics, FOS: Physical sciences, General Physics and Astronomy, General Relativity and Quantum Cosmology (gr-qc), Astrophysics, 01 natural sciences, General Relativity and Quantum Cosmology, LIGO, Supernova, Binary black hole, 0103 physical sciences, 010306 general physics, Degeneracy (mathematics), 010303 astronomy & astrophysics
Abstract: We report a degeneracy between the gravitational-wave signals from quasi-circular precessing black-hole mergers and those from extremely eccentric mergers, namely head-on collisions. Performing model selection on numerically simulated signals of head-on collisions using models for quasi-circular binaries we find that, for signal-to-noise ratios of 15 and 25, typical of Advanced LIGO observations, head-on mergers with respective total masses of $M\in (125,300)M_\odot$ and $M\in (200,440)M_\odot$ would be identified as precessing quasi-circular intermediate-mass black hole binaries, located at a much larger distance. Ruling out the head-on scenario would require to perform model selection using currently nonexistent waveform models for head-on collisions, together with the application of astrophysically motivated priors on the (rare) occurrence of those events. We show that in situations where standard parameter inference of compact binaries may report component masses inside (outside) the pair-instability supernova gap, the true object may be a head-on merger with masses outside (inside) this gap. We briefly discuss the potential implications of these findings for the recent gravitational-wave detection GW190521, which we analyse in detail in [Phys. Rev. Lett. 126, 081101]., 10 pages, 9 Figures. Version accepted in Phys. Rev. Lett. Includes Supplementary Material
Published: 2021
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3. GW190521 as a Merger of Proca Stars: A Potential New Vector Boson of 8.7×10−13 eV

Author: Nicolas Sanchis-Gual, Juan Calderón Bustillo, Carlos A. R. Herdeiro, José A. Font, Samson H. W. Leong, Eugen Radu, Alejandro Torres-Forné, A. Vajpeyi, and Rory Smith
Subjects: Physics, Particle physics, Astrophysics::High Energy Astrophysical Phenomena, Star (game theory), Theoretical models, General Physics and Astronomy, Astrophysics::Cosmology and Extragalactic Astrophysics, 01 natural sciences, Vector boson, Black hole, General Relativity and Quantum Cosmology, Stars, Supernova, 0103 physical sciences, 010306 general physics, Luminosity distance, Astrophysics::Galaxy Astrophysics, Spin-½
Abstract: Advanced LIGO-Virgo have reported a short gravitational-wave signal (GW190521) interpreted as a quasicircular merger of black holes, one at least populating the pair-instability supernova gap, that formed a remnant black hole of ${M}_{f}\ensuremath{\sim}142\text{ }\text{ }{M}_{\ensuremath{\bigodot}}$ at a luminosity distance of ${d}_{L}\ensuremath{\sim}5.3\text{ }\text{ }\mathrm{Gpc}$. With barely visible pre-merger emission, however, GW190521 merits further investigation of the pre-merger dynamics and even of the very nature of the colliding objects. We show that GW190521 is consistent with numerically simulated signals from head-on collisions of two (equal mass and spin) horizonless vector boson stars (aka Proca stars), forming a final black hole with ${M}_{f}=23{1}_{\ensuremath{-}17}^{+13}\text{ }\text{ }{M}_{\ensuremath{\bigodot}}$, located at a distance of ${d}_{L}=57{1}_{\ensuremath{-}181}^{+348}\text{ }\text{ }\mathrm{Mpc}$. This provides the first demonstration of close degeneracy between these two theoretical models, for a real gravitational-wave event. The favored mass for the ultralight vector boson constituent of the Proca stars is ${\ensuremath{\mu}}_{\mathrm{V}}=8.7{2}_{\ensuremath{-}0.82}^{+0.73}\ifmmode\times\else\texttimes\fi{}{10}^{\ensuremath{-}13}\text{ }\text{ }\mathrm{eV}$. Confirmation of the Proca star interpretation, which we find statistically slightly preferred, would provide the first evidence for a long sought dark matter particle.
Published: 2021
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4. Addendum to 'Numerical relativity injection analysis of signals from generically spinning intermediate mass black hole binaries in Advanced LIGO data'

Author: V. Gayathri, Archana Pai, Juan Calderón Bustillo, and K. Chandra
Subjects: Physics, Orbital plane, Spins, 010308 nuclear & particles physics, Gravitational wave, Astrophysics::High Energy Astrophysical Phenomena, Astrophysics, 01 natural sciences, LIGO, Black hole, Numerical relativity, Intermediate-mass black hole, 0103 physical sciences, Sensitivity (control systems), 010306 general physics
Abstract: The advent of gravitational wave (GW) astronomy has provided us with observations of black holes more massive than those known from x-ray astronomy. However, the observation of an intermediate-mass black hole (IMBH) remains a big challenge. After their second observing run, the LIGO Virgo Scientific collaborations (LVC) placed upper limits on the coalescence rate density of nonprecessing IMBH binaries (IMBHBs). In this Numerical Relativity Injection Analysis (NuRIA), we explore the sensitivity of two of the search pipelines used by the LVC to signals from 69 numerically simulated IMBHBs with total mass greater than $200\text{ }\text{ }{M}_{\ensuremath{\bigodot}}$ having generic spins, out of which 27 have a precessing orbital plane. In particular, we compare the matched-filter search PyCBC, and the coherent model-independent search technique cWB. We find that, in general, cWB is more sensitive to IMBHBs than PyCBC, with the difference in sensitivity depending on the masses and spins of the source. Consequently, we use cWB to place the first upper limits on the merger rate of generically spinning IMBH binaries using publicly available data from the first Advanced LIGO observing run.
Published: 2020
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5. Black-hole spectroscopy, the no-hair theorem and GW150914: Kerr vs. Occam

Author: Juan Calderón Bustillo, Eric Thrane, and Paul D. Lasky
Subjects: Physics, 010308 nuclear & particles physics, Astrophysics::High Energy Astrophysical Phenomena, FOS: Physical sciences, Perturbation (astronomy), Binary number, General Relativity and Quantum Cosmology (gr-qc), 01 natural sciences, General Relativity and Quantum Cosmology, Black hole, Superposition principle, Amplitude, No-hair theorem, 0103 physical sciences, Prior probability, 010306 general physics, Free parameter, Mathematical physics
Abstract: The "no-hair" theorem states that astrophysical black holes are fully characterised by just two numbers: their mass and spin. The gravitational-wave emission from a perturbed black-hole consists of a superposition of damped sinusoids, known as \textit{quasi-normal modes}. Quasi-normal modes are specified by three integers $(\ell,m,n)$: the $(\ell, m)$ integers describe the angular properties and $(n)$ specifies the (over)tone. If the no-hair theorem holds, the frequencies and damping times of quasi-normal modes are determined uniquely by the mass and spin of the black hole, while phases and amplitudes depend on the particular perturbation. Current tests of the no-hair theorem, attempt to identify these modes in a semi-agnostic way, without imposing priors on the source of the perturbation. This is usually known as \textit{black-hole spectroscopy}. Applying this framework to GW150914, the measurement of the first overtone led to the confirmation of the theorem to $20\%$ level. We show, however, that such semi-agnostic tests cannot provide strong evidence in favour of the no-hair theorem, even for extremely loud signals, given the increasing number of overtones (and free parameters) needed to fit the data. This can be solved by imposing prior assumptions on the origin of the perturbed black hole that can further constrain the explored parameters: in particular, our knowledge that the ringdown is sourced by a binary black hole merger. Applying this strategy to GW150914 we find a natural log Bayes factor of $\sim 6.5$ in favour of the Kerr nature of its remnant, indicating that the hairy object hypothesis is disfavoured with $, 12 pages, 4 figures, Version Accepted for publication in Phys.Rev.D
Published: 2020

6. Numerical relativity injection analysis of signals from generically spinning intermediate mass black hole binaries in Advanced LIGO data

Author: K. Chandra, Archana Pai, V. Gayathri, and Juan Calderón Bustillo
Subjects: Physics, Orbital plane, Spins, 010308 nuclear & particles physics, Gravitational wave, Astrophysics::High Energy Astrophysical Phenomena, Astrophysics, 01 natural sciences, LIGO, Black hole, General Relativity and Quantum Cosmology, Numerical relativity, Binary black hole, 0103 physical sciences, 010306 general physics, Spinning
Abstract: The advent of gravitational wave (GW) astronomy has provided us with observations of black holes more massive than those known from X-ray astronomy. However, the observation of an intermediate-mass black hole (IMBH) remains a big challenge. After their second observing run, the LIGO \& Virgo Scientific collaborations (LVC) placed upper limits on the coalescence rate density of non-precessing IMBH binaries (IMBHBs). In this article, we explore the sensitivity of two of the search pipelines used by the LVC to signals from 69 numerically simulated IMBHBs with generic spins, out of which 27 have a precessing orbital plane. In particular, we compare the matched-filter search PyCBC, and the coherent model-independent search technique cWB. We find that, in general, cWB is more sensitive to IMBHBs than PyCBC, with their difference depending on the masses and spins of the source. Consequently, we use cWB to place the first upper limits on the merger rate of generically spinning IMBH binaries using publicly available data from the first Advanced LIGO observing run.
Published: 2020
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7. Measuring Spin of the Remnant Black Hole from Maximum Amplitude

Author: Deirdre Shoemaker, D. L. Ferguson, Pablo Laguna, James A. Clark, S. Ghonge, and Juan Calderón Bustillo
Subjects: Physics, Cosmology and Nongalactic Astrophysics (astro-ph.CO), Gravitational wave, Astrophysics::High Energy Astrophysical Phenomena, General Physics and Astronomy, FOS: Physical sciences, General Relativity and Quantum Cosmology (gr-qc), Radiation, 01 natural sciences, Instantaneous phase, General Relativity and Quantum Cosmology, Black hole, Amplitude, Quantum electrodynamics, 0103 physical sciences, Chirp, 010306 general physics, Maximum amplitude, Astrophysics - Cosmology and Nongalactic Astrophysics, Spin-½
Abstract: Gravitational waves emitted during the merger of two black holes carry information about the remnant black hole, namely its mass and spin. This information is typically found from the ringdown radiation as the black hole settles to a final state. We find that the remnant black hole spin is already known at the peak amplitude of the gravitational wave strain. Using this knowledge, we present a new method for measuring the final spin that is template independent, using only the chirp mass, the instantaneous frequency of the strain, and its derivative at maximum amplitude, all template independent.
Published: 2019

8. On the properties of the massive binary black hole merger GW170729

Author: Vivien Raymond, Bela Szilagyi, Andrea Taracchini, Gregorio Carullo, Mark Hannam, Juan Calderón Bustillo, Daniel A. Hemberger, Alejandro Bohé, R. Cotesta, Alyssa Garcia, Richard O'Shaughnessy, Lawrence E. Kidder, Manuela Campanelli, Michael Pürrer, Patricia Schmidt, Kevin Barkett, Alessandra Buonanno, Michael Boyle, Sebastian Khan, Pablo Laguna, Geoffrey Lovelace, Margaret Millhouse, Lionel London, Salvatore Vitale, Nousha Afshari, Carl-Johan Haster, Harald P. Pfeiffer, Katerina Chatziioannou, H. Fong, Yosef Zlochower, I. W. Harry, Ian Hinder, Prayush Kumar, Francesco Pannarale, Lijing Shao, Eric B. Flynn, James S. Clark, Deirdre Shoemaker, Matthew Giesler, M. Haney, Carlos O. Lousto, Frank Ohme, Stanislav Babak, S. Ghonge, Saul A. Teukolsky, Mark A. Scheel, Tony Chu, Bhavesh Khamersa, Ken K. Y. Ng, L. K. Nuttall, Tyson Littenberg, James Healy, J. S. Lange, Jonathan Blackman, Karan Jani, S. Ossokine, AstroParticule et Cosmologie (APC (UMR_7164)), 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), Centre National d'Études Spatiales [Toulouse] (CNES), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP), Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), and Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité)
Subjects: gr-qc, ST/L000962/1, FOS: Physical sciences, alternative theories of gravity, Astophysics, General Relativity and Quantum Cosmology (gr-qc), spin, gravitational radiation: direct detection, 01 natural sciences, General Relativity and Quantum Cosmology, Gravitational waves, Binary black hole, Consistency (statistics), 0103 physical sciences, Prior probability, black hole, Waveform, ST/N000633/1, 010306 general physics, 10. No inequality, STFC, Spin-½, High Energy Astrophysical Phenomena (astro-ph.HE), Physics, astro-ph.HE, spin: precession, black holes, 010308 nuclear & particles physics, Gravitational wave, gravitational radiation, RCUK, Mass ratio, binary: compact, effect: higher-order, Computational physics, Black hole, General relativity, black hole: binary, gravitational radiation: emission, [PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc], mass ratio, Astrophysics - High Energy Astrophysical Phenomena, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
Abstract: We present a detailed investigation into the properties of GW170729, the gravitational wave with the most massive and distant source confirmed to date. We employ an extensive set of waveform models, including new improved models that incorporate the effect of higher-order waveform modes which are particularly important for massive systems. We find no indication of spin-precession, but the inclusion of higher-order modes in the models results in an improved estimate for the mass ratio of $(0.3-0.8)$ at the 90\% credible level. Our updated measurement excludes equal masses at that level. We also find that models with higher-order modes lead to the data being more consistent with a smaller effective spin, with the probability that the effective spin is greater than zero being reduced from $99\%$ to $94\%$. The 90\% credible interval for the effective spin parameter is now $(-0.01-0.50)$. Additionally, the recovered signal-to-noise ratio increases by $\sim0.3$ units compared to analyses without higher-order modes. We study the effect of common spin priors on the derived spin and mass measurements, and observe small shifts in the spins, while the masses remain unaffected. We argue that our conclusions are robust against systematic errors in the waveform models. We also compare the above waveform-based analysis which employs compact-binary waveform models to a more flexible wavelet- and chirplet-based analysis. We find consistency between the two, with overlaps of $\sim 0.9$, typical of what is expected from simulations of signals similar to GW170729, confirming that the data are well-described by the existing waveform models. Finally, we study the possibility that the primary component of GW170729 was the remnant of a past merger of two black holes and find this scenario to be indistinguishable from the standard formation scenario., Comment: 14 pages, 8 figures, final published version, samples available at https://git.ligo.org/katerina.chatziioannou/gw170729hm_datarelease
Published: 2019
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9. Potential observations of false deviations from general relativity in gravitational wave signals from binary black holes

Author: P. T.H. Pang, Tjonnie G. F. Li, Yi-Fan Wang, and Juan Calderón Bustillo
Subjects: Physics, Angular momentum, 010308 nuclear & particles physics, Gravitational wave, General relativity, Sigma, Orbital eccentricity, Mass ratio, 01 natural sciences, Theoretical physics, Binary black hole, Tests of general relativity, 0103 physical sciences, 010306 general physics
Abstract: Detections of gravitational waves emitted by binary black holes allow for tests of general relativity in the strong-field regime. In particular, deviations from general relativity can be observed by comparing incoming signals to waveform templates that include parametrized deviations from general relativity. However, it is essential that the general relativity sector of these templates accounts for all predictable physics. Otherwise, missing physics might be mimicked by the ``beyond general relativity'' sector of the templates, leading the analysis to report apparent deviations from general relativity. Current parametrized tests implement templates that omit physical phenomena such as orbital eccentricity and higher-order modes. In this paper, we show how the omission of higher modes can lead to false deviations from general relativity when these effects are strong enough. We study the extent of these deviations as a function of the mass ratio and the orbital orientation. We find that significant false deviations can arise when current tests are performed on signals emitted by asymmetric binaries whose orbital angular momentum is orthogonal to the line of sight. We estimate that the Advanced LIGO-Virgo network operating at its design sensitivity can observe false violations with a significance above $5\ensuremath{\sigma}$ as often as once per year. Similar results are expected for other tests of general relativity that compare the data to waveforms where some physical effects are omitted.
Published: 2018
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10. Tracking black hole kicks from gravitational wave observations

Author: Juan Calderón Bustillo, Deirdre Shoemaker, Pablo Laguna, and James A. Clark
Subjects: Physics, 010308 nuclear & particles physics, Gravitational wave, Astrophysics::High Energy Astrophysical Phenomena, General Physics and Astronomy, FOS: Physical sciences, Astrophysics, General Relativity and Quantum Cosmology (gr-qc), Mass ratio, Characteristic velocity, 01 natural sciences, LIGO, General Relativity and Quantum Cosmology, Gravitation, Black hole, Numerical relativity, Binary black hole, 0103 physical sciences, 010306 general physics
Abstract: Coalescing binary black holes emit anisotropic gravitational radiation. This causes a net emission of linear momentum that produces a gradual acceleration of the source. As a result, the final remnant black hole acquires a characteristic velocity known as recoil velocity or gravitational kick. The symmetries of gravitational wave emission are reflected in the interactions of the gravitational wave modes emitted by the binary. In this work we make use of the rich information encoded in the higher-order modes of the gravitational wave emission to infer the component of the kick along the line-of-sight (or \textit{radial kick}). We do this by performing parameter inference on simulated signals given by numerical relativity waveforms for non-spinning binaries using numerical relativity templates of aligned-spin (non-precessing) binary black holes. We find that for suitable sources, namely those with mass ratio $q\geq 2$ and total mass $M \sim 100M_\odot$, and for modest radial kicks of $120km/s$, the $90\%$ credible intervals of our posterior probability distributions can exclude a zero kick at a signal-to-noise ratio of $15$; using a single Advanced LIGO detector working at its early sensitivity. The measurement of a non-zero radial kick component would provide the first observational signature of net transport of linear momentum by gravitational waves away from their source., 6 pages, 5 figures
Published: 2018

11. Sensitivity of gravitational wave searches to the full signal of intermediate-mass black hole binaries during the first observing run of Advanced LIGO

Author: Francesco Salemi, Juan Calderón Bustillo, Karan Jani, and T. D. Canton
Subjects: Physics, 010308 nuclear & particles physics, Gravitational wave, Astrophysics, Parameter space, 01 natural sciences, LIGO, Black hole, General Relativity and Quantum Cosmology, Binary black hole, Search algorithm, Intermediate-mass black hole, 0103 physical sciences, 010306 general physics, LIGO Scientific Collaboration
Abstract: The sensitivity of gravitational wave searches for binary black holes is estimated via the injection and posterior recovery of simulated gravitational wave signals in the detector data streams. When a search reports no detections, the estimated sensitivity is then used to place upper limits on the coalescence rate of the target source. In order to obtain correct sensitivity and rate estimates, the injected waveforms must be faithful representations of the real signals. Up to date, however, injected waveforms have neglected radiation modes of order higher than the quadrupole, potentially biasing sensitivity and coalescence rate estimates. In particular, higher-order modes are known to have a large impact in the gravitational waves emitted by intermediate-mass black holes binaries. In this work, we evaluate the impact of this approximation in the context of two search algorithms run by the LIGO Scientific Collaboration in their search for intermediate-mass black hole binaries in the O1 LIGO Science Run data: a matched filter--based pipeline and a coherent unmodeled one. To this end, we estimate the sensitivity of both searches to simulated signals for nonspinning binaries including and omitting higher-order modes. We find that omission of higher-order modes leads to biases in the sensitivity estimates which depend on the masses of the binary, the search algorithm, and the required level of significance for detection. In addition, we compare the sensitivity of the two search algorithms across the studied parameter space. We conclude that the most recent LIGO-Virgo upper limits on the rate of coalescence of intermediate-mass black hole binaries are conservative for the case of highly asymmetric binaries. However, the tightest upper limits, placed for nearly equal-mass sources, remain unchanged due to the small contribution of higher modes to the corresponding sources.
Published: 2018
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12. Searching for the full symphony of black hole binary mergers

Author: Juan Calderón Bustillo, Alexander H. Nitz, and I. W. Harry
Subjects: High Energy Astrophysical Phenomena (astro-ph.HE), Physics, astro-ph.HE, Cosmology and Nongalactic Astrophysics (astro-ph.CO), 010308 nuclear & particles physics, Gravitational wave, gr-qc, Mode (statistics), FOS: Physical sciences, Binary number, General Relativity and Quantum Cosmology (gr-qc), Astrophysics, Mass ratio, 01 natural sciences, General Relativity and Quantum Cosmology, Black hole, Gravitation, 0103 physical sciences, Content (measure theory), astro-ph.CO, Sensitivity (control systems), 010306 general physics, Astrophysics - High Energy Astrophysical Phenomena, Algorithm, Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract: Current searches for the gravitational-wave signature of compact binary mergers rely on matched-filtering data from interferometric observatories with sets of modelled gravitational waveforms. These searches currently use model waveforms that do not include the higher-order mode content of the gravitational-wave signal. Higher-order modes are important for many compact binary mergers and their omission reduces the sensitivity to such sources. In this work we explore the sensitivity loss incurred from omitting higher-order modes. We present a new method for searching for compact binary mergers using waveforms that include higher-order mode effects, and evaluate the sensitivity increase that using our new method would allow. We find that, when evaluating sensitivity at a constant rate-of-false alarm, and when including the fact that signal-consistency tests can reject some signals that include higher-order mode content, we observe a sensitivity increase of up to a factor of 2 in volume for high mass ratio, high total-mass systems. For systems with equal mass, or with total mass $\sim 50 M_{\odot}$, we see more modest sensitivity increases, $< 10\%$, which indicates that the existing search is already performing well. Our new search method is also directly applicable in searches for generic compact binaries., 17 pages, 7 figures. Updating to match the published version (published in 2018)
Published: 2018
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13. Erratum: 'First Search for Gravitational Waves from Known Pulsars with Advanced LIGO' (2017, ApJ, 839, 12)

Author: M. Lee, G. Kang, M. Razzano, A. Pal-Singh, V. Kondrashov, A. Nitz, A. Hu, Kazuhiro Agatsuma, Zoheyr Doctor, Karan Jani, F. Frasconi, R. Mittleman, J. De, Nelson Christensen, Gijs Nelemans, William Yam, L. Wallace, A. Królak, R. Frey, R. Williams, Y. Minenkov, M. Turconi, Jolien D. E. Creighton, R. Flaminio, T. Whelan, Adam A. Miller, Soumi De, G. Mendell, J. Trinastic, L. Kuo, E. Capocasa, K. Blackburn, A. Schönbeck, S. Brunett, M. Haney, H. Wittel, S. G. Schwalbe, T. A. Callister, N. Kijbunchoo, K. Holt, Chunglee Kim, V. Sandberg, B. Shapiro, D. Hall, Carsten Kramer, B. Hobbs, V. Dolique, Vincenzo Pierro, R. Kirchhoff, T. Theeg, M. Hu, M. Phelps, B. Day, A. Avila-Alvarez, K. Gill, Walter Winkler, Harald Lück, B. U. Gadre, Sebastien Biscans, J. Prasad, Reinhard Prix, J. Li, B. Eggenstein, Paul D. Lasky, Q. Chu, Jade Powell, A. Bisht, Marco Bazzan, H. Qi, M. Branchesi, Zefeng Zhou, S. Ma, M. Ast, O. E. S. Sauter, J. Woehler, M. Prijatelj, M. Cho, G. Gaur, A. Clark, B. Coughlin, Thanh Phuong Nguyen, S. Hu, R. L. Ward, G. Hemming, Alvaro-Miguel Fernandez Galiana, C. Mcguire, Steven Bloemen, K. Izumi, T. M. C. Abbott, L. Pinard, Odylio D. Aguiar, Matthew Pitkin, N. Ma, C. Baune, D. Ugolini, J. Eichholz, L. Schaaf, B. L. Pearlstone, Michael Thomas, Sanjeev Dhurandhar, V. Fafone, M. Bader, N. A. Lockerbie, J. Lang, C. C. Buchanan, László Gondán, P. Pfeiffer, S. Kim, A. Cumming, Federico Ferrini, G. Vajente, G. P. Newton, A. Bohe, M. Fyffe, E. Goetz, S. Penn, M. Lormand, M. C. Heintze, Blake Moore, Carlos O. Lousto, B. Braginsky, M. Wade, Kendall Ackley, M. Granata, F. Garufi, Gabriela Gonzalez, V. Dattilo, F. Carbognani, A. Bilenko, Minchuan Zhou, P. Popolizio, Koji Arai, M. Shoemaker, Tejinder Kaur, T. De, Stefan Hild, Y. Ma, A. Brillet, J. Schmidt, J. Ma, M. Vardaro, F. Robinet, P. Fulda, F. Baldaccini, J. Cho, S. Chu, T. Zhang, M. Wei, L. Stuver, B. Kanner, S. G. Crowder, B. Li, P. Ajith, D. Passuello, Andrew Lyne, R. Passaquieti, S. Ascenzi, J. Daw, J. King, M. Factourovich, T. Hardwick, D. Steinmeyer, Fabrizio Barone, Alessandro Bertolini, F. Travasso, A. Viceré, Michał Bejger, E. Katsavounidis, Yi Chen, S. E. Barclay, K. S. Karvinen, Ofek Birnholtz, J. Betzwieser, M. C. Araya, Antoine Heidmann, R. Corbitt, E. Rhoades, Thibaut Jacqmin, Lucas Guillemot, C. Messenger, M. J. Hart, A. Quintero, A. Chiummo, C. Lazzaro, Patricia Schmidt, V. Brisson, H. Radkins, Mairi Sakellariadou, C. De, J. Warner, S. Rabeling, Laleh Sadeghian, G. Gemme, M. Drago, Guenakh Mitselmakher, R. Wade, L. Miller, B. A. Boom, A. M. Sergeev, O. V. Palashov, F. Piergiovanni, K. Gustafson, R. Wei, Surabhi Sachdev, Christopher J. Moore, M. Scott, Michael L. Gorodetsky, Ryan Lynch, C. I. Torrie, S. Wu, N. Straniero, F. Ricci, V. Gayathri, V. V. Frolov, M. Poe, L. Ma, J. Lehmann, T. D. Creighton, Badri Krishnan, Chang-Hwan Lee, S. Leavey, G. Pillant, R. Morriss, F. Brand, M. C. Edwards, H. Heitmann, I. Ma, N. Leroy, M. Kasprzack, J. Howell, C. Affeldt, E. Schreiber, G. McIntyre, J. Bulten, Debnandini Mukherjee, Luciano Di Fiore, C. Whittle, A. Sawadsky, E. Chassande-Mottin, Douglas Davis, H. Fair, Andrea Taracchini, D. Bersanetti, S. Mirshekari, D. Töyrä, H. Overmier, Juan Antonio Aguilar Sanchez, J. E. Broida, D. Sellers, J. Meidam, Alessandro Corongiu, Riccardo Sturani, R. Ingram, B. Ma, C. Driggers, D. Hoak, Samuele Cortese, Yu Wang, J. Oram, M. Sintes, Piotr Jaranowski, B. Kozak, B. K. Berger, Fabien Kéfélian, J. H. Hough, L. Willis, P. Kumar, Michele Zanolin, Sheila Rowan, D. Sentenac, A. Bozzi, K. Ma, Roman Schnabel, J. E. Brau, T. Vo, R. Bonnand, K. E. Gushwa, F. Costa, M. Pürrer, Andrew Melatos, M. Lorenzini, S. Cho, F. Oh, O. Lebigot, Luca Gammaitoni, D. Hu, B. R. Hall, L. Re, Tenglin Li, M. Guidi, I. Kowalska, T. Sadecki, D. Fiorucci, G. Kuehn, W. Z. Korth, L. Rolland, N. Indik, M. Mohan, B. Kelley, K. A. Strain, K. Haughian, J. Re, S. Vinciguerra, John D. Scott, W. Pratt, S. Grunewald, C. Batch, Catherine M. McGrath, R. Taylor, R. Brady, Jon M. Miller, G. Billingsley, B. B. Miller, S. Doravari, B. Adya, A. K. Lenon, N. Isa, V. Kalogera, L. Urban, D. De, G. D. Hammond, Eric Thrane, P. Lundgren, G. Ballardin, A. Houston, C. Michel, Alena Ananyeva, R. A. Mercer, Todd Adams, O. J. Piccinni, P. J. Veitch, L. Aiello, N. Letendre, M. Gosselin, A. Gennai, Rahul Kumar, B. Lantz, Sarah Caudill, M. Rakhmanov, M. Davier, Rana X. Adhikari, A. Sheperd, T. Hart, R. Gair, F. Donovan, M. J. Yap, C. Palomba, S. Privitera, M. S. Shahriar, Christopher M. Biwer, A. Possenti, Roger Smith, F. Brooks, P. Vyatchanin, Alberto Vecchio, R. Quitzow-James, R. Day, Zhihui Du, A. Prodi, C. Buy, S. Frasca, M. Constancio, Duncan A. Brown, John Worden, M. Oliver, P. Ast, P. Couvares, Hartmut Grote, Tobias Westphal, C. Casentini, Sebastian Khan, L. Prokhorov, B. D. Cheeseboro, G. Cerretani, Anna-Maria A. van Veggel, M. Rizzo, V. Predoi, David E. McClelland, E. E. Cowan, T. Re, B. Klein, James Healy, B. F. Whiting, H. Fong, G. Greco, Howard Pan, Aaron Buikema, A. Mytidis, R. Kennedy, Geoffrey Lovelace, P. Brockill, S. S. Eikenberry, C. C. Wipf, C. Ferreira, E. Cesarini, A. Shaddock, C. Aulbert, Laura Cadonati, Yanxi Zhang, L. Kleybolte, R. Roma, A. Moggi, J. Ming, A. Noack, L. J. Milano, V. Heijningen, B. C. Barish, M. Tonelli, G. Losurdo, R. Metzdorff, L. Conti, R. Abernathy, Christian Beer, C. Green, D. Talukder, M. Leonardi, P. Schale, Swatantra Kumar Tiwari, M. Montani, J. Zhu, R. L. Savage, A. S. Bell, M. Laxen, Rosa Poggiani, V. Frey, David A. Williams, David Jones, A. Perreca, J. Ju, M. J. Cowart, W. De, A. Pele, T. Baker, P. Weßels, G. Stratta, S. Buchner, Jesper Munch, Jan Harms, A. S. Sengupta, Nancy Aggarwal, Marco Cavaglia, Dániel Barta, Ben Farr, B. Mours, Benjamin William Allen, Christophe Collette, H. Cao, C. J. Perez, J. Ottaway, R. Robie, Marc Favata, Sung-Po Chao, T. Isogai, Carl Blair, Abhirup Ghosh, S. S. Forsyth, J. Vine, Karsten Danzmann, Y. Levin, Zahoor Ali Khan, Archana Pai, T. Etzel, R. M. S. Schofield, L. Naticchioni, Salvatore Vitale, Chunglee Chu, B. Sassolas, F. Y. Khalili, Daniele Trifirò, Chad Hanna, D. Buskulic, P. Raffai, Achamveedu Gopakumar, S. Kandhasamy, M. Koehlenbeck, J. Oberling, A. Wei, M. C. Tringali, I. Nardecchia, C. Vo, J. Hanks, C. S. Unnikrishnan, Viswanath Bavigadda, G. Cagnoli, Hua Wang, B. Tanner, M. Punturo, P. Murray, Robert J. McCarthy, Roger Jones, V. J. Roma, F. Paoletti, F. Clara, W. S. Kim, P. Ruggi, A. Allocca, Linqing Wen, N. Gehrels, Slawomir Gras, Fiodor Sorrentino, R. Gouaty, A. Usman, A. Ma, A. Giaime, R. Leong, Benjamin J. Owen, S. Fair, M. Nery, S. Mitra, A. Basti, Ryan N. Lang, K. Chu, M. Ma, Ryan Shannon, Z. Tornasi, A. Mullavey, T. J. N. Nelson, Matthew Kerr, J. Page, C. Messick, T. Ma, B. Hu, M. Tacca, A. W. Heptonstall, Vivien Raymond, Neil J. Cornish, W. Ma, M. Sampson, E. Schmidt, Martin Hendry, M. C. Díaz, Aniello Grado, K. V. Tokmakov, F. Nocera, Robert Lanza, H. Yam, C. Zhao, Michael E Zucker, Marek Szczepanczyk, C. Bradaschia, P. Oppermann, A. Li, C. Tomlinson, J. D. Lough, Soma Mukherjee, Imre Bartos, N. Bakel, B. D. Lackey, A. K. Zadrożny, M. Isa, M. Meyers, K. Kawabe, R. Cavalier, R. Mohapatra, S. Kaufer, Michael W. Coughlin, P. Singer, I. Khan, M. Was, Antonios Kontos, F. Cleva, M. Pichot, K. Venkateswara, M. Du, S. Re, P. Zendri, E. Cuoco, B. Camp, A. Gupta, V. Quetschke, Bangalore Suryanarayana Sathyaprakash, M. Fays, R. Abbott, M. Saleem, Peter Aufmuth, R. Sanders, S. J. Chamberlin, E. Ma, Maximiliano Isi, M. Vasúth, Z. Frei, Martin M. Fejer, R. Bork, Junwei Cao, Eugeniy E. Mikhailov, D. Schuette, J. C. Diaz, Xiaohui Fan, S. Heng, A. Post, Richard O'Shaughnessy, B. Barr, Peter Fritschel, G. Vedovato, Terry G. McRae, S. Meshkov, Jonathan Cripe, K. G. Arun, S. Márka, I. Dave, L. E. Wade, P. Thomas, A. Singer, H. Gabbard, V. De, R. W. P. Drever, M. Fletcher, S. Ghosh, Kipp Cannon, M. Steinke, V. Sequino, S. Caride, W. Harry, Juan Calderón Bustillo, Robert Stone, M. Coward, Kevin M. Ryan, Sibilla Di Pace, P. Bacon, J.-D. Fournier, Daniel E. Holz, Graham Woan, Robert Fisher, W. W. Johnson, M. Korobko, László Á. Gergely, D. Meacher, A. Rüdiger, M. Farr, A. Frei, P. A. Altin, Robert L. Byer, B. J. J. Slagmolen, G. Valdes, A. Samajdar, C. C. Yancey, R. Palamos, D. Barker, G. Blair, Philip F. Hopkins, C. Vander-Hyde, Fausto Acernese, M. Papa, Paul J. Groot, M. Zevin, L. Zangrando, R. Saulson, T. Prestegard, Jacob Scheuer, B. Patricelli, Margaret Millhouse, W. G. Anderson, G. Cella, A. Glaefke, B. Covas, S. Oh, M. De, Mi Zhang, C. Gray, G. H. Ogin, Enrico Calloni, John Veitch, G. Traylor, H. Yu, V. Re, Giacomo Ciani, R. A. Eisenstein, M. Pinto, L. Salconi, I. Fiori, S. G. Gaonkar, A. P. Singh, Haixing Miao, V. Vo, Benjamin Stappers, G. D. Meadors, Bernard F. Schutz, B. P. Abbott, M. Mow-Lowry, G. Bogaert, Li Ju, Alberto Di Lieto, M. Harry, N. Arnaud, T. Hu, T. J. Shaffer, R. N. Singh, S. Vass, Vijay Varma, Riccardo Bassiri, L. Wright, P. Rapagnani, Archisman Ghosh, K. L. Dooley, C. V. Kalaghatgi, J. Hanson, R. Coyne, K. Napier, T. Tippens, M. Castro, J. McIver, C. Raja, P. J. King, H. Vahlbruch, K. Riles, Lisa Barsotti, C. Pan, Anirban Dasgupta, R. J. G. Jonker, Guido Mueller, B. C. Stephens, Larne Pekowsky, L. Lombardi, H. Middleton, M. Kim, V. Tiwari, P. Mitrofanov, P. Puppo, Aaron Viets, M. Perri, M. H. Wimmer, F. Fidecaro, A. Effler, P. Weltevrede, G. Venugopalan, Meng Wang, Tristan Briant, L. Sun, V. Ma, S. Appert, A. Giazotto, G. De, J. Qi, L. Danilishin, Swetha Bhagwat, R. Paris, X. Guo, K. Siellez, Evan Ochsner, S. E. Gossan, L. Merilh, H. Fehrmann, R. Goetz, K. A. Thorne, S. Koley, T. Countryman, D. Moraru, F. Mezzani, J. Fauchon-Jones, P. Shawhan, I. Ferrante, V. Boschi, B. Cepeda, M. Gupta, D. Pascucci, Jimin George, M. Sieniawska, M. Landry, Gregory Ashton, Tarun Souradeep, Christopher P. L. Berry, A. D. Silva, M. Fries, P. Hello, Bala R. Iyer, S. McCormick, P. Spencer, G. Wang, B. O'Reilly, P. Charlton, Kejia Lee, A. Muir, Eric Oelker, M. Barsuglia, S. Qi, A. Grant, A. Staley, T. Mcwilliams, H. Vo, L. Zhang, F. Pan, A. Brown, F. Vetrano, Arunava Arun, Chandra Kant Mishra, R. Bhandare, S. Jawahar, S. Farinon, D. Re, Irene Di Palma, C. Barayoga, S. E. Dwyer, David Keitel, A. Paoli, M. Gaebel, C. Costa, S. J. Cooper, Matthew Evans, A. Lartaux-Vollard, Suvadeep Bose, S. Davies, O. Bock, Z. Márka, M. Merzougui, B. Anderson, Haocun Yu, R. Inta, S. Klimenko, T. Girolamo, I. Belahcene, D. Tuyenbayev, X. Siemens, P. Coulon, L. Sammut, A. Rocchi, C. Cocchieri, R. Birney, M. Muniz, E. Genin, V. Loriette, S. Areeda, Francesco Salemi, David H. Shoemaker, S. Karki, T. J. Cullen, D. Verkindt, B. Edo, S. Kissel, M. Belgin, Maria Ilaria Del Principe, M. Agathos, S. D'Antonio, V. Kringel, R. Tso, Patrick M. Koch, Tomasz Bulik, W. Vo, M. Brown, François Bondu, D. Rosińska, C. Coyne, I. Dorrington, R. Pedurand, Benno Willke, C. Cahillane, J. Hennig, A. Khazanov, S. Walsh, Miriam Cabero, Alessandra Buonanno, C.-J. Haster, Collin D. Capano, J. Bartlett, S. Babak, P. Leaci, A. Colla, P. Stevenson, D. Nolting, O. Puncken, P. J. Sutton, G. Thomas, J. H. Romie, R. Douglas, S. Ghonge, F. J. Raab, N. Mukund, L. R. Cominsky, R. Gustafson, G. Wu, S. Raja, S. E. Strigin, J. Zweizig, L. C. Baiardi, Sebastian Steinlechner, D. Mendoza-Gandara, Jessica Steinlechner, A. Neunzert, T. Chmiel, M. Heurs, H. Re, V. Germain, Sylvia J. Zhu, K. Nuttall, Reed Essick, R. Everett, Krishna M. Srivastava, B. Sorazu, A. Kutynia, Alessandro Ridolfi, Andrea Chincarini, T. Z. Summerscales, W. Katzman, M. Neri, R. Billman, M. Yvert, Martin van Beuzekom, C. Frei, L. Trozzo, P. Ehrens, Albert Lazzarini, M. Giovanni, M. Newport, Samaya Nissanke, M. A. Bizouard, J. J. Hacker, A. Pace, Ismaël Cognard, J. Birch, E. Coccia, C. Graef, B. A. Weaver, J. G. Rollins, L.-W. Wei, P. Chen, N. A. Robertson, William Parker, Márton Tápai, S. Sun, David Jonathan Hofman, M. Bitossi, G. Bergmann, B. Nielsen, J. Henry, Liam Cunningham, B. Pan, Beverly J. Smith, K. Wette, John J. Oh, Timothy Evans, Jonathan Blackman, M. Brinkmann, K. Toland, C. Adams, R. M. Blair, D. Sigg, S. W. Ballmer, M. E. N. Normandin, Michelle E. Walker, G. Moreno, Y. Setyawati, A. Pasqualetti, M. M. Hanke, M. Tse, B. L. Swinkels, F. Jiménez-Forteza, Zachariah B. Etienne, Jennifer Watchi, J. Son, Yann Bouffanais, R. De, T. P. Downes, M. Pedraza, M. Chan, A. Ain, T. D. Canton, F. Cavalier, M. A. Álvarez, M. Boer, F. Cohadon, Alessandra Corsi, J. E. Lord, Maurizio Canepa, Paolo Addesso, K. D. Giardina, Angela Di Virgilio, T. London, Department of Physics [Toronto], University of Toronto, Laboratoire d'Annecy de Physique des Particules (LAPP), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS), Max-Planck-Institut für Gravitationsphysik ( Albert-Einstein-Institut ) (AEI), Max-Planck-Gesellschaft, Los Alamos National Laboratory (LANL), Laboratoire de l'Accélérateur Linéaire (LAL), Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), AstroParticule et Cosmologie (APC (UMR_7164)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Max Delbrück Center for Molecular Medicine [Berlin] (MDC), Helmholtz-Gemeinschaft = Helmholtz Association, APC - Cosmologie, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Physique Corpusculaire et Cosmologie - Collège de France (PCC), Collège de France (CdF (institution))-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Department of Physics, Columbia University [New York], Dipartimento di Physica E. Firmi, University of Pisa - Università di Pisa, Department of Astrophysics [Nijmegen], Institute for Mathematics, Astrophysics and Particle Physics (IMAPP), Radboud University [Nijmegen]-Radboud University [Nijmegen], LAboratoire de REcherche en Géodésie [Paris] (LAREG), Laboratoire des Sciences et Technologies de l'Information Géographique (LaSTIG), École nationale des sciences géographiques (ENSG), Institut National de l'Information Géographique et Forestière [IGN] (IGN)-Institut National de l'Information Géographique et Forestière [IGN] (IGN)-École nationale des sciences géographiques (ENSG), Institut National de l'Information Géographique et Forestière [IGN] (IGN)-Institut National de l'Information Géographique et Forestière [IGN] (IGN), Observatoire de Haute-Provence (OHP), Institut Pythéas (OSU PYTHEAS), Institut de Recherche pour le Développement (IRD)-Aix Marseille Université (AMU)-Institut national de recherche en sciences et technologies pour l'environnement et l'agriculture (IRSTEA)-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Aix Marseille Université (AMU)-Institut national de recherche en sciences et technologies pour l'environnement et l'agriculture (IRSTEA)-Centre National de la Recherche Scientifique (CNRS), Astrophysique Relativiste Théories Expériences Métrologie Instrumentation Signaux (ARTEMIS), Université Nice Sophia Antipolis (1965 - 2019) (UNS), 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, COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Université Côte d'Azur (UCA)-Université Côte d'Azur (UCA)-Centre National de la Recherche Scientifique (CNRS), Laboratoire des matériaux avancés (LMA), Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Centre de Thermique de Lyon (CETHIL), Université de Lyon-Université de Lyon-Institut National des Sciences Appliquées de Lyon (INSA Lyon), Université de Lyon-Institut National des Sciences Appliquées (INSA)-Institut National des Sciences Appliquées (INSA)-Centre National de la Recherche Scientifique (CNRS), Laboratoire Kastler Brossel (LKB (Jussieu)), Fédération de recherche du Département de physique de l'Ecole Normale Supérieure - ENS Paris (FRDPENS), École normale supérieure - Paris (ENS-PSL), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-École normale supérieure - Paris (ENS-PSL), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Centre National de la Recherche Scientifique (CNRS), Institut Charles Sadron (ICS), Université de Strasbourg (UNISTRA)-Institut de Chimie du CNRS (INC)-Centre National de la Recherche Scientifique (CNRS)-Matériaux et Nanosciences Grand-Est (MNGE), Université de Strasbourg (UNISTRA)-Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA))-Institut National de la Santé et de la Recherche Médicale (INSERM)-Institut de Chimie du CNRS (INC)-Centre National de la Recherche Scientifique (CNRS)-Université de Strasbourg (UNISTRA)-Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA))-Institut National de la Santé et de la Recherche Médicale (INSERM)-Centre National de la Recherche Scientifique (CNRS)-Réseau nanophotonique et optique, Université de Strasbourg (UNISTRA)-Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA))-Centre National de la Recherche Scientifique (CNRS)-Université de Strasbourg (UNISTRA)-Centre National de la Recherche Scientifique (CNRS), APC - THEORIE, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut für theoretische Physik, Universität Hamburg (UHH)-Universität Hamburg (UHH), Physics Department, Amherst U., University of Massachusetts System (UMASS), Biomécanique et Bioingénierie (BMBI), Université de Technologie de Compiègne (UTC)-Centre National de la Recherche Scientifique (CNRS), Grupo de Investigación en Energía y Medioambiente [Bucaramanga]] (GIEMA), Universidad Industrial de Santander [Bucaramanga] (UIS), Chambre Agriculture Gard, Observatoire de la Côte d'Azur (OCA), Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), European Organization for Nuclear Research (CERN), Département de Physique Nucléaire (ex SPhN) (DPHN), Institut de Recherches sur les lois Fondamentales de l'Univers (IRFU), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, Centre de Recherche Saint-Antoine (UMRS893), Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut National de la Santé et de la Recherche Médicale (INSERM), Groupe d'étude des réseaux moteurs - GERM (GERMG), Université de la Méditerranée - Aix-Marseille 2-Centre National de la Recherche Scientifique (CNRS), Edmund Mach Foundation (FEM), Department of Geography, Swansea University, Département de Pharmacologie, sherbrooke, Istituto Nazionale di Fisica Nucleare, Sezione di Genova (INFN, Sezione di Genova), Istituto Nazionale di Fisica Nucleare (INFN), Leibniz Universität Hannover=Leibniz University Hannover, Laboratoire des symbioses tropicales et méditerranéennes (UMR LSTM), Centre de Coopération Internationale en Recherche Agronomique pour le Développement (Cirad)-Université Montpellier 1 (UM1)-Institut de Recherche pour le Développement (IRD)-Institut National de la Recherche Agronomique (INRA)-Université Montpellier 2 - Sciences et Techniques (UM2)-Université de Montpellier (UM)-Institut national d’études supérieures agronomiques de Montpellier (Montpellier SupAgro), Département Systèmes Biologiques (Cirad-BIOS), Centre de Coopération Internationale en Recherche Agronomique pour le Développement (Cirad), Pontifícia Universidade Católica do Rio de Janeiro (PUC-Rio), Department of Entomology, University of Arkansas [Fayetteville], NASA Goddard Space Flight Center (GSFC), Franche-Comté Électronique Mécanique, Thermique et Optique - Sciences et Technologies (UMR 6174) (FEMTO-ST), Université de Technologie de Belfort-Montbeliard (UTBM)-Ecole Nationale Supérieure de Mécanique et des Microtechniques (ENSMM)-Centre National de la Recherche Scientifique (CNRS)-Université de Franche-Comté (UFC), Université Bourgogne Franche-Comté [COMUE] (UBFC)-Université Bourgogne Franche-Comté [COMUE] (UBFC), Hulleras del Norte, S.A., Laboratoire d'Ingénierie des Matériaux de Bretagne (LIMATB), Université de Bretagne Sud (UBS)-Université de Brest (UBO)-Institut Brestois du Numérique et des Mathématiques (IBNM), Université de Brest (UBO)-Université de Brest (UBO), European gravitational Observatory (EGO), Istituto Nazionale di Fisica Nucleare (INFN)-Centre National de la Recherche Scientifique (CNRS), School of Electrical and Computer Engineering - Georgia Insitute of Technology (ECE GeorgiaTech), Georgia Institute of Technology [Atlanta], CNR Institute of Geosciences and Earth Resources (IGG), National Research Council of Italy | Consiglio Nazionale delle Ricerche (CNR), Imagerie Ultrasonore, Centre de Recherche en Acquisition et Traitement de l'Image pour la Santé (CREATIS), Université de Lyon-Institut National des Sciences Appliquées (INSA)-Institut National des Sciences Appliquées (INSA)-Université Jean Monnet - Saint-Étienne (UJM)-Institut National de la Santé et de la Recherche Médicale (INSERM)-Centre National de la Recherche Scientifique (CNRS)-Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Institut National des Sciences Appliquées (INSA)-Institut National des Sciences Appliquées (INSA)-Université Jean Monnet - Saint-Étienne (UJM)-Institut National de la Santé et de la Recherche Médicale (INSERM)-Centre National de la Recherche Scientifique (CNRS), Indian Institute of Technology Delhi (IIT Delhi), Bayerische Julius-Maximilians University, Tata Institute for Fundamental Research (TIFR), Istituto Nazionale di Fisica Nucleare, Sezione di Firenze (INFN, Sezione di Firenze), Évolution, génomes, comportement et écologie (EGCE), Université Paris-Sud - Paris 11 (UP11)-IRD-Centre National de la Recherche Scientifique (CNRS), Institut Européen des membranes (IEM), Ecole Nationale Supérieure de Chimie de Montpellier (ENSCM)-Institut de Chimie du CNRS (INC)-Université de Montpellier (UM)-Centre National de la Recherche Scientifique (CNRS), Commissariat à l'Energie Atomique, Commissariat à l'énergie atomique et aux énergies alternatives (CEA), Max-Planck-Institut für Quantenoptik (MPQ), University of Glasgow, College of Environmental Sciences and Engineering [Peking], Peking University [Beijing], East China Normal University [Shangaï] (ECNU), School of Dentistry and Dental Research Institute [UCLA], University of California [Los Angeles] (UCLA), University of California (UC)-University of California (UC), Laboratoire Kastler Brossel (LKB (Lhomond)), Chinese Academy of Sciences [Beijing] (CAS), University of Minnesota System, Inconnu, Informatics and Telematics Institute/Centre for Research Hellas, Instituto de RadioAstronomía Milimétrica (IRAM), Centre National de la Recherche Scientifique (CNRS), Civil and Environmental Engineering [Illinois] (CEE), University of Illinois at Urbana-Champaign [Urbana], University of Illinois System-University of Illinois System, Laboratoire de psychologie sociale et de psychologie cognitive (LAPSCO), Université Blaise Pascal - Clermont-Ferrand 2 (UBP)-Centre National de la Recherche Scientifique (CNRS), Helmholtz zentrum für Schwerionenforschung GmbH (GSI), Imagerie Moléculaire et Nanobiotechnologies - Institut Européen de Chimie et Biologie (IECB), Université Sciences et Technologies - Bordeaux 1 (UB)-Centre National de la Recherche Scientifique (CNRS), Univ Turin, Dept Chem, Via P Giuria 7, I-10125 Turin, Italy, Jet Propulsion Laboratory (JPL), NASA-California Institute of Technology (CALTECH), ArcelorMittal Maizières Research SA, ArcelorMittal, Dauphine Recherches en Management (DRM), Université Paris Dauphine-PSL, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS), Universidade Federal do Rio Grande do Sul [Porto Alegre] (UFRGS), Tsinghua University [Beijing] (THU), Ecole Superieure de Physique et de Chimie Industrielles de la Ville de Paris (ESPCI Paris), Université Paris sciences et lettres (PSL), Department of Radiation Oncology, Andrew Love Cancer Centre, Institut de Physique Nucléaire d'Orsay (IPNO), Division of Geological and Planetary Sciences [Pasadena], California Institute of Technology (CALTECH), DME (Dept. of Mech. Eng.), Hong Kong University of Science and Technology (HKUST), University of Huddersfield, Institut de biologie et chimie des protéines [Lyon] (IBCP), Université de Lyon-Université de Lyon-Centre National de la Recherche Scientifique (CNRS), Key Laboratory of of Optical Astronomy, University of Delaware [Newark], University of Bath [Bath], Géosciences Environnement Toulouse (GET), Institut de Recherche pour le Développement (IRD)-Université Toulouse III - Paul Sabatier (UT3), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire Midi-Pyrénées (OMP), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Institut de Recherche pour le Développement (IRD)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Centre National de la Recherche Scientifique (CNRS), Rothamsted Research, Biotechnology and Biological Sciences Research Council (BBSRC), Dipartimento di Fisica [Roma La Sapienza], Università degli Studi di Roma 'La Sapienza' = Sapienza University [Rome] (UNIROMA), Friction Stir Laboratory, Brigham Young University (BYU), Institut de recherches sur la catalyse et l'environnement de Lyon (IRCELYON), Université de Lyon-Université de Lyon-Institut de Chimie du CNRS (INC)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de rhéologie (LR), Université Joseph Fourier - Grenoble 1 (UJF)-Institut National Polytechnique de Grenoble (INPG)-Centre National de la Recherche Scientifique (CNRS), Department of Mechanical Engineering, Sogang University, parent, Laboratoire de Mesures et Modélisation de la Migration des Radionucléides (L3MR), Service d'Etudes du Comportement des Radionucléides (SECR), Département de Physico-Chimie (DPC), CEA-Direction des Energies (ex-Direction de l'Energie Nucléaire) (CEA-DES (ex-DEN)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay-CEA-Direction des Energies (ex-Direction de l'Energie Nucléaire) (CEA-DES (ex-DEN)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay-Département de Physico-Chimie (DPC), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, Istituto Nazionale di Fisica Nucleare, Sezione di Catania (INFN), Università degli studi di Catania = University of Catania (Unict), Unité Mixte de Recherche Epidémiologique et de Surveillance Transport Travail Environnement UMRT9002 (UMRESTTE), Université de Lyon-Université de Lyon-Institut National de Recherche sur les Transports et leur Sécurité (INRETS)-Institut de Veille Sanitaire (INVS), Institut d'Electronique du Solide et des Systèmes (InESS), The Istituto dei Materiali per l'Elettronica ed il Magnetismo (IMEN) (IMEN-CNR), Southern University of Science and Technology (SUSTech), Istituto Nazionale di Fisica Nucleare, Sezione di Pisa, Istituto Matematico, Scuola Normale Superiore di Pisa (SNS), SensorDynamics AG, Institut d'Astrophysique de Paris (IAP), Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), ESRL Chemical Sciences Division [Boulder] (CSD), NOAA Earth System Research Laboratory (ESRL), National Oceanic and Atmospheric Administration (NOAA)-National Oceanic and Atmospheric Administration (NOAA), Physics Department, University of Wisconsin at Milwaukee, University of Wisconsin - Milwaukee, Departements of Chemistry and Biochemistry, Seattle University [Seattle], Friedrich-Alexander Universität Erlangen-Nürnberg (FAU), Institute for Plasma Research [Gandhinagar], Zurich Research Laboratory, IBM Research GmbH, Dipartimento di Fisica e Astronomia [Firenze], Università degli Studi di Firenze = University of Florence (UniFI), National Physical Laboratory [Teddington] (NPL), Centre d'étude spatiale des rayonnements (CESR), Université Toulouse III - Paul Sabatier (UT3), Department of Materials Science and Engineering, Cornell University, USA, Cornell University [New York], Banaras Hindu University [Varanasi] (BHU), University of South Carolina [Columbia], The McDonnell Genome Institute (MGI), Washington University in Saint Louis (WUSTL), Laboratoire de Physique des Lasers, Atomes et Molécules - UMR 8523 (PhLAM), Université de Lille-Centre National de la Recherche Scientifique (CNRS), Università della Calabria [Arcavacata di Rende] (Unical), Università degli studi di Torino = University of Turin (UNITO), Techniques pour l'Evaluation et la Modélisation des Actions de la Santé (TIMC-IMAG-ThEMAS), Techniques de l'Ingénierie Médicale et de la Complexité - Informatique, Mathématiques et Applications, Grenoble - UMR 5525 (TIMC-IMAG), Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-VetAgro Sup - Institut national d'enseignement supérieur et de recherche en alimentation, santé animale, sciences agronomiques et de l'environnement (VAS)-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes [2016-2019] (UGA [2016-2019])-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-VetAgro Sup - Institut national d'enseignement supérieur et de recherche en alimentation, santé animale, sciences agronomiques et de l'environnement (VAS)-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes [2016-2019] (UGA [2016-2019]), Key Lab of Computer System and Architecture, Institute of Computing Technology [Beijing] (ICT), National Center for Atmospheric Research [Boulder] (NCAR), Shenzhen University, Centre for Ultrahigh Bandwidth Devices for Optical Systems (CUDOS), Macquarie University, Texas Instruments Dallas, Centre de Recherche en Transplantation et Immunologie (U1064 Inserm - CRTI), Institut National de la Santé et de la Recherche Médicale (INSERM)-Université de Nantes - UFR de Médecine et des Techniques Médicales (UFR MEDECINE), Université de Nantes (UN)-Université de Nantes (UN), Beijing Normal University (BNU), Laboratori Nazionali di Legnaro (LNL), AIR (AIR), Université de Lyon-Université de Lyon-Institut de Chimie du CNRS (INC)-Centre National de la Recherche Scientifique (CNRS)-Université Claude Bernard Lyon 1 (UCBL), National Astronomical Observatories [Beijing] (NAOC), Pathologie et virologie moléculaire (PVM (UMR_7151)), Université Paris Diderot - Paris 7 (UPD7)-Institut National de la Santé et de la Recherche Médicale (INSERM)-Centre National de la Recherche Scientifique (CNRS), SFA Inc/NRL (SFA INC/NRL), SFA Inc/NRL, Laboratoire de Physique et Chimie de l'Environnement et de l'Espace (LPC2E), Observatoire des Sciences de l'Univers en région Centre (OSUC), Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université d'Orléans (UO)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université d'Orléans (UO)-Centre National de la Recherche Scientifique (CNRS)-Centre National d’Études Spatiales [Paris] (CNES), Unité Scientifique de la Station de Nançay (USN), Université Paris sciences et lettres (PSL)-Université d'Orléans (UO)-Centre National de la Recherche Scientifique (CNRS), INAF - Osservatorio Astronomico di Cagliari (OAC), Istituto Nazionale di Astrofisica (INAF), Australian Resources Research Centre (CSIRO), Department of Physics [Seattle], University of Washington [Seattle], Jodrell Bank Centre for Astrophysics, University of Manchester [Manchester], CSIRO Astronomy and Space Science, Commonwealth Scientific and Industrial Research Organisation [Canberra] (CSIRO), Jodrell Bank Centre for Astrophysics (JBCA), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11), 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), 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)-Observatoire de Paris, Radboud university [Nijmegen]-Radboud university [Nijmegen], Aix Marseille Université (AMU)-Centre National de la Recherche Scientifique (CNRS)-Institut national de recherche en sciences et technologies pour l'environnement et l'agriculture (IRSTEA)-Institut de Recherche pour le Développement (IRD)-Aix Marseille Université (AMU)-Centre National de la Recherche Scientifique (CNRS)-Institut national de recherche en sciences et technologies pour l'environnement et l'agriculture (IRSTEA)-Institut de Recherche pour le Développement (IRD), Centre National de la Recherche Scientifique (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)-COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Nice Sophia Antipolis (... - 2019) (UNS), COMUE Université Côte d'Azur (2015-2019) (COMUE UCA), Université Nice Sophia Antipolis (... - 2019) (UNS), 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), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon, Université Pierre et Marie Curie - Paris 6 (UPMC)-Fédération de recherche du Département de physique de l'Ecole Normale Supérieure - ENS Paris (FRDPENS), 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)-École normale supérieure - Paris (ENS Paris), Université de Strasbourg (UNISTRA)-Institut de Chimie du CNRS (INC)-Centre National de la Recherche Scientifique (CNRS)-Réseau nanophotonique et optique, Centre National de la Recherche Scientifique (CNRS)-Université de Strasbourg (UNISTRA)-Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA))-Centre National de la Recherche Scientifique (CNRS)-Université de Strasbourg (UNISTRA)-Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA))-Matériaux et nanosciences d'Alsace (FMNGE), Institut de Chimie du CNRS (INC)-Université de Strasbourg (UNISTRA)-Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA))-Institut National de la Santé et de la Recherche Médicale (INSERM)-Centre National de la Recherche Scientifique (CNRS)-Université de Strasbourg (UNISTRA)-Institut National de la Santé et de la Recherche Médicale (INSERM)-Centre National de la Recherche Scientifique (CNRS), 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)-Institut für theoretische Physik, Leibniz Universität Hannover [Hannover] (LUH), Institut national d'enseignement supérieur pour l'agriculture, l'alimentation et l'environnement (Institut Agro)-Institut national d'enseignement supérieur pour l'agriculture, l'alimentation et l'environnement (Institut Agro), Université de Technologie de Belfort-Montbeliard (UTBM)-Ecole Nationale Supérieure de Mécanique et des Microtechniques (ENSMM)-Université de Franche-Comté (UFC), Université Bourgogne Franche-Comté [COMUE] (UBFC)-Université Bourgogne Franche-Comté [COMUE] (UBFC)-Centre National de la Recherche Scientifique (CNRS), Université de Bretagne Sud (UBS)-Institut Brestois du Numérique et des Mathématiques (IBNM), Université de Brest (UBO)-Université de Brest (UBO)-Université de Brest (UBO), Consiglio Nazionale delle Ricerche (CNR), Université Jean Monnet [Saint-Étienne] (UJM)-Hospices Civils de Lyon (HCL)-Institut National des Sciences Appliquées de Lyon (INSA Lyon), Université de Lyon-Institut National des Sciences Appliquées (INSA)-Université de Lyon-Institut National des Sciences Appliquées (INSA)-Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Centre National de la Recherche Scientifique (CNRS)-Institut National de la Santé et de la Recherche Médicale (INSERM)-Université Jean Monnet [Saint-Étienne] (UJM)-Hospices Civils de Lyon (HCL)-Institut National des Sciences Appliquées de Lyon (INSA Lyon), Université de Lyon-Centre National de la Recherche Scientifique (CNRS)-Institut National de la Santé et de la Recherche Médicale (INSERM), Université Montpellier 2 - Sciences et Techniques (UM2)-Ecole Nationale Supérieure de Chimie de Montpellier (ENSCM)-Institut de Chimie du CNRS (INC)-Université de Montpellier (UM)-Centre National de la Recherche Scientifique (CNRS), University of California-University of California, Centre National de la Recherche Scientifique (CNRS)-Université Blaise Pascal - Clermont-Ferrand 2 (UBP), Université Sciences et Technologies - Bordeaux 1-Centre National de la Recherche Scientifique (CNRS), Chinese Academy of Sciences [Changchun Branch] (CAS)-National Astronomical Observatories of China, Photonics and photonic materials group, Departement of Physics, University of bath, Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Université Toulouse III - Paul Sabatier (UT3), Université Fédérale Toulouse Midi-Pyrénées-Université Fédérale Toulouse Midi-Pyrénées-Observatoire Midi-Pyrénées (OMP), Institut de Recherche pour le Développement (IRD)-Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Université Fédérale Toulouse Midi-Pyrénées-Institut de Recherche pour le Développement (IRD)-Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS), Department of Physics [Roma La Sapienza], Università degli Studi di Roma 'La Sapienza' = Sapienza University [Rome], Centre National de la Recherche Scientifique (CNRS)-Institut National Polytechnique de Grenoble (INPG)-Université Joseph Fourier - Grenoble 1 (UJF), Università degli studi di Catania [Catania], Institut National de Recherche sur les Transports et leur Sécurité (INRETS)-Institut de Veille Sanitaire (INVS)-Université Claude Bernard Lyon 1 (UCBL), Consiglio Nazionale delle Ricerche [Roma] (CNR), Southern University of Science and Technology of China (SUSTech), Scuola Normale Superiore, Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Pierre et Marie Curie - Paris 6 (UPMC), Dipartimento di Fisica and LENS, Università di Firenze-INFN, LENS, INFN, Observatoire Midi-Pyrénées (OMP), Institut de Recherche pour le Développement (IRD)-Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Université Fédérale Toulouse Midi-Pyrénées-Institut de Recherche pour le Développement (IRD)-Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Toulouse III - Paul Sabatier (UT3), Université Fédérale Toulouse Midi-Pyrénées, Università degli studi di Torino (UNITO), Laboratoire Réactions et Génie des Procédés (LRGP), Centre National de la Recherche Scientifique (CNRS)-Université de Lorraine (UL), Centre National de la Recherche Scientifique (CNRS)-Institut National de la Santé et de la Recherche Médicale (INSERM)-Université Paris Diderot - Paris 7 (UPD7), Centre National de la Recherche Scientifique (CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire des Sciences de l'Univers en région Centre (OSUC), Université Paris sciences et lettres (PSL)-Université d'Orléans (UO)-Centre National de la Recherche Scientifique (CNRS)-Université d'Orléans (UO), Laboratoire d'Annecy de Physique des Particules (LAPP/Laboratoire d'Annecy-le-Vieux de Physique des Particules), 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), Max-Delbrück-Center for Molecular Medicine (MDC), Center for Molecular Medicine, Collège de France (CdF)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Collège de France (CdF)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-AstroParticule et Cosmologie (APC (UMR_7164)), PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, Collège de France (CdF)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Université Côte d'Azur (UCA)-Université Côte d'Azur (UCA)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de la Côte d'Azur, Université Côte d'Azur (UCA)-Centre National de la Recherche Scientifique (CNRS), Université de Lyon-Université de Lyon-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Centre National de la Recherche Scientifique (CNRS), Centre National de la Recherche Scientifique (CNRS)-École normale supérieure - Paris (ENS Paris)-Centre National de la Recherche Scientifique (CNRS)-École normale supérieure - Paris (ENS Paris)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Centre National de la Recherche Scientifique (CNRS), Université de Strasbourg (UNISTRA)-Centre National de la Recherche Scientifique (CNRS)-Matériaux et nanosciences d'Alsace, Université de Strasbourg (UNISTRA)-Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA))-Institut National de la Santé et de la Recherche Médicale (INSERM)-Centre National de la Recherche Scientifique (CNRS)-Université de Strasbourg (UNISTRA)-Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA))-Institut National de la Santé et de la Recherche Médicale (INSERM)-Centre National de la Recherche Scientifique (CNRS)-Réseau nanophotonique et optique, Université de Strasbourg (UNISTRA)-Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA))-Centre National de la Recherche Scientifique (CNRS)-Université de Strasbourg (UNISTRA), Laboratoire de Physique Nucléaire et de Hautes Énergies (LPNHE), Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-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 für theoretische Physik, Grupo de Investigación en Energía y Medioambiente (GIEMA), Centre de Recherche Saint-Antoine (CR Saint-Antoine), National Institute for Nuclear Physics (INFN), Université de Franche-Comté (UFC)-Centre National de la Recherche Scientifique (CNRS)-Ecole Nationale Supérieure de Mécanique et des Microtechniques (ENSMM)-Université de Technologie de Belfort-Montbeliard (UTBM), Ecosystèmes forestiers (UR EFNO), Institut national de recherche en sciences et technologies pour l'environnement et l'agriculture (IRSTEA), Tata Institute of Fundamental Research [Bombay] (TIFR), Université de Montpellier (UM)-Université Montpellier 2 - Sciences et Techniques (UM2)-Ecole Nationale Supérieure de Chimie de Montpellier (ENSCM)-Centre National de la Recherche Scientifique (CNRS), University of Minnesota, University of Minnesota [Twin Cities], University of Minnesota System-University of Minnesota System, Civil and Environmental Engineering (CEE), Centre National de la Recherche Scientifique (CNRS)-Université Paris Dauphine-PSL, Tsinghua University [Beijing], ESPCI ParisTech, Institute of Climate System, Chinese Academy of Meteorological Sciences (CAMS), Centre National de la Recherche Scientifique (CNRS)-Observatoire Midi-Pyrénées (OMP), Université Fédérale Toulouse Midi-Pyrénées-Université Fédérale Toulouse Midi-Pyrénées-Université Toulouse III - Paul Sabatier (UT3), Université Fédérale Toulouse Midi-Pyrénées-Institut de Recherche pour le Développement (IRD)-Centre National d'Études Spatiales [Toulouse] (CNES), Università degli Studi di Roma 'La Sapienza' [Rome], CEA-Direction de l'Energie Nucléaire (CEA-DEN), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay-CEA-Direction de l'Energie Nucléaire (CEA-DEN), Institut de Physique Nucléaire de Lyon (IPNL), University of Wisconsin at Milwaukee, Institute for Plasma Research, MN2S, Université de Franche-Comté (UFC)-Centre National de la Recherche Scientifique (CNRS)-Ecole Nationale Supérieure de Mécanique et des Microtechniques (ENSMM)-Université de Technologie de Belfort-Montbeliard (UTBM)-Université de Franche-Comté (UFC)-Centre National de la Recherche Scientifique (CNRS)-Ecole Nationale Supérieure de Mécanique et des Microtechniques (ENSMM)-Université de Technologie de Belfort-Montbeliard (UTBM), Université Fédérale Toulouse Midi-Pyrénées-Université Fédérale Toulouse Midi-Pyrénées-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire Midi-Pyrénées (OMP), Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS), Cornell University, Washington University in St Louis, Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP)-IMAG-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes (UGA)-Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP)-IMAG-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes (UGA), Laboratoire Matériaux Optiques, Photonique et Systèmes (LMOPS), CentraleSupélec-Université de Lorraine (UL), LAboratoire PLasma et Conversion d'Energie (LAPLACE), Université Fédérale Toulouse Midi-Pyrénées-Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS)-Institut National Polytechnique (Toulouse) (Toulouse INP), Beijing Normal University, Université de Lorraine (UL)-Centre National de la Recherche Scientifique (CNRS), Université de Lyon-Université de Lyon-Centre National de la Recherche Scientifique (CNRS)-Université Claude Bernard Lyon 1 (UCBL), Pathologie et virologie moléculaire (PVM), Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Université d'Orléans (UO)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Université d'Orléans (UO)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Centre National d’Études Spatiales [Paris] (CNES), Université d'Orléans (UO)-Observatoire des Sciences de l'Univers en région Centre (OSUC), PSL Research University (PSL)-PSL Research University (PSL)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, PSL Research University (PSL)-Centre National de la Recherche Scientifique (CNRS), PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Centre National de la Recherche Scientifique (CNRS), Centre National de la Recherche Scientifique (CNRS)-Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Institut National des Sciences Appliquées (INSA)-Institut National des Sciences Appliquées (INSA), PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Institut für theoretische Physik, Institut National de la Santé et de la Recherche Médicale (INSERM)-Université Pierre et Marie Curie - Paris 6 (UPMC), California Institute of Technology (CALTECH)-NASA, Université de Lyon-Université de Lyon-Centre National de la Recherche Scientifique (CNRS)-Institut National des Sciences Appliquées de Lyon (INSA Lyon), Centre National de la Recherche Scientifique (CNRS)-Ecole Nationale Supérieure de Chimie de Montpellier (ENSCM)-Université Montpellier 2 - Sciences et Techniques (UM2)-Institut de Chimie du CNRS (INC)-Université de Montpellier (UM), Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD), Université de Lyon-Université de Lyon-Centre National de la Recherche Scientifique (CNRS)-Institut de Chimie du CNRS (INC), Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Toulouse III - Paul Sabatier (UT3), and Université de Lyon-Université de Lyon-Centre National de la Recherche Scientifique (CNRS)-Institut de Chimie du CNRS (INC)-Université Claude Bernard Lyon 1 (UCBL)
Subjects: Physics, [PHYS]Physics [physics], Gravitational wave, Astronomy, Astronomy and Astrophysics, 01 natural sciences, LIGO, Pulsar, Space and Planetary Science, 0103 physical sciences, 010306 general physics, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], 010303 astronomy & astrophysics, ComputingMilieux_MISCELLANEOUS
Abstract: International audience
Published: 2017
Full Text: View/download PDF

14. Impact of gravitational radiation higher order modes on single aligned-spin gravitational wave searches for binary black holes

Author: Michael Pürrer, Sascha Husa, Juan Calderón Bustillo, and Alicia M. Sintes
Subjects: Physics, Particle physics, 010308 nuclear & particles physics, Gravitational wave, FOS: Physical sciences, Order (ring theory), General Relativity and Quantum Cosmology (gr-qc), Astrophysics, Mass ratio, 01 natural sciences, General Relativity and Quantum Cosmology, LIGO, Numerical relativity, Theory of relativity, Binary black hole, 0103 physical sciences, Content (measure theory), 010306 general physics
Abstract: Current template-based gravitational wave searches for compact binary coalescences (CBC) use waveform models that neglect the higher order modes content of the gravitational radiation emitted, considering only the quadrupolar $(\ell,|m|)=(2,2)$ modes. We study the effect of such a neglection for the case of aligned-spin CBC searches for equal-spin (and non-spinning) binary black holes in the context of two versions of Advanced LIGO: the upcoming 2015 version, known as early Advanced LIGO (eaLIGO) and its Zero-Detuned High Energy Power version, that we will refer to as Advanced LIGO (AdvLIGO). In addition, we study the case of a non-spinning search for initial LIGO (iLIGO). We do this via computing the effectualness of the aligned-spin SEOBNRv1 ROM waveform family, which only considers quadrupolar modes, towards hybrid post-Newtonian/Numerical Relativity waveforms which contain higher order modes. We find that for all LIGO versions, losses of more than $10\%$ of events occur for mass ratio $q\geq6$ and $M \geq 100M_\odot$ due to the neglection of higher modes. Moreover, for iLIGO and eaLIGO, losses notably increase up to $(39,23)\%$ respectively for the highest mass $(220M_\odot)$ and mass ratio ($q=8$) studied. For the case of early AdvLIGO, losses of $10\%$ occur for $M>50M_\odot$ and $q\geq6$. Neglection of higher modes leads to observation-averaged systematic parameter biases towards lower spin, total mass and chirp mass. For completeness, we perform a preliminar, non-exhaustive comparison of systematic biases to statistical errors. We find that, for a given SNR, systematic biases dominate over statistical errors at much lower total mass for eaLIGO than for AdvLIGO., 11 pages, 10 figures
Published: 2016
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15. Detectability of gravitational waves from binary black holes: Impact of precession and higher modes

Author: Pablo Laguna, Deirdre Shoemaker, and Juan Calderón Bustillo
Subjects: Physics, 010308 nuclear & particles physics, Gravitational wave, FOS: Physical sciences, Astrophysics, General Relativity and Quantum Cosmology (gr-qc), Mass ratio, 01 natural sciences, LIGO, General Relativity and Quantum Cosmology, Numerical relativity, Theory of relativity, Binary black hole, Quantum mechanics, 0103 physical sciences, Precession, Sensitivity (control systems), 010306 general physics
Abstract: Gravitational wave templates used in current searches for binary black holes omit the effects of precession of the orbital plane and higher order modes. While this omission seems not to impact the detection of sources having mass ratios and spins similar to those of GW150914, even for total masses $M > 200M_{\odot}$; we show that it can cause large fractional losses of sensitive volume for binaries with mass ratio $q \geq 4$ and $M>100M_{\odot}$, measured the detector frame. For the highest precessing cases, this is true even when the source is face-on to the detector. Quantitatively, we show that the aforementioned omission can lead to fractional losses of sensitive volume of $\sim15\%$, reaching $>25\%$ for the worst cases studied. Loss estimates are obtained by evaluating the effectualness of the SEOBNRv2-ROM double spin model, currently used in binary black hole searches, towards gravitational wave signals from precessing binaries computed by means of numerical relativity. We conclude that, for sources with $q \geq 4$, a reliable search for binary black holes heavier than $M>100M_\odot$ needs to consider the effects of higher order modes and precession. The latter seems specially necessary when Advanced LIGO reaches its design sensitivity., 10 pages, 4 Figures
Published: 2016
Full Text: View/download PDF

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15 results on '"Juan Calderón Bustillo"'

1. Post-merger chirps from binary black holes as probes of the final black-hole horizon

2. Confusing Head-On Collisions with Precessing Intermediate-Mass Binary Black Hole Mergers

3. GW190521 as a Merger of Proca Stars: A Potential New Vector Boson of 8.7×10−13 eV

4. Addendum to 'Numerical relativity injection analysis of signals from generically spinning intermediate mass black hole binaries in Advanced LIGO data'

5. Black-hole spectroscopy, the no-hair theorem and GW150914: Kerr vs. Occam

6. Numerical relativity injection analysis of signals from generically spinning intermediate mass black hole binaries in Advanced LIGO data

7. Measuring Spin of the Remnant Black Hole from Maximum Amplitude

8. On the properties of the massive binary black hole merger GW170729

9. Potential observations of false deviations from general relativity in gravitational wave signals from binary black holes

10. Tracking black hole kicks from gravitational wave observations

11. Sensitivity of gravitational wave searches to the full signal of intermediate-mass black hole binaries during the first observing run of Advanced LIGO

12. Searching for the full symphony of black hole binary mergers

13. Erratum: 'First Search for Gravitational Waves from Known Pulsars with Advanced LIGO' (2017, ApJ, 839, 12)

14. Impact of gravitational radiation higher order modes on single aligned-spin gravitational wave searches for binary black holes

15. Detectability of gravitational waves from binary black holes: Impact of precession and higher modes

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15 results on '"Juan Calderón Bustillo"'

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