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_citations.md

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## Citation Summary
22

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- **Total ADS citations**: 9656
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- **Total INSPIRE citations**: 10726
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- **Total MAX citations**: 10800
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- **Total ADS citations**: 9661
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- **Total INSPIRE citations**: 10727
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- **Total MAX citations**: 10804
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- **h-index**: 48
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## Paper list sorted by citation count
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1111
|---|--------|------|-------|-----|---------|-----|
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| **1** | Berti | 2015 | Testing general relativity with present and future astrophysical observations | 1414 | 1599 | 1599 |
1313
| **2** | Barack | 2019 | Black holes, gravitational waves and fundamental physics: a roadmap | 843 | 937 | 937 |
14-
| **3** | Amaro-Seoane | 2022 | Astrophysics with the Laser Interferometer Space Antenna | 747 | 702 | 747 |
15-
| **4** | Belczynski | 2020 | Evolutionary roads leading to low effective spins, high black hole masses, and O1/O2 rates for LIGO/Virgo binary black holes | 460 | 477 | 477 |
16-
| **5** | Varma | 2019 | Surrogate models for precessing binary black hole simulations with unequal masses | 435 | 453 | 453 |
14+
| **3** | Amaro-Seoane | 2022 | Astrophysics with the Laser Interferometer Space Antenna | 749 | 702 | 749 |
15+
| **4** | Belczynski | 2020 | Evolutionary roads leading to low effective spins, high black hole masses, and O1/O2 rates for LIGO/Virgo binary black holes | 458 | 477 | 477 |
16+
| **5** | Varma | 2019 | Surrogate models for precessing binary black hole simulations with unequal masses | 435 | 454 | 454 |
1717
| **6** | Barausse | 2020 | Prospects for fundamental physics with LISA | 391 | 440 | 440 |
1818
| **7** | Arun | 2022 | New horizons for fundamental physics with LISA | 308 | 360 | 360 |
19-
| **8** | Gerosa | 2017 | Are merging black holes born from stellar collapse or previous mergers? | 334 | 359 | 359 |
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| **8** | Gerosa | 2017 | Are merging black holes born from stellar collapse or previous mergers? | 333 | 359 | 359 |
2020
| **9** | Gerosa | 2021 | Hierarchical mergers of stellar-mass black holes and their gravitational-wave signatures | 270 | 288 | 288 |
2121
| **10** | Gerosa | 2018 | Spin orientations of merging black holes formed from the evolution of stellar binaries | 219 | 240 | 240 |
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| **11** | Afshordi | 2025 | Waveform modelling for the Laser Interferometer Space Antenna | 0 | 177 | 177 |
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| **17** | Kesden | 2015 | Effective potentials and morphological transitions for binary black-hole spin precession | 114 | 138 | 138 |
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| **18** | Ng | 2018 | Gravitational-wave astrophysics with effective-spin measurements: asymmetries and selection biases | 117 | 130 | 130 |
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| **19** | Baibhav | 2019 | Gravitational-wave detection rates for compact binaries formed in isolation: LIGO/Virgo O3 and beyond | 109 | 128 | 128 |
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| **20** | Gerosa | 2019 | Multiband gravitational-wave event rates and stellar physics | 111 | 121 | 121 |
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| **20** | Gerosa | 2019 | Multiband gravitational-wave event rates and stellar physics | 110 | 121 | 121 |
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| **21** | Gerosa | 2019 | Escape speed of stellar clusters from multiple-generation black-hole mergers in the upper mass gap | 110 | 119 | 119 |
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| **22** | Gerosa | 2016 | PRECESSION: Dynamics of spinning black-hole binaries with python | 93 | 103 | 103 |
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| **23** | Wysocki | 2018 | Explaining LIGO's observations via isolated binary evolution with natal kicks | 98 | 102 | 102 |
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| **24** | Vitale | 2017 | Impact of Bayesian priors on the characterization of binary black hole coalescences | 88 | 102 | 102 |
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| **25** | Moore | 2019 | Are stellar-mass black-hole binaries too quiet for LISA? | 89 | 100 | 100 |
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| **25** | Moore | 2019 | Are stellar-mass black-hole binaries too quiet for LISA? | 88 | 100 | 100 |
3737
| **26** | Romero-Shaw | 2023 | Eccentricity or spin precession? Distinguishing subdominant effects in gravitational-wave data | 83 | 98 | 98 |
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| **27** | Taylor | 2018 | Mining gravitational-wave catalogs to understand binary stellar evolution: a new hierarchical bayesian framework | 92 | 98 | 98 |
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| **28** | Baibhav | 2020 | The mass gap, the spin gap, and the origin of merging binary black holes | 81 | 94 | 94 |
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| **55** | Lodato | 2013 | Black hole mergers: do gas discs lead to spin alignment? | 38 | 39 | 39 |
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| **56** | Rosca-Mead | 2020 | Core collapse in massive scalar-tensor gravity | 27 | 34 | 34 |
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| **57** | Gerosa | 2021 | High mass but low spin: an exclusion region to rule out hierarchical black-hole mergers as a mechanism to populate the pair-instability mass gap | 29 | 32 | 32 |
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| **58** | Spadaro | 2023 | Glitch systematics on the observation of massive black-hole binaries with LISA | 27 | 31 | 31 |
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| **58** | Spadaro | 2023 | Glitch systematics on the observation of massive black-hole binaries with LISA | 29 | 31 | 31 |
7070
| **59** | Gerosa | 2023 | Efficient multi-timescale dynamics of precessing black-hole binaries | 28 | 31 | 31 |
7171
| **60** | Sayeb | 2021 | Massive black hole binary inspiral and spin evolution in a cosmological framework | 31 | 29 | 31 |
7272
| **61** | Mould | 2022 | Gravitational-wave population inference at past time infinity | 26 | 30 | 30 |
7373
| **62** | Wong | 2019 | Machine-learning interpolation of population-synthesis simulations to interpret gravitational-wave observations: a case study | 25 | 30 | 30 |
7474
| **63** | Baibhav | 2021 | Looking for the parents of LIGO's black holes | 28 | 29 | 29 |
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| **64** | Chamberlain | 2019 | Frequency-domain waveform approximants capturing Doppler shifts | 27 | 29 | 29 |
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| **65** | Fumagalli | 2024 | Residual eccentricity as a systematic uncertainty on the formation channels of binary black holes | 28 | 27 | 28 |
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| **66** | Pacilio | 2024 | Flexible mapping of ringdown amplitudes for nonprecessing binary black holes | 21 | 26 | 26 |
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| **66** | Pacilio | 2024 | Flexible mapping of ringdown amplitudes for nonprecessing binary black holes | 22 | 26 | 26 |
7878
| **67** | Rosca-Mead | 2020 | Structure of neutron stars in massive scalar-tensor gravity | 23 | 26 | 26 |
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| **68** | Croon | 2024 | Can GW231123 have a stellar origin? | 25 | 23 | 25 |
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| **69** | Fumagalli | 2023 | Spin-eccentricity interplay in merging binary black holes | 23 | 25 | 25 |
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| **70** | Moore | 2021 | Population-informed priors in gravitational-wave astronomy | 25 | 25 | 25 |
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| **71** | Boschini | 2025 | Orbital eccentricity in general relativity from catastrophe theory | 22 | 24 | 24 |
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| **72** | Romero-Shaw | 2025 | GW200208_222617 as an eccentric black-hole binary merger: properties and astrophysical implications | 22 | 23 | 23 |
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| **72** | Romero-Shaw | 2025 | GW200208_222617 as an eccentric black-hole binary merger: properties and astrophysical implications | 23 | 23 | 23 |
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| **73** | Sperhake | 2020 | Amplification of superkicks in black-hole binaries through orbital eccentricity | 23 | 23 | 23 |
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| **74** | Zhao | 2017 | Nutational resonances, transitional precession, and precession-averaged evolution in binary black-hole systems | 21 | 23 | 23 |
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| **75** | Gerosa | 2017 | On the equal-mass limit of precessing black-hole binaries | 19 | 23 | 23 |
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| **80** | Mancarella | 2025 | Sampling the full hierarchical population posterior distribution in gravitational-wave astronomy | 14 | 20 | 20 |
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| **81** | Gangardt | 2021 | A taxonomy of black-hole binary spin precession and nutation | 16 | 20 | 20 |
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| **82** | Varma | 2021 | Up-down instability of binary black holes in numerical relativity | 17 | 19 | 19 |
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| **83** | Nobili | 2025 | Ringdown mode amplitudes of precessing binary black holes | 16 | 18 | 18 |
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| **83** | Nobili | 2025 | Ringdown mode amplitudes of precessing binary black holes | 17 | 18 | 18 |
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| **84** | Buscicchio | 2025 | A test for LISA foreground Gaussianity and stationarity. I. Galactic white-dwarf binaries | 17 | 17 | 17 |
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| **85** | Boschini | 2023 | Extending black-hole remnant surrogate models to extreme mass ratios | 16 | 17 | 17 |
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| **86** | Gerosa | 2020 | The Bardeen-Petterson effect in accreting supermassive black-hole binaries: a systematic approach | 17 | 17 | 17 |
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| **87** | Mould | 2023 | One to many: comparing single gravitational-wave events to astrophysical populations | 14 | 16 | 16 |
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| **88** | Gerosa | 2017 | filltex: Automatic queries to ADS and INSPIRE databases to fill LaTex bibliography | 13 | 16 | 16 |
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| **89** | Gerosa | 2024 | Quick recipes for gravitational-wave selection effects | 13 | 14 | 14 |
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| **90** | Tenorio | 2025 | Scalable data-analysis framework for long-duration gravitational waves from compact binaries using short Fourier transforms | 10 | 13 | 13 |
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| **90** | Tenorio | 2025 | Scalable data-analysis framework for long-duration gravitational waves from compact binaries using short Fourier transforms | 11 | 13 | 13 |
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| **91** | Pacilio | 2024 | Catalog variance of testing general relativity with gravitational-wave data | 9 | 13 | 13 |
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| **92** | Steinle | 2023 | The Bardeen-Petterson effect, disk breaking, and the spin orientations of supermassive black-hole binaries | 10 | 12 | 12 |
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| **93** | Reali | 2020 | Mapping the asymptotic inspiral of precessing binary black holes to their merger remnants | 10 | 12 | 12 |
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| **106** | Gerosa | 2025 | Which is which? Identification of the two compact objects in gravitational-wave binaries | 6 | 7 | 7 |
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| **107** | Kritos | 2024 | Minimum gas mass accreted by spinning intermediate-mass black holes in stellar clusters | 6 | 7 | 7 |
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| **108** | Steinle | 2024 | Probing AGN jet precession with LISA | 6 | 4 | 6 |
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| **109** | Gerosa | 2022 | The irreducible mass and the horizon area of LIGO's black holes | 6 | 5 | 6 |
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| **110** | Dabrowny | 2021 | Modeling the outcome of supernova explosions in binary population synthesis using the stellar compactness | 5 | 6 | 6 |
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| **111** | Varma | 2019 | The binary black hole explorer: on-the-fly visualizations of precessing binary black holes | 4 | 6 | 6 |
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| **112** | Speri | 2026 | Single-harmonic search for extreme mass-ratio inspirals | 4 | 5 | 5 |
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| **113** | Toubiana | 2025 | Comparing astrophysical models to gravitational-wave data in the observable space | 5 | 4 | 5 |
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| **114** | Chiaberge | 2025 | A recoiling supermassive black hole in a powerful quasar | 5 | 5 | 5 |
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| **115** | Boschini | 2024 | Astrophysical and relativistic modeling of the recoiling black-hole candidate in quasar 3C 186 | 5 | 4 | 5 |
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| **109** | Boschini | 2024 | Astrophysical and relativistic modeling of the recoiling black-hole candidate in quasar 3C 186 | 6 | 4 | 6 |
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| **110** | Gerosa | 2022 | The irreducible mass and the horizon area of LIGO's black holes | 6 | 5 | 6 |
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| **111** | Dabrowny | 2021 | Modeling the outcome of supernova explosions in binary population synthesis using the stellar compactness | 5 | 6 | 6 |
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| **112** | Varma | 2019 | The binary black hole explorer: on-the-fly visualizations of precessing binary black holes | 4 | 6 | 6 |
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| **113** | Speri | 2026 | Single-harmonic search for extreme mass-ratio inspirals | 5 | 5 | 5 |
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| **114** | Toubiana | 2025 | Comparing astrophysical models to gravitational-wave data in the observable space | 5 | 4 | 5 |
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| **115** | Chiaberge | 2025 | A recoiling supermassive black hole in a powerful quasar | 5 | 5 | 5 |
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| **116** | Gerosa | 2018 | Surprises from the spins: astrophysics and relativity with detections of spinning black-hole mergers | 4 | 5 | 5 |
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| **117** | Giarda | 2025 | Accelerated inference of binary black-hole populations from the stochastic gravitational-wave background | 2 | 4 | 4 |
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| **118** | Tenorio | 2025 | Where did heavy binaries go? Gravitational-wave populations using Delaunay triangulation with optimized complexity | 3 | 2 | 3 |
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| **121** | Tenorio | 2026 | On the exceptionality of exceptional gravitational-wave events | 1 | 1 | 1 |
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| **122** | Anselmo | 2025 | Black-hole ringdown with templates capturing spin precession: a criticalre-analysis of GW190521 | 1 | 1 | 1 |
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| **123** | Gerosa | 2015 | Rival families: waveforms from resonant black-hole binaries as probes of their astrophysical formation history | 0 | 1 | 1 |
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| **124** | De Santi | 2026 | Inferring the population properties of galactic binaries from LISA'sstochastic foreground | 0 | 0 | 0 |
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| **125** | Borhanian | 2025 | Impact of facility timing and coordination for next-generation gravitational-wave detectors | 0 | 0 | 0 |
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| **126** | Loutrel | 2025 | Probing modified gravitational-wave dispersion with bursts from eccentric black-hole binaries | 0 | 0 | 0 |
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| **127** | Tornotti | 2025 | Bayesian luminosity function estimation in multidepth datasets with selection effects: a case study for $$3<z<5$$ Lyman $$\alpha$$ emitters | 0 | 0 | 0 |
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| **128** | Boschini | 2025 | “LHS in LHS”: a new expansion strategy for Latin hypercube sampling in simulation design | 0 | 0 | 0 |
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| **129** | Fumagalli | 2025 | PRECESSION 2.1: black-hole binary spin precession on eccentric orbits | 0 | 0 | 0 |
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| **130** | Gerosa | 2025 | Coincident morphological transitions in precessing black-hole binaries | 0 | 0 | 0 |
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| **131** | Gerosa | 2016 | Source modelling at the dawn of gravitational-wave astronomy | 0 | 0 | 0 |
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| **132** | Gerosa | 2014 | Spin alignment effects in black hole binaries | 0 | 0 | 0 |
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| **124** | Borhanian | 2025 | Impact of facility timing and coordination for next-generation gravitational-wave detectors | 0 | 0 | 0 |
136+
| **125** | Loutrel | 2025 | Probing modified gravitational-wave dispersion with bursts from eccentric black-hole binaries | 0 | 0 | 0 |
137+
| **126** | Tornotti | 2025 | Bayesian luminosity function estimation in multidepth datasets with selection effects: a case study for $$3<z<5$$ Lyman $$\alpha$$ emitters | 0 | 0 | 0 |
138+
| **127** | Boschini | 2025 | “LHS in LHS”: a new expansion strategy for Latin hypercube sampling in simulation design | 0 | 0 | 0 |
139+
| **128** | Fumagalli | 2025 | PRECESSION 2.1: black-hole binary spin precession on eccentric orbits | 0 | 0 | 0 |
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| **129** | Gerosa | 2025 | Coincident morphological transitions in precessing black-hole binaries | 0 | 0 | 0 |
141+
| **130** | Gerosa | 2016 | Source modelling at the dawn of gravitational-wave astronomy | 0 | 0 | 0 |
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| **131** | Gerosa | 2014 | Spin alignment effects in black hole binaries | 0 | 0 | 0 |
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## Papers per year
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| 2023 | 11 |
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| 2024 | 11 |
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| 2025 | 26 |
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| 2026 | 3 |
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| 2026 | 2 |
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## Papers per journal
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| Physical Review D | 59 |
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| Monthly Notices of the Royal Astronomical Society | 13 |
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| Classical and Quantum Gravity | 11 |
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| arXiv | 10 |
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| arXiv | 9 |
172171
| Physical Review Letters | 9 |
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| Astronomy & Astrophysics | 5 |
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| Astrophysical Journal | 5 |
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| Category | Paper Count |
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|----------|--------------|
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| gr-qc | 71 |
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| astro-ph.HE | 44 |
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| astro-ph.HE | 43 |
200199
| astro-ph.GA | 9 |
201200
| astro-ph.CO | 2 |
202201
| astro-ph.IM | 1 |
203202
| stat.ME | 1 |
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*Last updated: 2026-02-25 01:03:12 UTC*

_group.md

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_publications.md

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## Summary
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**9** [Submitted papers](#submitted-papers)\
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**8** [Submitted papers](#submitted-papers)\
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**108** [Papers published in major peer-reviewed journals](#papers-published-in-major-peer-reviewed-journals)\
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**14** [Other publications (white papers, proceedings, etc.)](#other-publications-white-papers-proceedings-etc)
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## Submitted papers
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**9.**
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*Inferring the population properties of galactic binaries from LISA'sstochastic foreground.*\
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F. De Santi, A. Santini, A. Toubiana, N. Karnesis, **D. Gerosa**.\
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<a href="https://arxiv.org/abs/2602.18560" style="color: inherit; text-decoration: none;">arXiv:2602.18560 [astro-ph.HE]</a>.
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*On the exceptionality of exceptional gravitational-wave events.*\
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R. Tenorio, **D. Gerosa**.\
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_talks.md

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metricspapers.tex

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\cvitem{}{\begin{tabular}{rcl}
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\textcolor{mark_color}{\textbf{Publications}}: &\hspace{0.3cm} &
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\textbf{108} papers published in major peer-reviewed journals,
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\textbf{9} papers in submission stage,
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\textbf{8} papers in submission stage,
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\\ & &
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\textbf{14} other publications (white papers, proceedings, etc.)
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\\ & &

parsepapers.tex

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\cvitem{}{\small\hspace{-1cm}\begin{longtable}{rp{0.3cm}p{15.8cm}}
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%
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\textbf{9.} & & \textit{Inferring the population properties of galactic binaries from LISA'sstochastic foreground.}
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\newline{}
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F. De Santi, A. Santini, A. Toubiana, N. Karnesis, \textbf{D. Gerosa}.
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\newline{}
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\href{https://arxiv.org/abs/2602.18560}{arXiv:2602.18560 [astro-ph.HE].}
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\vspace{0.09cm}\\
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%
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\textbf{8.} & & \textit{On the exceptionality of exceptional gravitational-wave events.}
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\newline{}
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R. Tenorio, \textbf{D. Gerosa}.

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