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_citations.md

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## Citation Summary
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- **Total ADS citations**: 9883
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- **Total INSPIRE citations**: 10852
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- **Total MAX citations**: 10928
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- **Total ADS citations**: 9892
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- **Total INSPIRE citations**: 10849
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- **Total MAX citations**: 10924
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- **h-index**: 48
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## Paper list sorted by citation count
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| # | Author | Year | Title | ADS | INSPIRE | MAX |
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|---|--------|------|-------|-----|---------|-----|
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| **1** | Berti | 2015 | Testing general relativity with present and future astrophysical observations | 1420 | 1612 | 1612 |
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| **2** | Barack | 2019 | Black holes, gravitational waves and fundamental physics: a roadmap | 850 | 945 | 945 |
14-
| **3** | Amaro-Seoane | 2022 | Astrophysics with the Laser Interferometer Space Antenna | 761 | 713 | 761 |
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| **1** | Berti | 2015 | Testing general relativity with present and future astrophysical observations | 1422 | 1612 | 1612 |
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| **2** | Barack | 2019 | Black holes, gravitational waves and fundamental physics: a roadmap | 851 | 945 | 945 |
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| **3** | Amaro-Seoane | 2022 | Astrophysics with the Laser Interferometer Space Antenna | 760 | 713 | 760 |
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| **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 | 479 | 479 |
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| **5** | Varma | 2019 | Surrogate models for precessing binary black hole simulations with unequal masses | 438 | 459 | 459 |
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| **6** | Barausse | 2020 | Prospects for fundamental physics with LISA | 398 | 456 | 456 |
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| **7** | Arun | 2022 | New horizons for fundamental physics with LISA | 311 | 367 | 367 |
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| **8** | Gerosa | 2017 | Are merging black holes born from stellar collapse or previous mergers? | 336 | 364 | 364 |
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| **5** | Varma | 2019 | Surrogate models for precessing binary black hole simulations with unequal masses | 437 | 460 | 460 |
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| **6** | Barausse | 2020 | Prospects for fundamental physics with LISA | 401 | 456 | 456 |
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| **7** | Arun | 2022 | New horizons for fundamental physics with LISA | 313 | 367 | 367 |
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| **8** | Gerosa | 2017 | Are merging black holes born from stellar collapse or previous mergers? | 337 | 364 | 364 |
2020
| **9** | Gerosa | 2021 | Hierarchical mergers of stellar-mass black holes and their gravitational-wave signatures | 272 | 295 | 295 |
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| **10** | Gerosa | 2018 | Spin orientations of merging black holes formed from the evolution of stellar binaries | 221 | 244 | 244 |
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| **11** | Afshordi | 2025 | Waveform modelling for the Laser Interferometer Space Antenna | 148 | 182 | 182 |
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| **11** | Afshordi | 2025 | Waveform modelling for the Laser Interferometer Space Antenna | 149 | 182 | 182 |
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| **12** | Varma | 2019 | High-accuracy mass, spin, and recoil predictions of generic black-hole merger remnants | 144 | 164 | 164 |
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| **13** | Gerosa | 2015 | Multi-timescale analysis of phase transitions in precessing black-hole binaries | 138 | 163 | 163 |
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| **14** | Gerosa | 2013 | Resonant-plane locking and spin alignment in stellar-mass black-hole binaries: a diagnostic of compact-binary formation | 145 | 161 | 161 |
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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 | Escape speed of stellar clusters from multiple-generation black-hole mergers in the upper mass gap | 112 | 121 | 121 |
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| **21** | Gerosa | 2019 | Multiband gravitational-wave event rates and stellar physics | 111 | 121 | 121 |
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| **22** | Wysocki | 2018 | Explaining LIGO's observations via isolated binary evolution with natal kicks | 98 | 105 | 105 |
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| **22** | Wysocki | 2018 | Explaining LIGO's observations via isolated binary evolution with natal kicks | 98 | 104 | 104 |
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| **23** | Gerosa | 2016 | PRECESSION: Dynamics of spinning black-hole binaries with python | 93 | 104 | 104 |
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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** | Romero-Shaw | 2023 | Eccentricity or spin precession? Distinguishing subdominant effects in gravitational-wave data | 85 | 101 | 101 |
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| **25** | Romero-Shaw | 2023 | Eccentricity or spin precession? Distinguishing subdominant effects in gravitational-wave data | 85 | 100 | 100 |
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| **26** | Moore | 2019 | Are stellar-mass black-hole binaries too quiet for LISA? | 88 | 100 | 100 |
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| **27** | Taylor | 2018 | Mining gravitational-wave catalogs to understand binary stellar evolution: a new hierarchical bayesian framework | 93 | 98 | 98 |
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| **28** | Baibhav | 2020 | The mass gap, the spin gap, and the origin of merging binary black holes | 83 | 95 | 95 |
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| **29** | O'Shaughnessy | 2017 | Inferences about supernova physics from gravitational-wave measurements: GW151226 spin misalignment as an indicator of strong black-hole natal kicks | 79 | 88 | 88 |
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| **30** | Gerosa | 2021 | A generalized precession parameter $$\chi_\mathrm{p}$$ to interpret gravitational-wave data | 68 | 81 | 81 |
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| **31** | Bouffanais | 2019 | Constraining the fraction of binary black holes formed in isolation and young star clusters with gravitational-wave data | 77 | 79 | 79 |
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| **32** | Korol | 2020 | Populations of double white dwarfs in Milky Way satellites and their detectability with LISA | 78 | 77 | 78 |
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| **32** | Korol | 2020 | Populations of double white dwarfs in Milky Way satellites and their detectability with LISA | 77 | 77 | 77 |
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| **33** | Horbatsch | 2015 | Tensor-multi-scalar theories: relativistic stars and 3+1 decomposition | 70 | 76 | 76 |
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| **34** | Klein | 2022 | The last three years: multiband gravitational-wave observations of stellar-mass binary black holes | 62 | 70 | 70 |
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| **34** | Klein | 2022 | The last three years: multiband gravitational-wave observations of stellar-mass binary black holes | 63 | 69 | 69 |
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| **35** | Gerosa | 2016 | Black-hole kicks as new gravitational-wave observables | 63 | 68 | 68 |
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| **36** | Gupta | 2020 | Black holes in the low mass gap: Implications for gravitational wave observations | 58 | 64 | 64 |
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| **37** | Buscicchio | 2021 | Bayesian parameter estimation of stellar-mass black-hole binaries with LISA | 55 | 63 | 63 |
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| **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** | Fumagalli | 2023 | Spin-eccentricity interplay in merging binary black holes | 23 | 27 | 27 |
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| **67** | Pacilio | 2024 | Flexible mapping of ringdown amplitudes for nonprecessing binary black holes | 22 | 26 | 26 |
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| **66** | Pacilio | 2024 | Flexible mapping of ringdown amplitudes for nonprecessing binary black holes | 22 | 26 | 26 |
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| **67** | Fumagalli | 2023 | Spin-eccentricity interplay in merging binary black holes | 23 | 26 | 26 |
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| **68** | Moore | 2021 | Population-informed priors in gravitational-wave astronomy | 26 | 26 | 26 |
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| **69** | Rosca-Mead | 2020 | Structure of neutron stars in massive scalar-tensor gravity | 23 | 26 | 26 |
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| **70** | Croon | 2026 | Can GW231123 have a stellar origin? | 25 | 24 | 25 |
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| **120** | Gerosa | 2018 | Reanalysis of LIGO black-hole coalescences with alternative prior assumptions | 2 | 2 | 2 |
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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** | Corelli | 2026 | Variance of gravitational-wave populations | 0 | 0 | 0 |
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| **125** | De Santi | 2026 | Inferring the population properties of galactic binaries from LISA's stochastic foreground | 0 | 0 | 0 |
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| **126** | Borhanian | 2025 | Impact of facility timing and coordination for next-generation gravitational-wave detectors | 0 | 0 | 0 |
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| **127** | Loutrel | 2025 | Probing modified gravitational-wave dispersion with bursts from eccentric black-hole binaries | 0 | 0 | 0 |
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| **128** | 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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| **129** | Boschini | 2025 | “LHS in LHS”: a new expansion strategy for Latin hypercube sampling in simulation design | 0 | 0 | 0 |
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| **123** | Boschini | 2025 | “LHS in LHS”: a new expansion strategy for Latin hypercube sampling in simulation design | 1 | 0 | 1 |
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| **124** | Gerosa | 2015 | Rival families: waveforms from resonant black-hole binaries as probes of their astrophysical formation history | 0 | 1 | 1 |
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| **125** | Corelli | 2026 | Variance of gravitational-wave populations | 0 | 0 | 0 |
137+
| **126** | De Santi | 2026 | Inferring the population properties of galactic binaries from LISA's stochastic foreground | 0 | 0 | 0 |
138+
| **127** | Borhanian | 2025 | Impact of facility timing and coordination for next-generation gravitational-wave detectors | 0 | 0 | 0 |
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| **128** | Loutrel | 2025 | Probing modified gravitational-wave dispersion with bursts from eccentric black-hole binaries | 0 | 0 | 0 |
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| **129** | 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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| **130** | Fumagalli | 2025 | PRECESSION 2.1: black-hole binary spin precession on eccentric orbits | 0 | 0 | 0 |
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| **131** | Gerosa | 2025 | Coincident morphological transitions in precessing black-hole binaries | 0 | 0 | 0 |
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| **132** | Gerosa | 2016 | Source modelling at the dawn of gravitational-wave astronomy | 0 | 0 | 0 |
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_group.md

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_publications.md

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_talks.md

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