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‎_citations.md‎

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## Citation Summary
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- **Total ADS citations**: 9656
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- **Total INSPIRE citations**: 10718
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- **Total MAX citations**: 10792
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- **Total INSPIRE citations**: 10726
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- **Total MAX citations**: 10800
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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 | 1414 | 1597 | 1597 |
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| **2** | Barack | 2019 | Black holes, gravitational waves and fundamental physics: a roadmap | 843 | 936 | 936 |
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| **1** | Berti | 2015 | Testing general relativity with present and future astrophysical observations | 1414 | 1599 | 1599 |
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| **2** | Barack | 2019 | Black holes, gravitational waves and fundamental physics: a roadmap | 843 | 937 | 937 |
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| **3** | Amaro-Seoane | 2022 | Astrophysics with the Laser Interferometer Space Antenna | 747 | 702 | 747 |
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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 | 460 | 477 | 477 |
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| **5** | Varma | 2019 | Surrogate models for precessing binary black hole simulations with unequal masses | 435 | 453 | 453 |
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| **8** | Gerosa | 2017 | Are merging black holes born from stellar collapse or previous mergers? | 334 | 359 | 359 |
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| **9** | Gerosa | 2021 | Hierarchical mergers of stellar-mass black holes and their gravitational-wave signatures | 270 | 288 | 288 |
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| **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 | 176 | 176 |
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| **11** | Afshordi | 2025 | Waveform modelling for the Laser Interferometer Space Antenna | 0 | 177 | 177 |
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| **12** | Gerosa | 2015 | Multi-timescale analysis of phase transitions in precessing black-hole binaries | 138 | 163 | 163 |
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| **13** | Varma | 2019 | High-accuracy mass, spin, and recoil predictions of generic black-hole merger remnants | 144 | 162 | 162 |
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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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| **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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| **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 | 97 | 97 |
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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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| **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 | 87 | 87 |
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| **30** | Gerosa | 2021 | A generalized precession parameter $$\chi_\mathrm{p}$$ to interpret gravitational-wave data | 69 | 81 | 81 |
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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** | Sperhake | 2020 | Amplification of superkicks in black-hole binaries through orbital eccentricity | 23 | 23 | 23 |
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| **73** | Zhao | 2017 | Nutational resonances, transitional precession, and precession-averaged evolution in binary black-hole systems | 21 | 23 | 23 |
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| **74** | Gerosa | 2017 | On the equal-mass limit of precessing black-hole binaries | 19 | 23 | 23 |
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| **75** | Romero-Shaw | 2025 | GW200208_222617 as an eccentric black-hole binary merger: properties and astrophysical implications | 22 | 22 | 22 |
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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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| **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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| **76** | Mould | 2020 | Endpoint of the up-down instability in precessing binary black holes | 18 | 22 | 22 |
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| **77** | Gerosa | 2019 | Wide nutation: binary black-hole spins repeatedly oscillating from full alignment to full anti-alignment | 20 | 22 | 22 |
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| **78** | Mancarella | 2023 | Inferring, not just detecting: metrics for high-redshift sources observed with third-generation gravitational-wave detectors | 16 | 21 | 21 |
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| **95** | Mould | 2024 | Calibrating signal-to-noise ratio detection thresholds using gravitational-wave catalogs | 10 | 11 | 11 |
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| **96** | De Renzis | 2022 | Characterization of merging black holes with two precessing spins | 8 | 11 | 11 |
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| **97** | Gangardt | 2022 | Constraining black-hole binary spin precession and nutation with sequential prior conditioning | 10 | 11 | 11 |
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| **98** | Santoliquido | 2024 | Classifying binary black holes from Population III stars with the Einstein Telescope: a machine-learning approach | 10 | 8 | 10 |
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| **99** | Cole | 2025 | Sequential simulation-based inference for extreme mass ratio inspirals | 9 | 9 | 9 |
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| **100** | Fumagalli | 2025 | Non-adiabatic dynamics of eccentric black-hole binaries in post-Newtonian theory | 9 | 9 | 9 |
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| **101** | Fabbri | 2025 | Reconstructing parametric gravitational-wave population fits from non-parametric results without refitting the data | 8 | 9 | 9 |
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| **102** | Stegmann | 2025 | Distinguishing the origin of eccentric black-hole mergers with gravitational-wave spin measurements | 8 | 8 | 8 |
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| **98** | Fabbri | 2025 | Reconstructing parametric gravitational-wave population fits from non-parametric results without refitting the data | 8 | 10 | 10 |
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| **99** | Santoliquido | 2024 | Classifying binary black holes from Population III stars with the Einstein Telescope: a machine-learning approach | 10 | 8 | 10 |
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| **100** | Cole | 2025 | Sequential simulation-based inference for extreme mass ratio inspirals | 9 | 9 | 9 |
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| **101** | Stegmann | 2025 | Distinguishing the origin of eccentric black-hole mergers with gravitational-wave spin measurements | 8 | 9 | 9 |
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| **102** | Fumagalli | 2025 | Non-adiabatic dynamics of eccentric black-hole binaries in post-Newtonian theory | 9 | 9 | 9 |
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| **103** | De Renzis | 2025 | Forecasting the population properties of merging black holes | 5 | 8 | 8 |
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| **104** | Spadaro | 2025 | Stars or gas? Constraining the hardening processes of massive black-hole binaries with LISA | 8 | 7 | 8 |
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| **105** | De Renzis | 2023 | Parameter estimation of binary black holes in the endpoint of the up-down instability | 4 | 8 | 8 |
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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** | Borhanian | 2025 | Impact of facility timing and coordination for next-generation gravitational-wave detectors | 0 | 0 | 0 |
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| **125** | Loutrel | 2025 | Probing modified gravitational-wave dispersion with bursts from eccentric black-hole binaries | 0 | 0 | 0 |
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| **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 |
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| **127** | Boschini | 2025 | “LHS in LHS”: a new expansion strategy for Latin hypercube sampling in simulation design | 0 | 0 | 0 |
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| **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 |
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| **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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| **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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## 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 | 2 |
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| 2026 | 3 |
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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 | 9 |
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| arXiv | 10 |
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| 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 | 43 |
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| astro-ph.HE | 44 |
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| astro-ph.GA | 9 |
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| astro-ph.CO | 2 |
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| astro-ph.IM | 1 |
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| stat.ME | 1 |
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<br><br>
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*Last updated: 2026-02-24 01:03:06 UTC*
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*Last updated: 2026-02-24 05:29:52 UTC*

‎_group.md‎

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*Last updated: 2026-02-24 01:03:06 UTC*
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*Last updated: 2026-02-24 05:29:52 UTC*

‎_publications.md‎

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## Summary
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**8** [Submitted papers](#submitted-papers)\
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**9** [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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**8.**
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*On the exceptionality of exceptional gravitational-wave events.*\
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R. Tenorio, **D. Gerosa**.\
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*Last updated: 2026-02-24 01:03:06 UTC*
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*Last updated: 2026-02-24 05:29:52 UTC*

‎_talks.md‎

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*Last updated: 2026-02-24 01:03:06 UTC*
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*Last updated: 2026-02-24 05:29:52 UTC*

‎database.py‎

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papers['submitted']['label'] = 'Submitted papers'
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papers['submitted']['data'] = []
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papers['submitted']['data'].append({
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"title": "Inferring the population properties of galactic binaries from LISA'sstochastic foreground",
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"author": "F. De Santi, A. Santini, A. Toubiana, N. Karnesis, D. Gerosa",
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"journal": "",
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"link": "",
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"arxiv": "arXiv:2602.18560 [astro-ph.HE]",
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"ads": "2026arXiv260218560D",
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"inspire": "DeSanti:2026xhs",
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"more": ""
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})
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papers['submitted']['data'].append({
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"title": "On the exceptionality of exceptional gravitational-wave events",
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"author": "R. Tenorio, D. Gerosa",

‎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{8} papers in submission stage,
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\textbf{9} papers in submission stage,
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\\ & &
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\textbf{14} other publications (white papers, proceedings, etc.)
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\end{tabular} }
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Summary metrics reported using ADS and InSpire excluding [including] long-authorlist papers:
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\\
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\textcolor{mark_color}{\textbf{Total number of citations}}: >6500 [>10700]
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\textcolor{mark_color}{\textbf{Total number of citations}}: >6500 [>10800]
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---
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\textcolor{mark_color}{\textbf{h-index}}: 44 [48].
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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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