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‎_citations.md‎

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## Citation Summary
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- **Total ADS citations**: 9718
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- **Total INSPIRE citations**: 10620
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- **Total MAX citations**: 10698
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- **Total ADS citations**: 9730
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- **Total INSPIRE citations**: 10630
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- **Total MAX citations**: 10708
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- **h-index**: 47
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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 | 1591 | 1591 |
13-
| **2** | Barack | 2019 | Black holes, gravitational waves and fundamental physics: a roadmap | 839 | 930 | 930 |
14-
| **3** | Amaro-Seoane | 2022 | Astrophysics with the Laser Interferometer Space Antenna | 741 | 693 | 741 |
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 | 456 | 474 | 474 |
16-
| **5** | Varma | 2019 | Surrogate models for precessing binary black hole simulations with unequal masses | 434 | 450 | 450 |
12+
| **1** | Berti | 2015 | Testing general relativity with present and future astrophysical observations | 1411 | 1592 | 1592 |
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| **2** | Barack | 2019 | Black holes, gravitational waves and fundamental physics: a roadmap | 840 | 931 | 931 |
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| **3** | Amaro-Seoane | 2022 | Astrophysics with the Laser Interferometer Space Antenna | 741 | 694 | 741 |
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 | 456 | 475 | 475 |
16+
| **5** | Varma | 2019 | Surrogate models for precessing binary black hole simulations with unequal masses | 432 | 450 | 450 |
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| **6** | Barausse | 2020 | Prospects for fundamental physics with LISA | 390 | 440 | 440 |
18-
| **7** | Arun | 2022 | New horizons for fundamental physics with LISA | 302 | 356 | 356 |
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| **7** | Arun | 2022 | New horizons for fundamental physics with LISA | 304 | 357 | 357 |
1919
| **8** | Gerosa | 2017 | Are merging black holes born from stellar collapse or previous mergers? | 331 | 356 | 356 |
2020
| **9** | Gerosa | 2021 | Hierarchical mergers of stellar-mass black holes and their gravitational-wave signatures | 266 | 282 | 282 |
21-
| **10** | Gerosa | 2018 | Spin orientations of merging black holes formed from the evolution of stellar binaries | 215 | 237 | 237 |
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| **11** | Afshordi | 2025 | Waveform modelling for the Laser Interferometer Space Antenna | 144 | 174 | 174 |
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| **12** | Gerosa | 2015 | Multi-timescale analysis of phase transitions in precessing black-hole binaries | 139 | 162 | 162 |
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| **13** | Varma | 2019 | High-accuracy mass, spin, and recoil predictions of generic black-hole merger remnants | 143 | 159 | 159 |
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| **10** | Gerosa | 2018 | Spin orientations of merging black holes formed from the evolution of stellar binaries | 217 | 237 | 237 |
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| **11** | Afshordi | 2025 | Waveform modelling for the Laser Interferometer Space Antenna | 144 | 175 | 175 |
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| **12** | Gerosa | 2015 | Multi-timescale analysis of phase transitions in precessing black-hole binaries | 138 | 162 | 162 |
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| **13** | Varma | 2019 | High-accuracy mass, spin, and recoil predictions of generic black-hole merger remnants | 142 | 160 | 160 |
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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 | 143 | 159 | 159 |
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| **15** | Islam | 2021 | Eccentric binary black hole surrogate models for the gravitational waveform and remnant properties: comparable mass, nonspinning case | 128 | 139 | 139 |
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| **16** | Vitale | 2020 | Inferring the properties of a population of compact binaries in presence of selection effects | 130 | 139 | 139 |
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| **17** | Kesden | 2015 | Effective potentials and morphological transitions for binary black-hole spin precession | 115 | 137 | 137 |
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| **18** | Ng | 2018 | Gravitational-wave astrophysics with effective-spin measurements: asymmetries and selection biases | 115 | 127 | 127 |
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| **16** | Vitale | 2020 | Inferring the properties of a population of compact binaries in presence of selection effects | 131 | 139 | 139 |
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| **17** | Kesden | 2015 | Effective potentials and morphological transitions for binary black-hole spin precession | 114 | 137 | 137 |
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| **18** | Ng | 2018 | Gravitational-wave astrophysics with effective-spin measurements: asymmetries and selection biases | 115 | 128 | 128 |
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| **19** | Baibhav | 2019 | Gravitational-wave detection rates for compact binaries formed in isolation: LIGO/Virgo O3 and beyond | 108 | 125 | 125 |
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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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| **27** | Romero-Shaw | 2023 | Eccentricity or spin precession? Distinguishing subdominant effects in gravitational-wave data | 82 | 96 | 96 |
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| **28** | Baibhav | 2020 | The mass gap, the spin gap, and the origin of merging binary black holes | 80 | 92 | 92 |
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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 | 68 | 79 | 79 |
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| **30** | Gerosa | 2021 | A generalized precession parameter $$\chi_\mathrm{p}$$ to interpret gravitational-wave data | 68 | 80 | 80 |
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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 | 76 | 78 | 78 |
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| **32** | Korol | 2020 | Populations of double white dwarfs in Milky Way satellites and their detectability with LISA | 77 | 76 | 77 |
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| **32** | Korol | 2020 | Populations of double white dwarfs in Milky Way satellites and their detectability with LISA | 76 | 76 | 76 |
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| **33** | Horbatsch | 2015 | Tensor-multi-scalar theories: relativistic stars and 3+1 decomposition | 70 | 74 | 74 |
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| **34** | Klein | 2022 | The last three years: multiband gravitational-wave observations of stellar-mass binary black holes | 61 | 68 | 68 |
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| **35** | Gerosa | 2016 | Black-hole kicks as new gravitational-wave observables | 63 | 67 | 67 |
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| **35** | Gerosa | 2016 | Black-hole kicks as new gravitational-wave observables | 62 | 67 | 67 |
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| **36** | Buscicchio | 2021 | Bayesian parameter estimation of stellar-mass black-hole binaries with LISA | 55 | 64 | 64 |
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| **37** | Gupta | 2020 | Black holes in the low mass gap: Implications for gravitational wave observations | 59 | 64 | 64 |
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| **38** | Gerosa | 2018 | Black-hole kicks from numerical-relativity surrogate models | 56 | 62 | 62 |
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| **39** | Gerosa | 2015 | Precessional instability in binary black holes with aligned spins | 56 | 61 | 61 |
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| **40** | Gerosa | 2020 | Astrophysical implications of GW190412 as a remnant of a previous black-hole merger | 54 | 60 | 60 |
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| **41** | Gerosa | 2016 | Numerical simulations of stellar collapse in scalar-tensor theories of gravity | 52 | 60 | 60 |
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| **42** | Gerosa | 2014 | Distinguishing black-hole spin-orbit resonances by their gravitational-wave signatures | 47 | 57 | 57 |
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| **39** | Gerosa | 2015 | Precessional instability in binary black holes with aligned spins | 55 | 61 | 61 |
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| **40** | Gerosa | 2020 | Astrophysical implications of GW190412 as a remnant of a previous black-hole merger | 53 | 60 | 60 |
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| **41** | Gerosa | 2016 | Numerical simulations of stellar collapse in scalar-tensor theories of gravity | 51 | 60 | 60 |
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| **42** | Gerosa | 2014 | Distinguishing black-hole spin-orbit resonances by their gravitational-wave signatures | 46 | 57 | 57 |
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| **43** | Mould | 2022 | Deep learning and Bayesian inference of gravitational-wave populations: hierarchical black-hole mergers | 52 | 56 | 56 |
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| **44** | Gerosa | 2015 | Spin alignment and differential accretion in merging black hole binaries | 55 | 50 | 55 |
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| **45** | Mould | 2022 | Which black hole formed first? Mass-ratio reversal in massive binary stars from gravitational-wave data | 47 | 53 | 53 |
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| **64** | Baibhav | 2021 | Looking for the parents of LIGO's black holes | 28 | 28 | 28 |
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| **65** | Chamberlain | 2019 | Frequency-domain waveform approximants capturing Doppler shifts | 26 | 28 | 28 |
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| **66** | Rosca-Mead | 2020 | Structure of neutron stars in massive scalar-tensor gravity | 23 | 26 | 26 |
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| **67** | Pacilio | 2024 | Flexible mapping of ringdown amplitudes for nonprecessing binary black holes | 21 | 25 | 25 |
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| **68** | Fumagalli | 2023 | Spin-eccentricity interplay in merging binary black holes | 23 | 25 | 25 |
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| **69** | Boschini | 2025 | Orbital eccentricity in general relativity from catastrophe theory | 22 | 24 | 24 |
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| **70** | Moore | 2021 | Population-informed priors in gravitational-wave astronomy | 24 | 23 | 24 |
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| **71** | Croon | 2025 | Can GW231123 have a stellar origin? | 0 | 23 | 23 |
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| **72** | Sperhake | 2020 | Amplification of superkicks in black-hole binaries through orbital eccentricity | 23 | 23 | 23 |
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| **67** | Croon | 2024 | Can GW231123 have a stellar origin? | 25 | 23 | 25 |
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| **68** | Pacilio | 2024 | Flexible mapping of ringdown amplitudes for nonprecessing binary black holes | 21 | 25 | 25 |
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| **69** | Fumagalli | 2023 | Spin-eccentricity interplay in merging binary black holes | 23 | 25 | 25 |
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| **70** | Boschini | 2025 | Orbital eccentricity in general relativity from catastrophe theory | 22 | 24 | 24 |
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| **71** | Moore | 2021 | Population-informed priors in gravitational-wave astronomy | 24 | 23 | 24 |
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| **72** | Sperhake | 2020 | Amplification of superkicks in black-hole binaries through orbital eccentricity | 22 | 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** | Mould | 2020 | Endpoint of the up-down instability in precessing binary black holes | 18 | 22 | 22 |
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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** | Toubiana | 2025 | Comparing astrophysical models to gravitational-wave data in the observable space | 5 | 4 | 5 |
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| **113** | Chiaberge | 2025 | A recoiling supermassive black hole in a powerful quasar | 5 | 4 | 5 |
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| **113** | Chiaberge | 2025 | A recoiling supermassive black hole in a powerful quasar | 5 | 5 | 5 |
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| **114** | Boschini | 2024 | Astrophysical and relativistic modeling of the recoiling black-hole candidate in quasar 3C 186 | 5 | 4 | 5 |
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| **115** | Gerosa | 2018 | Surprises from the spins: astrophysics and relativity with detections of spinning black-hole mergers | 4 | 5 | 5 |
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| **116** | Speri | 2026 | Single-harmonic search for extreme mass-ratio inspirals | 2 | 4 | 4 |
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| **116** | Speri | 2026 | Single-harmonic search for extreme mass-ratio inspirals | 3 | 4 | 4 |
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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 | 2 | 2 | 2 |
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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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| **119** | Gerosa | 2023 | QLUSTER: quick clusters of merging binary black holes | 2 | 0 | 2 |
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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** | Anselmo | 2025 | Black-hole ringdown with templates capturing spin precession: a criticalre-analysis of GW190521 | 1 | 1 | 1 |
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| 2021 | 12 |
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| 2022 | 10 |
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| 2023 | 11 |
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| 2024 | 10 |
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| 2025 | 27 |
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| 2024 | 11 |
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| 2025 | 26 |
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| 2026 | 2 |
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## Papers per journal
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*Last updated: 2026-02-11 01:01:19 UTC*
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*Last updated: 2026-02-11 13:23:57 UTC*

‎_group.md‎

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*Last updated: 2026-02-11 13:23:57 UTC*

‎_publications.md‎

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**107.**
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*Can GW231123 have a stellar origin?*\
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D. Croon, **D. Gerosa**, J. Sakstein.\
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Monthly Notices of the Royal Astronomical Society, in press. <a href="https://arxiv.org/abs/2508.10088" style="color: inherit; text-decoration: none;">arXiv:2508.10088 [astro-ph.HE]</a>.
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<a href="https://academic.oup.com/mnras/article/doi/10.1093/mnras/stag073/8431335" style="color: inherit; text-decoration: none;">Monthly Notices of the Royal Astronomical Society 530 (2024) stag073</a>. <a href="https://arxiv.org/abs/2508.10088" style="color: inherit; text-decoration: none;">arXiv:2508.10088 [astro-ph.HE]</a>.
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*Single-harmonic search for extreme mass-ratio inspirals.*\
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*Last updated: 2026-02-11 01:01:19 UTC*
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‎_talks.md‎

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*Last updated: 2026-02-11 01:01:19 UTC*
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*Last updated: 2026-02-11 13:23:57 UTC*

‎metricspapers.tex‎

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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}}: >6400 [>10600]
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\textcolor{mark_color}{\textbf{Total number of citations}}: >6400 [>10700]
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---
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\textcolor{mark_color}{\textbf{h-index}}: 44 [47].
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‎parsepapers.tex‎

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\newline{}
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D. Croon, \textbf{D. Gerosa}, J. Sakstein.
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\newline{}
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{\mnras, in press}. \href{https://arxiv.org/abs/2508.10088}{arXiv:2508.10088 [astro-ph.HE].}
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\href{https://academic.oup.com/mnras/article/doi/10.1093/mnras/stag073/8431335}{\mnras 530 (2024) stag073}. \href{https://arxiv.org/abs/2508.10088}{arXiv:2508.10088 [astro-ph.HE].}
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\textbf{106.} & & \textit{Single-harmonic search for extreme mass-ratio inspirals.}

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