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‎_citations.md‎

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## Citation Summary
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- **Total ADS citations**: 9839
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- **Total INSPIRE citations**: 10777
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- **Total MAX citations**: 10851
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- **Total ADS citations**: 9855
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- **Total INSPIRE citations**: 10789
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- **Total MAX citations**: 10866
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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 | 1416 | 1606 | 1606 |
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| **1** | Berti | 2015 | Testing general relativity with present and future astrophysical observations | 1417 | 1606 | 1606 |
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| **2** | Barack | 2019 | Black holes, gravitational waves and fundamental physics: a roadmap | 848 | 939 | 939 |
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| **3** | Amaro-Seoane | 2022 | Astrophysics with the Laser Interferometer Space Antenna | 754 | 707 | 754 |
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| **3** | Amaro-Seoane | 2022 | Astrophysics with the Laser Interferometer Space Antenna | 755 | 707 | 755 |
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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 | 434 | 455 | 455 |
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| **6** | Barausse | 2020 | Prospects for fundamental physics with LISA | 395 | 443 | 443 |
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| **7** | Arun | 2022 | New horizons for fundamental physics with LISA | 309 | 361 | 361 |
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| **8** | Gerosa | 2017 | Are merging black holes born from stellar collapse or previous mergers? | 335 | 361 | 361 |
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| **9** | Gerosa | 2021 | Hierarchical mergers of stellar-mass black holes and their gravitational-wave signatures | 269 | 291 | 291 |
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| **10** | Gerosa | 2018 | Spin orientations of merging black holes formed from the evolution of stellar binaries | 219 | 242 | 242 |
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| **5** | Varma | 2019 | Surrogate models for precessing binary black hole simulations with unequal masses | 436 | 456 | 456 |
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| **6** | Barausse | 2020 | Prospects for fundamental physics with LISA | 395 | 444 | 444 |
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| **7** | Gerosa | 2017 | Are merging black holes born from stellar collapse or previous mergers? | 336 | 362 | 362 |
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| **8** | Arun | 2022 | New horizons for fundamental physics with LISA | 309 | 361 | 361 |
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| **9** | Gerosa | 2021 | Hierarchical mergers of stellar-mass black holes and their gravitational-wave signatures | 271 | 294 | 294 |
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| **10** | Gerosa | 2018 | Spin orientations of merging black holes formed from the evolution of stellar binaries | 219 | 243 | 243 |
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| **11** | Afshordi | 2025 | Waveform modelling for the Laser Interferometer Space Antenna | 146 | 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 | 143 | 162 | 162 |
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| **12** | Varma | 2019 | High-accuracy mass, spin, and recoil predictions of generic black-hole merger remnants | 144 | 163 | 163 |
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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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| **15** | Vitale | 2020 | Inferring the properties of a population of compact binaries in presence of selection effects | 132 | 142 | 142 |
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| **16** | Islam | 2021 | Eccentric binary black hole surrogate models for the gravitational waveform and remnant properties: comparable mass, nonspinning case | 129 | 140 | 140 |
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| **15** | Vitale | 2020 | Inferring the properties of a population of compact binaries in presence of selection effects | 132 | 143 | 143 |
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| **16** | Islam | 2021 | Eccentric binary black hole surrogate models for the gravitational waveform and remnant properties: comparable mass, nonspinning case | 129 | 141 | 141 |
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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 | 116 | 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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| **21** | Gerosa | 2019 | Escape speed of stellar clusters from multiple-generation black-hole mergers in the upper mass gap | 111 | 120 | 120 |
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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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| **22** | Wysocki | 2018 | Explaining LIGO's observations via isolated binary evolution with natal kicks | 99 | 104 | 104 |
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| **23** | Gerosa | 2016 | PRECESSION: Dynamics of spinning black-hole binaries with python | 94 | 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 | 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 | 82 | 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 | 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 | 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 | 77 | 77 |
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| **31** | Korol | 2020 | Populations of double white dwarfs in Milky Way satellites and their detectability with LISA | 78 | 77 | 78 |
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| **32** | 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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| **33** | Horbatsch | 2015 | Tensor-multi-scalar theories: relativistic stars and 3+1 decomposition | 70 | 75 | 75 |
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| **34** | Klein | 2022 | The last three years: multiband gravitational-wave observations of stellar-mass binary black holes | 62 | 67 | 67 |
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| **35** | Gerosa | 2016 | Black-hole kicks as new gravitational-wave observables | 62 | 67 | 67 |
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| **35** | Gerosa | 2016 | Black-hole kicks as new gravitational-wave observables | 63 | 67 | 67 |
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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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| **38** | Gerosa | 2018 | Black-hole kicks from numerical-relativity surrogate models | 56 | 63 | 63 |
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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 | 2016 | Numerical simulations of stellar collapse in scalar-tensor theories of gravity | 51 | 60 | 60 |
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| **41** | Gerosa | 2020 | Astrophysical implications of GW190412 as a remnant of a previous black-hole merger | 53 | 59 | 59 |
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| **42** | Mould | 2022 | Deep learning and Bayesian inference of gravitational-wave populations: hierarchical black-hole mergers | 55 | 58 | 58 |
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| **41** | Mould | 2022 | Deep learning and Bayesian inference of gravitational-wave populations: hierarchical black-hole mergers | 55 | 59 | 59 |
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| **42** | Gerosa | 2020 | Astrophysical implications of GW190412 as a remnant of a previous black-hole merger | 54 | 59 | 59 |
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| **43** | Gerosa | 2014 | Distinguishing black-hole spin-orbit resonances by their gravitational-wave signatures | 46 | 57 | 57 |
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| **44** | Mould | 2022 | Which black hole formed first? Mass-ratio reversal in massive binary stars from gravitational-wave data | 47 | 55 | 55 |
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| **44** | Mould | 2022 | Which black hole formed first? Mass-ratio reversal in massive binary stars from gravitational-wave data | 48 | 55 | 55 |
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| **45** | Gerosa | 2015 | Spin alignment and differential accretion in merging black hole binaries | 55 | 50 | 55 |
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| **46** | Roebber | 2020 | Milky Way satellites shining bright in gravitational waves | 46 | 52 | 52 |
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| **47** | Sperhake | 2017 | Long-lived inverse chirp signals from core collapse in massive scalar-tensor gravity | 43 | 50 | 50 |
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| **51** | Tso | 2019 | Optimizing LIGO with LISA forewarnings to improve black-hole spectroscopy | 37 | 43 | 43 |
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| **52** | Gerosa | 2020 | Gravitational-wave selection effects using neural-network classifiers | 38 | 42 | 42 |
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| **53** | Trifiro' | 2016 | Distinguishing black-hole spin-orbit resonances by their gravitational wave signatures. II: Full parameter estimation | 34 | 42 | 42 |
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| **54** | Santini | 2023 | Black-hole mergers in disk-like environments could explain the observed $$q-\chi_\mathrm{eff}$$ correlation | 40 | 40 | 40 |
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| **54** | Santini | 2023 | Black-hole mergers in disk-like environments could explain the observed $$q-\chi_\mathrm{eff}$$ correlation | 40 | 41 | 41 |
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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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| **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** | Moore | 2021 | Population-informed priors in gravitational-wave astronomy | 26 | 26 | 26 |
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| **67** | Rosca-Mead | 2020 | Structure of neutron stars in massive scalar-tensor gravity | 23 | 26 | 26 |
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| **68** | Croon | 2026 | Can GW231123 have a stellar origin? | 25 | 24 | 25 |
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| **66** | Croon | 2026 | Can GW231123 have a stellar origin? | 26 | 24 | 26 |
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| **67** | Moore | 2021 | Population-informed priors in gravitational-wave astronomy | 26 | 26 | 26 |
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| **68** | Rosca-Mead | 2020 | Structure of neutron stars in massive scalar-tensor gravity | 23 | 26 | 26 |
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| **69** | Romero-Shaw | 2025 | GW200208_222617 as an eccentric black-hole binary merger: properties and astrophysical implications | 25 | 24 | 25 |
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| **70** | Pacilio | 2024 | Flexible mapping of ringdown amplitudes for nonprecessing binary black holes | 22 | 25 | 25 |
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| **71** | Fumagalli | 2023 | Spin-eccentricity interplay in merging binary black holes | 23 | 25 | 25 |
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| **72** | Boschini | 2025 | Orbital eccentricity in general relativity from catastrophe theory | 22 | 24 | 24 |
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| **73** | Sperhake | 2020 | Amplification of superkicks in black-hole binaries through orbital eccentricity | 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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‎_group.md‎

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‎_publications.md‎

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‎_talks.md‎

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