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‎CV.tex‎

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For collaborative grants, the reported amount refers to the portion awarded to my unit/group.
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\cvitemwithcomment{}{\textbf{Italian-French University (UIF/UFI) - Chapter 3 Grant}. PI unit leader, 78k EUR, No.~2025-C3-386.}{2025-2029}\vspace{-0.05cm}
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\cvitemwithcomment{}{\textbf{Italian-French University (UIF/UFI) - Chapter 3 Grant}. PI, unit leader, 78k EUR, No.~2025-C3-386.}{2025-2029}\vspace{-0.05cm}
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\cvitemwithcomment{}{\hspace{0.6cm}\textit{``Populations of compact objects for next-generation gravitational-wave detectors''}}{}
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\cvitemwithcomment{}{\textbf{Ministero Universit\`a e Ricerca (MUR) -- PRIN Grant}. Co-I unit leader, 85k EUR. No. 2022-Z9X4XS}{2023-2025}\vspace{-0.05cm}
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\cvitemwithcomment{}{\textbf{Ministero Universit\`a e Ricerca (MUR) -- PRIN Grant}. Co-I, unit leader, 85k EUR. No. 2022-Z9X4XS}{2023-2025}\vspace{-0.05cm}
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\cvitemwithcomment{}{\hspace{0.6cm}\textit{``Gravitational-wave astronomy as a mature field: selection biases and environmental effects''}}{}
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\cvitemwithcomment{}{\textbf{European Research Council (ERC) -- Starting Grant}. PI, 1.5M EUR, No.~945155--GWmining.}{2021-2026}\vspace{-0.05cm}

‎CVshort.tex‎

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For collaborative grants, the reported amount refers to the portion awarded to my unit/group.
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\cvitemwithcomment{}{\textbf{Italian-French University (UIF/UFI) - Chapter 3 Grant}. PI unit leader, 78k EUR, No.~2025-C3-386.}{2025-2029}\vspace{-0.05cm}
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\cvitemwithcomment{}{\textbf{Italian-French University (UIF/UFI) - Chapter 3 Grant}. PI, unit leader, 78k EUR, No.~2025-C3-386.}{2025-2029}\vspace{-0.05cm}
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\cvitemwithcomment{}{\hspace{0.6cm}\textit{``Populations of compact objects for next-generation gravitational-wave detectors''}}{}
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\cvitemwithcomment{}{\textbf{Ministero Universit\`a e Ricerca (MUR) -- PRIN Grant}. Co-I unit leader, 85k EUR. No. 2022-Z9X4XS}{2023-2025}\vspace{-0.05cm}
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\cvitemwithcomment{}{\textbf{Ministero Universit\`a e Ricerca (MUR) -- PRIN Grant}. Co-I, unit leader, 85k EUR. No. 2022-Z9X4XS}{2023-2025}\vspace{-0.05cm}
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\cvitemwithcomment{}{\hspace{0.6cm}\textit{``Gravitational-wave astronomy as a mature field: selection biases and environmental effects''}}{}
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\cvitemwithcomment{}{\textbf{European Research Council (ERC) -- Starting Grant}. PI, 1.5M EUR, No.~945155--GWmining.}{2021-2026}\vspace{-0.05cm}

‎_citations.md‎

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## Citation Summary
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- **Total ADS citations**: 9779
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- **Total INSPIRE citations**: 10692
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- **Total MAX citations**: 10766
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- **Total ADS citations**: 9791
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- **Total INSPIRE citations**: 10695
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- **Total MAX citations**: 10770
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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 | 1413 | 1597 | 1597 |
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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 | 935 | 935 |
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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 | 458 | 476 | 476 |
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| **5** | Varma | 2019 | Surrogate models for precessing binary black hole simulations with unequal masses | 432 | 451 | 451 |
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| **6** | Barausse | 2020 | Prospects for fundamental physics with LISA | 391 | 439 | 439 |
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| **6** | Barausse | 2020 | Prospects for fundamental physics with LISA | 391 | 440 | 440 |
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| **7** | Arun | 2022 | New horizons for fundamental physics with LISA | 308 | 360 | 360 |
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| **8** | Gerosa | 2017 | Are merging black holes born from stellar collapse or previous mergers? | 333 | 358 | 358 |
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| **9** | Gerosa | 2021 | Hierarchical mergers of stellar-mass black holes and their gravitational-wave signatures | 267 | 285 | 285 |
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| **9** | Gerosa | 2021 | Hierarchical mergers of stellar-mass black holes and their gravitational-wave signatures | 270 | 286 | 286 |
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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 | 146 | 176 | 176 |
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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** | Gerosa | 2013 | Resonant-plane locking and spin alignment in stellar-mass black-hole binaries: a diagnostic of compact-binary formation | 144 | 161 | 161 |
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| **14** | Varma | 2019 | High-accuracy mass, spin, and recoil predictions of generic black-hole merger remnants | 143 | 160 | 160 |
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| **13** | 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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| **14** | Varma | 2019 | High-accuracy mass, spin, and recoil predictions of generic black-hole merger remnants | 144 | 160 | 160 |
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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 | 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 | 116 | 129 | 129 |
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| **19** | Baibhav | 2019 | Gravitational-wave detection rates for compact binaries formed in isolation: LIGO/Virgo O3 and beyond | 109 | 127 | 127 |
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| **20** | Gerosa | 2019 | Multiband gravitational-wave event rates and stellar physics | 110 | 121 | 121 |
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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 | 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 | 87 | 102 | 102 |
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| **25** | Moore | 2019 | Are stellar-mass black-hole binaries too quiet for LISA? | 88 | 100 | 100 |
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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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| **28** | Baibhav | 2020 | The mass gap, the spin gap, and the origin of merging binary black holes | 80 | 93 | 93 |
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| **28** | Baibhav | 2020 | The mass gap, the spin gap, and the origin of merging binary black holes | 81 | 93 | 93 |
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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 | 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 | 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 | 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 | 62 | 67 | 67 |
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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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| **46** | Roebber | 2020 | Milky Way satellites shining bright in gravitational waves | 45 | 51 | 51 |
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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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| **48** | Moore | 2021 | Testing general relativity with gravitational-wave catalogs: the insidious nature of waveform systematics | 42 | 48 | 48 |
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| **48** | Moore | 2021 | Testing general relativity with gravitational-wave catalogs: the insidious nature of waveform systematics | 43 | 48 | 48 |
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| **49** | Gerosa | 2015 | Missing black holes in brightest cluster galaxies as evidence for the occurrence of superkicks in nature | 41 | 47 | 47 |
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| **50** | Gangardt | 2024 | pAGN: the one-stop solution for AGN disc modeling | 45 | 46 | 46 |
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| **51** | Tso | 2019 | Optimizing LIGO with LISA forewarnings to improve black-hole spectroscopy | 37 | 43 | 43 |
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| **60** | Sayeb | 2021 | Massive black hole binary inspiral and spin evolution in a cosmological framework | 31 | 29 | 31 |
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| **61** | Mould | 2022 | Gravitational-wave population inference at past time infinity | 26 | 30 | 30 |
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| **62** | Wong | 2019 | Machine-learning interpolation of population-synthesis simulations to interpret gravitational-wave observations: a case study | 25 | 30 | 30 |
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| **63** | Chamberlain | 2019 | Frequency-domain waveform approximants capturing Doppler shifts | 26 | 29 | 29 |
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| **63** | Chamberlain | 2019 | Frequency-domain waveform approximants capturing Doppler shifts | 27 | 29 | 29 |
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| **64** | Fumagalli | 2024 | Residual eccentricity as a systematic uncertainty on the formation channels of binary black holes | 28 | 27 | 28 |
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| **65** | Baibhav | 2021 | Looking for the parents of LIGO's black holes | 28 | 28 | 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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| **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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| **79** | Nealon | 2022 | The Bardeen-Petterson effect in accreting supermassive black-hole binaries: disc breaking and critical obliquity | 21 | 14 | 21 |
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| **80** | Gangardt | 2021 | A taxonomy of black-hole binary spin precession and nutation | 16 | 20 | 20 |
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| **81** | Mancarella | 2025 | Sampling the full hierarchical population posterior distribution in gravitational-wave astronomy | 14 | 19 | 19 |
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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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| **84** | Buscicchio | 2025 | A test for LISA foreground Gaussianity and stationarity. I. Galactic white-dwarf binaries | 17 | 17 | 17 |
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‎_group.md‎

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‎_publications.md‎

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‎_talks.md‎

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