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1 | 1 | ## Citation Summary |
2 | 2 |
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3 | | -- **Total ADS citations**: 9773 |
4 | | -- **Total INSPIRE citations**: 10672 |
5 | | -- **Total MAX citations**: 10748 |
| 3 | +- **Total ADS citations**: 9767 |
| 4 | +- **Total INSPIRE citations**: 10676 |
| 5 | +- **Total MAX citations**: 10751 |
6 | 6 | - **h-index**: 47 |
7 | 7 |
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8 | 8 | ## Paper list sorted by citation count |
9 | 9 |
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10 | 10 | | # | Author | Year | Title | ADS | INSPIRE | MAX | |
11 | 11 | |---|--------|------|-------|-----|---------|-----| |
12 | | -| **1** | Berti | 2015 | Testing general relativity with present and future astrophysical observations | 1413 | 1593 | 1593 | |
| 12 | +| **1** | Berti | 2015 | Testing general relativity with present and future astrophysical observations | 1412 | 1593 | 1593 | |
13 | 13 | | **2** | Barack | 2019 | Black holes, gravitational waves and fundamental physics: a roadmap | 842 | 935 | 935 | |
14 | 14 | | **3** | Amaro-Seoane | 2022 | Astrophysics with the Laser Interferometer Space Antenna | 745 | 699 | 745 | |
15 | 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 | 458 | 476 | 476 | |
16 | 16 | | **5** | Varma | 2019 | Surrogate models for precessing binary black hole simulations with unequal masses | 434 | 450 | 450 | |
17 | 17 | | **6** | Barausse | 2020 | Prospects for fundamental physics with LISA | 391 | 440 | 440 | |
18 | 18 | | **7** | Arun | 2022 | New horizons for fundamental physics with LISA | 307 | 360 | 360 | |
19 | 19 | | **8** | Gerosa | 2017 | Are merging black holes born from stellar collapse or previous mergers? | 331 | 358 | 358 | |
20 | | -| **9** | Gerosa | 2021 | Hierarchical mergers of stellar-mass black holes and their gravitational-wave signatures | 268 | 284 | 284 | |
| 20 | +| **9** | Gerosa | 2021 | Hierarchical mergers of stellar-mass black holes and their gravitational-wave signatures | 267 | 284 | 284 | |
21 | 21 | | **10** | Gerosa | 2018 | Spin orientations of merging black holes formed from the evolution of stellar binaries | 218 | 240 | 240 | |
22 | 22 | | **11** | Afshordi | 2025 | Waveform modelling for the Laser Interferometer Space Antenna | 146 | 175 | 175 | |
23 | 23 | | **12** | Gerosa | 2015 | Multi-timescale analysis of phase transitions in precessing black-hole binaries | 138 | 162 | 162 | |
24 | | -| **13** | Varma | 2019 | High-accuracy mass, spin, and recoil predictions of generic black-hole merger remnants | 144 | 160 | 160 | |
| 24 | +| **13** | Varma | 2019 | High-accuracy mass, spin, and recoil predictions of generic black-hole merger remnants | 143 | 160 | 160 | |
25 | 25 | | **14** | Gerosa | 2013 | Resonant-plane locking and spin alignment in stellar-mass black-hole binaries: a diagnostic of compact-binary formation | 144 | 160 | 160 | |
26 | 26 | | **15** | Islam | 2021 | Eccentric binary black hole surrogate models for the gravitational waveform and remnant properties: comparable mass, nonspinning case | 128 | 139 | 139 | |
27 | 27 | | **16** | Vitale | 2020 | Inferring the properties of a population of compact binaries in presence of selection effects | 131 | 139 | 139 | |
28 | 28 | | **17** | Kesden | 2015 | Effective potentials and morphological transitions for binary black-hole spin precession | 114 | 137 | 137 | |
29 | | -| **18** | Ng | 2018 | Gravitational-wave astrophysics with effective-spin measurements: asymmetries and selection biases | 116 | 128 | 128 | |
| 29 | +| **18** | Ng | 2018 | Gravitational-wave astrophysics with effective-spin measurements: asymmetries and selection biases | 116 | 129 | 129 | |
30 | 30 | | **19** | Baibhav | 2019 | Gravitational-wave detection rates for compact binaries formed in isolation: LIGO/Virgo O3 and beyond | 108 | 127 | 127 | |
31 | 31 | | **20** | Gerosa | 2019 | Multiband gravitational-wave event rates and stellar physics | 110 | 121 | 121 | |
32 | 32 | | **21** | Gerosa | 2019 | Escape speed of stellar clusters from multiple-generation black-hole mergers in the upper mass gap | 110 | 119 | 119 | |
33 | 33 | | **22** | Gerosa | 2016 | PRECESSION: Dynamics of spinning black-hole binaries with python | 93 | 103 | 103 | |
34 | 34 | | **23** | Wysocki | 2018 | Explaining LIGO's observations via isolated binary evolution with natal kicks | 98 | 102 | 102 | |
35 | | -| **24** | Vitale | 2017 | Impact of Bayesian priors on the characterization of binary black hole coalescences | 86 | 101 | 101 | |
| 35 | +| **24** | Vitale | 2017 | Impact of Bayesian priors on the characterization of binary black hole coalescences | 86 | 102 | 102 | |
36 | 36 | | **25** | Moore | 2019 | Are stellar-mass black-hole binaries too quiet for LISA? | 89 | 100 | 100 | |
37 | | -| **26** | Romero-Shaw | 2023 | Eccentricity or spin precession? Distinguishing subdominant effects in gravitational-wave data | 82 | 97 | 97 | |
| 37 | +| **26** | Romero-Shaw | 2023 | Eccentricity or spin precession? Distinguishing subdominant effects in gravitational-wave data | 82 | 98 | 98 | |
38 | 38 | | **27** | Taylor | 2018 | Mining gravitational-wave catalogs to understand binary stellar evolution: a new hierarchical bayesian framework | 92 | 97 | 97 | |
39 | 39 | | **28** | Baibhav | 2020 | The mass gap, the spin gap, and the origin of merging binary black holes | 80 | 93 | 93 | |
40 | 40 | | **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 | |
41 | 41 | | **30** | Gerosa | 2021 | A generalized precession parameter $$\chi_\mathrm{p}$$ to interpret gravitational-wave data | 69 | 80 | 80 | |
42 | | -| **31** | Korol | 2020 | Populations of double white dwarfs in Milky Way satellites and their detectability with LISA | 78 | 77 | 78 | |
43 | | -| **32** | Bouffanais | 2019 | Constraining the fraction of binary black holes formed in isolation and young star clusters with gravitational-wave data | 76 | 78 | 78 | |
| 42 | +| **31** | Bouffanais | 2019 | Constraining the fraction of binary black holes formed in isolation and young star clusters with gravitational-wave data | 76 | 78 | 78 | |
| 43 | +| **32** | Korol | 2020 | Populations of double white dwarfs in Milky Way satellites and their detectability with LISA | 77 | 77 | 77 | |
44 | 44 | | **33** | Horbatsch | 2015 | Tensor-multi-scalar theories: relativistic stars and 3+1 decomposition | 70 | 74 | 74 | |
45 | 45 | | **34** | Klein | 2022 | The last three years: multiband gravitational-wave observations of stellar-mass binary black holes | 61 | 68 | 68 | |
46 | | -| **35** | Gerosa | 2016 | Black-hole kicks as new gravitational-wave observables | 63 | 67 | 67 | |
| 46 | +| **35** | Gerosa | 2016 | Black-hole kicks as new gravitational-wave observables | 62 | 67 | 67 | |
47 | 47 | | **36** | Buscicchio | 2021 | Bayesian parameter estimation of stellar-mass black-hole binaries with LISA | 55 | 64 | 64 | |
48 | 48 | | **37** | Gupta | 2020 | Black holes in the low mass gap: Implications for gravitational wave observations | 59 | 64 | 64 | |
49 | 49 | | **38** | Gerosa | 2018 | Black-hole kicks from numerical-relativity surrogate models | 56 | 62 | 62 | |
50 | 50 | | **39** | Gerosa | 2015 | Precessional instability in binary black holes with aligned spins | 55 | 61 | 61 | |
51 | | -| **40** | Gerosa | 2020 | Astrophysical implications of GW190412 as a remnant of a previous black-hole merger | 54 | 60 | 60 | |
| 51 | +| **40** | Gerosa | 2020 | Astrophysical implications of GW190412 as a remnant of a previous black-hole merger | 53 | 60 | 60 | |
52 | 52 | | **41** | Gerosa | 2016 | Numerical simulations of stellar collapse in scalar-tensor theories of gravity | 51 | 60 | 60 | |
53 | 53 | | **42** | Mould | 2022 | Deep learning and Bayesian inference of gravitational-wave populations: hierarchical black-hole mergers | 54 | 57 | 57 | |
54 | 54 | | **43** | Gerosa | 2014 | Distinguishing black-hole spin-orbit resonances by their gravitational-wave signatures | 46 | 57 | 57 | |
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83 | 83 | | **72** | Sperhake | 2020 | Amplification of superkicks in black-hole binaries through orbital eccentricity | 23 | 23 | 23 | |
84 | 84 | | **73** | Zhao | 2017 | Nutational resonances, transitional precession, and precession-averaged evolution in binary black-hole systems | 21 | 23 | 23 | |
85 | 85 | | **74** | Gerosa | 2017 | On the equal-mass limit of precessing black-hole binaries | 19 | 23 | 23 | |
86 | | -| **75** | Mould | 2020 | Endpoint of the up-down instability in precessing binary black holes | 18 | 22 | 22 | |
87 | | -| **76** | Gerosa | 2019 | Wide nutation: binary black-hole spins repeatedly oscillating from full alignment to full anti-alignment | 20 | 22 | 22 | |
88 | | -| **77** | Romero-Shaw | 2025 | GW200208_222617 as an eccentric black-hole binary merger: properties and astrophysical implications | 21 | 21 | 21 | |
| 86 | +| **75** | Romero-Shaw | 2025 | GW200208_222617 as an eccentric black-hole binary merger: properties and astrophysical implications | 21 | 22 | 22 | |
| 87 | +| **76** | Mould | 2020 | Endpoint of the up-down instability in precessing binary black holes | 18 | 22 | 22 | |
| 88 | +| **77** | Gerosa | 2019 | Wide nutation: binary black-hole spins repeatedly oscillating from full alignment to full anti-alignment | 20 | 22 | 22 | |
89 | 89 | | **78** | Mancarella | 2023 | Inferring, not just detecting: metrics for high-redshift sources observed with third-generation gravitational-wave detectors | 16 | 21 | 21 | |
90 | 90 | | **79** | Nealon | 2022 | The Bardeen-Petterson effect in accreting supermassive black-hole binaries: disc breaking and critical obliquity | 21 | 14 | 21 | |
91 | 91 | | **80** | Gangardt | 2021 | A taxonomy of black-hole binary spin precession and nutation | 16 | 20 | 20 | |
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205 | 205 | <br><br> |
206 | | -*Last updated: 2026-02-18 01:01:20 UTC* |
| 206 | +*Last updated: 2026-02-18 11:59:16 UTC* |
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