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1 | 1 | ## Citation Summary |
2 | 2 |
|
3 | | -- **Total ADS citations**: 9894 |
4 | | -- **Total INSPIRE citations**: 10832 |
5 | | -- **Total MAX citations**: 10914 |
| 3 | +- **Total ADS citations**: 9884 |
| 4 | +- **Total INSPIRE citations**: 10840 |
| 5 | +- **Total MAX citations**: 10919 |
6 | 6 | - **h-index**: 48 |
7 | 7 |
|
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 | 1420 | 1610 | 1610 | |
13 | | -| **2** | Barack | 2019 | Black holes, gravitational waves and fundamental physics: a roadmap | 850 | 942 | 942 | |
14 | | -| **3** | Amaro-Seoane | 2022 | Astrophysics with the Laser Interferometer Space Antenna | 761 | 709 | 761 | |
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 | 459 | 479 | 479 | |
16 | | -| **5** | Varma | 2019 | Surrogate models for precessing binary black hole simulations with unequal masses | 439 | 458 | 458 | |
17 | | -| **6** | Barausse | 2020 | Prospects for fundamental physics with LISA | 398 | 454 | 454 | |
18 | | -| **7** | Arun | 2022 | New horizons for fundamental physics with LISA | 311 | 365 | 365 | |
| 12 | +| **1** | Berti | 2015 | Testing general relativity with present and future astrophysical observations | 1420 | 1611 | 1611 | |
| 13 | +| **2** | Barack | 2019 | Black holes, gravitational waves and fundamental physics: a roadmap | 850 | 943 | 943 | |
| 14 | +| **3** | Amaro-Seoane | 2022 | Astrophysics with the Laser Interferometer Space Antenna | 761 | 711 | 761 | |
| 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 | 479 | 479 | |
| 16 | +| **5** | Varma | 2019 | Surrogate models for precessing binary black hole simulations with unequal masses | 438 | 458 | 458 | |
| 17 | +| **6** | Barausse | 2020 | Prospects for fundamental physics with LISA | 398 | 455 | 455 | |
| 18 | +| **7** | Arun | 2022 | New horizons for fundamental physics with LISA | 311 | 366 | 366 | |
19 | 19 | | **8** | Gerosa | 2017 | Are merging black holes born from stellar collapse or previous mergers? | 336 | 364 | 364 | |
20 | | -| **9** | Gerosa | 2021 | Hierarchical mergers of stellar-mass black holes and their gravitational-wave signatures | 274 | 295 | 295 | |
| 20 | +| **9** | Gerosa | 2021 | Hierarchical mergers of stellar-mass black holes and their gravitational-wave signatures | 272 | 295 | 295 | |
21 | 21 | | **10** | Gerosa | 2018 | Spin orientations of merging black holes formed from the evolution of stellar binaries | 221 | 244 | 244 | |
22 | 22 | | **11** | Afshordi | 2025 | Waveform modelling for the Laser Interferometer Space Antenna | 148 | 180 | 180 | |
23 | 23 | | **12** | Varma | 2019 | High-accuracy mass, spin, and recoil predictions of generic black-hole merger remnants | 144 | 164 | 164 | |
|
30 | 30 | | **19** | Baibhav | 2019 | Gravitational-wave detection rates for compact binaries formed in isolation: LIGO/Virgo O3 and beyond | 109 | 128 | 128 | |
31 | 31 | | **20** | Gerosa | 2019 | Escape speed of stellar clusters from multiple-generation black-hole mergers in the upper mass gap | 112 | 121 | 121 | |
32 | 32 | | **21** | Gerosa | 2019 | Multiband gravitational-wave event rates and stellar physics | 111 | 121 | 121 | |
33 | | -| **22** | Wysocki | 2018 | Explaining LIGO's observations via isolated binary evolution with natal kicks | 99 | 105 | 105 | |
| 33 | +| **22** | Wysocki | 2018 | Explaining LIGO's observations via isolated binary evolution with natal kicks | 98 | 105 | 105 | |
34 | 34 | | **23** | Gerosa | 2016 | PRECESSION: Dynamics of spinning black-hole binaries with python | 93 | 104 | 104 | |
35 | 35 | | **24** | Vitale | 2017 | Impact of Bayesian priors on the characterization of binary black hole coalescences | 88 | 102 | 102 | |
36 | | -| **25** | Romero-Shaw | 2023 | Eccentricity or spin precession? Distinguishing subdominant effects in gravitational-wave data | 86 | 101 | 101 | |
| 36 | +| **25** | Romero-Shaw | 2023 | Eccentricity or spin precession? Distinguishing subdominant effects in gravitational-wave data | 85 | 101 | 101 | |
37 | 37 | | **26** | Moore | 2019 | Are stellar-mass black-hole binaries too quiet for LISA? | 88 | 100 | 100 | |
38 | 38 | | **27** | Taylor | 2018 | Mining gravitational-wave catalogs to understand binary stellar evolution: a new hierarchical bayesian framework | 93 | 98 | 98 | |
39 | 39 | | **28** | Baibhav | 2020 | The mass gap, the spin gap, and the origin of merging binary black holes | 83 | 95 | 95 | |
|
42 | 42 | | **31** | Bouffanais | 2019 | Constraining the fraction of binary black holes formed in isolation and young star clusters with gravitational-wave data | 77 | 79 | 79 | |
43 | 43 | | **32** | Korol | 2020 | Populations of double white dwarfs in Milky Way satellites and their detectability with LISA | 78 | 77 | 78 | |
44 | 44 | | **33** | Horbatsch | 2015 | Tensor-multi-scalar theories: relativistic stars and 3+1 decomposition | 70 | 76 | 76 | |
45 | | -| **34** | Klein | 2022 | The last three years: multiband gravitational-wave observations of stellar-mass binary black holes | 63 | 69 | 69 | |
| 45 | +| **34** | Klein | 2022 | The last three years: multiband gravitational-wave observations of stellar-mass binary black holes | 62 | 69 | 69 | |
46 | 46 | | **35** | Gerosa | 2016 | Black-hole kicks as new gravitational-wave observables | 63 | 68 | 68 | |
47 | 47 | | **36** | Gupta | 2020 | Black holes in the low mass gap: Implications for gravitational wave observations | 58 | 64 | 64 | |
48 | 48 | | **37** | Buscicchio | 2021 | Bayesian parameter estimation of stellar-mass black-hole binaries with LISA | 55 | 63 | 63 | |
|
52 | 52 | | **41** | Mould | 2022 | Deep learning and Bayesian inference of gravitational-wave populations: hierarchical black-hole mergers | 55 | 59 | 59 | |
53 | 53 | | **42** | Gerosa | 2020 | Astrophysical implications of GW190412 as a remnant of a previous black-hole merger | 54 | 59 | 59 | |
54 | 54 | | **43** | Gerosa | 2014 | Distinguishing black-hole spin-orbit resonances by their gravitational-wave signatures | 46 | 57 | 57 | |
55 | | -| **44** | Mould | 2022 | Which black hole formed first? Mass-ratio reversal in massive binary stars from gravitational-wave data | 48 | 55 | 55 | |
| 55 | +| **44** | Mould | 2022 | Which black hole formed first? Mass-ratio reversal in massive binary stars from gravitational-wave data | 47 | 55 | 55 | |
56 | 56 | | **45** | Gerosa | 2015 | Spin alignment and differential accretion in merging black hole binaries | 55 | 50 | 55 | |
57 | 57 | | **46** | Roebber | 2020 | Milky Way satellites shining bright in gravitational waves | 46 | 52 | 52 | |
58 | 58 | | **47** | Sperhake | 2017 | Long-lived inverse chirp signals from core collapse in massive scalar-tensor gravity | 43 | 50 | 50 | |
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69 | 69 | | **58** | Spadaro | 2023 | Glitch systematics on the observation of massive black-hole binaries with LISA | 29 | 31 | 31 | |
70 | 70 | | **59** | Gerosa | 2023 | Efficient multi-timescale dynamics of precessing black-hole binaries | 28 | 31 | 31 | |
71 | 71 | | **60** | Sayeb | 2021 | Massive black hole binary inspiral and spin evolution in a cosmological framework | 31 | 29 | 31 | |
72 | | -| **61** | Mould | 2022 | Gravitational-wave population inference at past time infinity | 26 | 30 | 30 | |
73 | | -| **62** | Wong | 2019 | Machine-learning interpolation of population-synthesis simulations to interpret gravitational-wave observations: a case study | 25 | 30 | 30 | |
| 72 | +| **61** | Wong | 2019 | Machine-learning interpolation of population-synthesis simulations to interpret gravitational-wave observations: a case study | 25 | 31 | 31 | |
| 73 | +| **62** | Mould | 2022 | Gravitational-wave population inference at past time infinity | 26 | 30 | 30 | |
74 | 74 | | **63** | Baibhav | 2021 | Looking for the parents of LIGO's black holes | 28 | 29 | 29 | |
75 | 75 | | **64** | Chamberlain | 2019 | Frequency-domain waveform approximants capturing Doppler shifts | 27 | 29 | 29 | |
76 | 76 | | **65** | Fumagalli | 2024 | Residual eccentricity as a systematic uncertainty on the formation channels of binary black holes | 28 | 27 | 28 | |
77 | 77 | | **66** | Croon | 2026 | Can GW231123 have a stellar origin? | 26 | 24 | 26 | |
78 | | -| **67** | Fumagalli | 2023 | Spin-eccentricity interplay in merging binary black holes | 24 | 26 | 26 | |
79 | | -| **68** | Moore | 2021 | Population-informed priors in gravitational-wave astronomy | 26 | 26 | 26 | |
80 | | -| **69** | Rosca-Mead | 2020 | Structure of neutron stars in massive scalar-tensor gravity | 23 | 26 | 26 | |
81 | | -| **70** | Romero-Shaw | 2025 | GW200208_222617 as an eccentric black-hole binary merger: properties and astrophysical implications | 25 | 24 | 25 | |
82 | | -| **71** | Pacilio | 2024 | Flexible mapping of ringdown amplitudes for nonprecessing binary black holes | 22 | 25 | 25 | |
| 78 | +| **67** | Pacilio | 2024 | Flexible mapping of ringdown amplitudes for nonprecessing binary black holes | 22 | 26 | 26 | |
| 79 | +| **68** | Fumagalli | 2023 | Spin-eccentricity interplay in merging binary black holes | 23 | 26 | 26 | |
| 80 | +| **69** | Moore | 2021 | Population-informed priors in gravitational-wave astronomy | 26 | 26 | 26 | |
| 81 | +| **70** | Rosca-Mead | 2020 | Structure of neutron stars in massive scalar-tensor gravity | 23 | 26 | 26 | |
| 82 | +| **71** | Romero-Shaw | 2025 | GW200208_222617 as an eccentric black-hole binary merger: properties and astrophysical implications | 25 | 24 | 25 | |
83 | 83 | | **72** | Boschini | 2025 | Orbital eccentricity in general relativity from catastrophe theory | 22 | 24 | 24 | |
84 | 84 | | **73** | Sperhake | 2020 | Amplification of superkicks in black-hole binaries through orbital eccentricity | 24 | 24 | 24 | |
85 | 85 | | **74** | Zhao | 2017 | Nutational resonances, transitional precession, and precession-averaged evolution in binary black-hole systems | 21 | 23 | 23 | |
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91 | 91 | | **80** | Nealon | 2022 | The Bardeen-Petterson effect in accreting supermassive black-hole binaries: disc breaking and critical obliquity | 21 | 14 | 21 | |
92 | 92 | | **81** | Gangardt | 2021 | A taxonomy of black-hole binary spin precession and nutation | 17 | 20 | 20 | |
93 | 93 | | **82** | Varma | 2021 | Up-down instability of binary black holes in numerical relativity | 17 | 19 | 19 | |
94 | | -| **83** | Gerosa | 2020 | The Bardeen-Petterson effect in accreting supermassive black-hole binaries: a systematic approach | 19 | 18 | 19 | |
95 | | -| **84** | Nobili | 2025 | Ringdown mode amplitudes of precessing binary black holes | 17 | 18 | 18 | |
| 94 | +| **83** | Nobili | 2025 | Ringdown mode amplitudes of precessing binary black holes | 17 | 18 | 18 | |
| 95 | +| **84** | Gerosa | 2020 | The Bardeen-Petterson effect in accreting supermassive black-hole binaries: a systematic approach | 18 | 18 | 18 | |
96 | 96 | | **85** | Buscicchio | 2025 | A test for LISA foreground Gaussianity and stationarity. I. Galactic white-dwarf binaries | 17 | 17 | 17 | |
97 | 97 | | **86** | Boschini | 2023 | Extending black-hole remnant surrogate models to extreme mass ratios | 16 | 17 | 17 | |
98 | 98 | | **87** | Mould | 2023 | One to many: comparing single gravitational-wave events to astrophysical populations | 14 | 16 | 16 | |
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207 | 207 | <br><br> |
208 | | -*Last updated: 2026-03-17 01:01:12 UTC* |
| 208 | +*Last updated: 2026-03-17 20:56:07 UTC* |
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