| 1 |
Berti |
2015 |
Testing general relativity with present and future astrophysical observations |
1569 |
1768 |
1768 |
| 2 |
Barack |
2019 |
Black holes, gravitational waves and fundamental physics: a roadmap |
937 |
1035 |
1035 |
| 3 |
Amaro-Seoane |
2022 |
Astrophysics with the Laser Interferometer Space Antenna |
964 |
848 |
964 |
| 4 |
Varma |
2019 |
Surrogate models for precessing binary black hole simulations with unequal masses |
533 |
550 |
550 |
| 5 |
Belczynski |
2020 |
Evolutionary roads leading to low effective spins, high black hole masses, and O1/O2 rates for LIGO/Virgo binary black holes |
497 |
530 |
530 |
| 6 |
Barausse |
2020 |
Prospects for fundamental physics with LISA |
443 |
502 |
502 |
| 7 |
Arun |
2022 |
New horizons for fundamental physics with LISA |
375 |
439 |
439 |
| 8 |
Gerosa |
2017 |
Are merging black holes born from stellar collapse or previous mergers? |
366 |
398 |
398 |
| 9 |
Gerosa |
2021 |
Hierarchical mergers of stellar-mass black holes and their gravitational-wave signatures |
336 |
366 |
366 |
| 10 |
Gerosa |
2018 |
Spin orientations of merging black holes formed from the evolution of stellar binaries |
237 |
272 |
272 |
| 11 |
Afshordi |
2025 |
Waveform modelling for the Laser Interferometer Space Antenna |
210 |
244 |
244 |
| 12 |
Varma |
2019 |
High-accuracy mass, spin, and recoil predictions of generic black-hole merger remnants |
157 |
180 |
180 |
| 13 |
Gerosa |
2015 |
Multi-timescale analysis of phase transitions in precessing black-hole binaries |
144 |
174 |
174 |
| 14 |
Vitale |
2020 |
Inferring the properties of a population of compact binaries in presence of selection effects |
157 |
169 |
169 |
| 15 |
Gerosa |
2013 |
Resonant-plane locking and spin alignment in stellar-mass black-hole binaries: a diagnostic of compact-binary formation |
149 |
167 |
167 |
| 16 |
Islam |
2021 |
Eccentric binary black hole surrogate models for the gravitational waveform and remnant properties: comparable mass, nonspinning case |
142 |
154 |
154 |
| 17 |
Ng |
2018 |
Gravitational-wave astrophysics with effective-spin measurements: asymmetries and selection biases |
126 |
142 |
142 |
| 18 |
Kesden |
2015 |
Effective potentials and morphological transitions for binary black-hole spin precession |
116 |
140 |
140 |
| 19 |
Baibhav |
2019 |
Gravitational-wave detection rates for compact binaries formed in isolation: LIGO/Virgo O3 and beyond |
115 |
133 |
133 |
| 20 |
Gerosa |
2019 |
Escape speed of stellar clusters from multiple-generation black-hole mergers in the upper mass gap |
117 |
128 |
128 |
| 21 |
Gerosa |
2019 |
Multiband gravitational-wave event rates and stellar physics |
114 |
126 |
126 |
| 22 |
Romero-Shaw |
2023 |
Eccentricity or spin precession? Distinguishing subdominant effects in gravitational-wave data |
108 |
119 |
119 |
| 23 |
Wysocki |
2018 |
Explaining LIGO’s observations via isolated binary evolution with natal kicks |
108 |
116 |
116 |
| 24 |
Gerosa |
2016 |
PRECESSION: Dynamics of spinning black-hole binaries with python |
98 |
112 |
112 |
| 25 |
Baibhav |
2020 |
The mass gap, the spin gap, and the origin of merging binary black holes |
94 |
109 |
109 |
| 26 |
Vitale |
2017 |
Impact of Bayesian priors on the characterization of binary black hole coalescences |
95 |
108 |
108 |
| 27 |
Taylor |
2018 |
Mining gravitational-wave catalogs to understand binary stellar evolution: a new hierarchical bayesian framework |
101 |
107 |
107 |
| 28 |
Moore |
2019 |
Are stellar-mass black-hole binaries too quiet for LISA? |
92 |
104 |
104 |
| 29 |
O’Shaughnessy |
2017 |
Inferences about supernova physics from gravitational-wave measurements: GW151226 spin misalignment as an indicator of strong black-hole natal kicks |
83 |
93 |
93 |
| 30 |
Gerosa |
2021 |
A generalized precession parameter \(\chi_\mathrm{p}\) to interpret gravitational-wave data |
78 |
91 |
91 |
| 31 |
Korol |
2020 |
Populations of double white dwarfs in Milky Way satellites and their detectability with LISA |
91 |
88 |
91 |
| 32 |
Bouffanais |
2019 |
Constraining the fraction of binary black holes formed in isolation and young star clusters with gravitational-wave data |
79 |
82 |
82 |
| 33 |
Horbatsch |
2015 |
Tensor-multi-scalar theories: relativistic stars and 3+1 decomposition |
74 |
78 |
78 |
| 34 |
Mould |
2022 |
Deep learning and Bayesian inference of gravitational-wave populations: hierarchical black-hole mergers |
68 |
74 |
74 |
| 35 |
Klein |
2022 |
The last three years: multiband gravitational-wave observations of stellar-mass binary black holes |
69 |
74 |
74 |
| 36 |
Gerosa |
2016 |
Black-hole kicks as new gravitational-wave observables |
67 |
73 |
73 |
| 37 |
Gerosa |
2018 |
Black-hole kicks from numerical-relativity surrogate models |
61 |
69 |
69 |
| 38 |
Mould |
2022 |
Which black hole formed first? Mass-ratio reversal in massive binary stars from gravitational-wave data |
56 |
67 |
67 |
| 39 |
Gupta |
2020 |
Black holes in the low mass gap: Implications for gravitational wave observations |
61 |
67 |
67 |
| 40 |
Buscicchio |
2021 |
Bayesian parameter estimation of stellar-mass black-hole binaries with LISA |
60 |
66 |
66 |
| 41 |
Gerosa |
2016 |
Numerical simulations of stellar collapse in scalar-tensor theories of gravity |
53 |
64 |
64 |
| 42 |
Gerosa |
2015 |
Precessional instability in binary black holes with aligned spins |
57 |
64 |
64 |
| 43 |
Gerosa |
2020 |
Astrophysical implications of GW190412 as a remnant of a previous black-hole merger |
58 |
63 |
63 |
| 44 |
Gangardt |
2024 |
pAGN: the one-stop solution for AGN disc modeling |
62 |
58 |
62 |
| 45 |
Gerosa |
2015 |
Spin alignment and differential accretion in merging black hole binaries |
61 |
54 |
61 |
| 46 |
Gerosa |
2014 |
Distinguishing black-hole spin-orbit resonances by their gravitational-wave signatures |
49 |
60 |
60 |
| 47 |
Moore |
2021 |
Testing general relativity with gravitational-wave catalogs: the insidious nature of waveform systematics |
47 |
57 |
57 |
| 48 |
Sperhake |
2017 |
Long-lived inverse chirp signals from core collapse in massive scalar-tensor gravity |
49 |
55 |
55 |
| 49 |
Roebber |
2020 |
Milky Way satellites shining bright in gravitational waves |
48 |
54 |
54 |
| 50 |
Santini |
2023 |
Black-hole mergers in disk-like environments could explain the observed \(q-\chi_\mathrm{eff}\) correlation |
50 |
51 |
51 |
| 51 |
Gerosa |
2020 |
Gravitational-wave selection effects using neural-network classifiers |
45 |
51 |
51 |
| 52 |
Gerosa |
2015 |
Missing black holes in brightest cluster galaxies as evidence for the occurrence of superkicks in nature |
45 |
49 |
49 |
| 53 |
Romero-Shaw |
2025 |
GW200208_222617 as an eccentric black-hole binary merger: properties and astrophysical implications |
48 |
45 |
48 |
| 54 |
Tso |
2019 |
Optimizing LIGO with LISA forewarnings to improve black-hole spectroscopy |
38 |
44 |
44 |
| 55 |
Croon |
2026 |
Can GW231123 have a stellar origin? |
43 |
42 |
43 |
| 56 |
Trifirò |
2016 |
Distinguishing black-hole spin-orbit resonances by their gravitational wave signatures. II: Full parameter estimation |
35 |
43 |
43 |
| 57 |
Lodato |
2013 |
Black hole mergers: do gas discs lead to spin alignment? |
40 |
41 |
41 |
| 58 |
Spadaro |
2023 |
Glitch systematics on the observation of massive black-hole binaries with LISA |
34 |
39 |
39 |
| 59 |
Gerosa |
2023 |
Efficient multi-timescale dynamics of precessing black-hole binaries |
34 |
38 |
38 |
| 60 |
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 |
35 |
38 |
38 |
| 61 |
Sayeb |
2021 |
Massive black hole binary inspiral and spin evolution in a cosmological framework |
38 |
35 |
38 |
| 62 |
Rosca-Mead |
2020 |
Core collapse in massive scalar-tensor gravity |
31 |
38 |
38 |
| 63 |
Mancarella |
2025 |
Sampling the full hierarchical population posterior distribution in gravitational-wave astronomy |
30 |
36 |
36 |
| 64 |
Pacilio |
2024 |
Flexible mapping of ringdown amplitudes for nonprecessing binary black holes |
31 |
35 |
35 |
| 65 |
Fumagalli |
2024 |
Residual eccentricity as a systematic uncertainty on the formation channels of binary black holes |
33 |
34 |
34 |
| 66 |
Baibhav |
2021 |
Looking for the parents of LIGO’s black holes |
33 |
34 |
34 |
| 67 |
Wong |
2019 |
Machine-learning interpolation of population-synthesis simulations to interpret gravitational-wave observations: a case study |
28 |
33 |
33 |
| 68 |
Chamberlain |
2019 |
Frequency-domain waveform approximants capturing Doppler shifts |
31 |
33 |
33 |
| 69 |
Fumagalli |
2023 |
Spin-eccentricity interplay in merging binary black holes |
27 |
32 |
32 |
| 70 |
Mould |
2022 |
Gravitational-wave population inference at past time infinity |
28 |
32 |
32 |
| 71 |
Moore |
2021 |
Population-informed priors in gravitational-wave astronomy |
31 |
30 |
31 |
| 72 |
Rosca-Mead |
2020 |
Structure of neutron stars in massive scalar-tensor gravity |
26 |
29 |
29 |
| 73 |
Boschini |
2025 |
Orbital eccentricity in general relativity from catastrophe theory |
25 |
28 |
28 |
| 74 |
Sperhake |
2020 |
Amplification of superkicks in black-hole binaries through orbital eccentricity |
27 |
28 |
28 |
| 75 |
Pedrotti |
2026 |
Cosmology with the angular cross-correlation of gravitational-wave and galaxy catalogs: forecasts for next-generation interferometers and the Euclid survey |
26 |
27 |
27 |
| 76 |
Zhao |
2017 |
Nutational resonances, transitional precession, and precession-averaged evolution in binary black-hole systems |
25 |
27 |
27 |
| 77 |
Buscicchio |
2025 |
Test for LISA foreground Gaussianity and stationarity: galactic white-dwarf binaries |
24 |
26 |
26 |
| 78 |
Gangardt |
2021 |
A taxonomy of black-hole binary spin precession and nutation |
20 |
26 |
26 |
| 79 |
Mancarella |
2023 |
Inferring, not just detecting: metrics for high-redshift sources observed with third-generation gravitational-wave detectors |
19 |
25 |
25 |
| 80 |
Nealon |
2022 |
The Bardeen-Petterson effect in accreting supermassive black-hole binaries: disc breaking and critical obliquity |
25 |
19 |
25 |
| 81 |
Gerosa |
2019 |
Wide nutation: binary black-hole spins repeatedly oscillating from full alignment to full anti-alignment |
22 |
25 |
25 |
| 82 |
Varma |
2021 |
Up-down instability of binary black holes in numerical relativity |
18 |
23 |
23 |
| 83 |
Mould |
2020 |
Endpoint of the up-down instability in precessing binary black holes |
19 |
23 |
23 |
| 84 |
Gerosa |
2017 |
On the equal-mass limit of precessing black-hole binaries |
19 |
23 |
23 |
| 85 |
Nobili |
2025 |
Ringdown mode amplitudes of precessing binary black holes |
21 |
22 |
22 |
| 86 |
Tenorio |
2025 |
Scalable data-analysis framework for long-duration gravitational waves from compact binaries using short Fourier transforms |
20 |
21 |
21 |
| 87 |
Gerosa |
2024 |
Quick recipes for gravitational-wave selection effects |
21 |
21 |
21 |
| 88 |
Boschini |
2023 |
Extending black-hole remnant surrogate models to extreme mass ratios |
17 |
20 |
20 |
| 89 |
Gerosa |
2020 |
The Bardeen-Petterson effect in accreting supermassive black-hole binaries: a systematic approach |
20 |
20 |
20 |
| 90 |
Stegmann |
2025 |
Distinguishing the origin of eccentric black-hole mergers with gravitational-wave spin measurements |
18 |
19 |
19 |
| 91 |
Pacilio |
2024 |
Catalog variance of testing general relativity with gravitational-wave data |
17 |
19 |
19 |
| 92 |
Cole |
2026 |
Sequential simulation-based inference for extreme mass ratio inspirals |
18 |
18 |
18 |
| 93 |
Mould |
2023 |
One to many: comparing single gravitational-wave events to astrophysical populations |
17 |
18 |
18 |
| 94 |
Fumagalli |
2025 |
Non-adiabatic dynamics of eccentric black-hole binaries in post-Newtonian theory |
14 |
17 |
17 |
| 95 |
Mould |
2024 |
Calibrating signal-to-noise ratio detection thresholds using gravitational-wave catalogs |
15 |
16 |
16 |
| 96 |
Gerosa |
2017 |
filltex: Automatic queries to ADS and INSPIRE databases to fill LaTex bibliography |
13 |
16 |
16 |
| 97 |
Steinle |
2023 |
The Bardeen-Petterson effect, disk breaking, and the spin orientations of supermassive black-hole binaries |
12 |
15 |
15 |
| 98 |
Speri |
2026 |
Single-harmonic search for extreme mass-ratio inspirals |
14 |
14 |
14 |
| 99 |
Tenorio |
2025 |
Where did heavy binaries go? Gravitational-wave populations using Delaunay triangulation with optimized complexity |
14 |
14 |
14 |
| 100 |
Gangardt |
2022 |
Constraining black-hole binary spin precession and nutation with sequential prior conditioning |
12 |
14 |
14 |
| 101 |
Reali |
2020 |
Mapping the asymptotic inspiral of precessing binary black holes to their merger remnants |
11 |
14 |
14 |
| 102 |
Fabbri |
2025 |
Reconstructing parametric gravitational-wave population fits from non-parametric results without refitting the data |
13 |
13 |
13 |
| 103 |
De Renzis |
2025 |
Forecasting the population properties of merging black holes |
13 |
13 |
13 |
| 104 |
Santoliquido |
2024 |
Classifying binary black holes from Population III stars with the Einstein Telescope: a machine-learning approach |
12 |
13 |
13 |
| 105 |
Toubiana |
2026 |
Comparing astrophysical models to gravitational-wave data in the observable space |
12 |
12 |
12 |
| 106 |
Spadaro |
2025 |
Stars or gas? Constraining the hardening processes of massive black-hole binaries with LISA |
11 |
12 |
12 |
| 107 |
De Renzis |
2022 |
Characterization of merging black holes with two precessing spins |
9 |
12 |
12 |
| 108 |
Gerosa |
2025 |
Which is which? Identification of the two compact objects in gravitational-wave binaries |
10 |
11 |
11 |
| 109 |
Kritos |
2024 |
Minimum gas mass accreted by spinning intermediate-mass black holes in stellar clusters |
8 |
11 |
11 |
| 110 |
Mould |
2026 |
Gravitational-wave astronomy requires population-informed parameter estimation |
7 |
9 |
9 |
| 111 |
De Renzis |
2023 |
Parameter estimation of binary black holes in the endpoint of the up-down instability |
4 |
9 |
9 |
| 112 |
Corelli |
2026 |
Variance of gravitational-wave populations |
8 |
8 |
8 |
| 113 |
Tenorio |
2026 |
Exceptionality of exceptional gravitational-wave events |
8 |
8 |
8 |
| 114 |
Steinle |
2024 |
Probing AGN jet precession with LISA |
8 |
4 |
8 |
| 115 |
Boschini |
2025 |
“LHS in LHS”: a new expansion strategy for Latin hypercube sampling in simulation design |
7 |
2 |
7 |
| 116 |
Spadaro |
2026 |
Accurate and efficient simulation-based inference for massive black-hole binaries with LISA |
5 |
6 |
6 |
| 117 |
Chiaberge |
2025 |
A recoiling supermassive black hole in a powerful quasar |
5 |
6 |
6 |
| 118 |
Giarda |
2025 |
Accelerated inference of binary black-hole populations from the stochastic gravitational-wave background |
6 |
5 |
6 |
| 119 |
Boschini |
2024 |
Astrophysical and relativistic modeling of the recoiling black-hole candidate in quasar 3C 186 |
6 |
4 |
6 |
| 120 |
Gerosa |
2022 |
The irreducible mass and the horizon area of LIGO’s black holes |
6 |
6 |
6 |
| 121 |
Dabrowny |
2021 |
Modeling the outcome of supernova explosions in binary population synthesis using the stellar compactness |
5 |
6 |
6 |
| 122 |
Varma |
2019 |
The binary black hole explorer: on-the-fly visualizations of precessing binary black holes |
4 |
6 |
6 |
| 123 |
Gerosa |
2018 |
Surprises from the spins: astrophysics and relativity with detections of spinning black-hole mergers |
4 |
5 |
5 |
| 124 |
De Santi |
2026 |
Inferring the population properties of galactic binaries from LISA’s stochastic foreground |
2 |
4 |
4 |
| 125 |
Gerosa |
2023 |
QLUSTER: quick clusters of merging binary black holes |
4 |
0 |
4 |
| 126 |
Borhanian |
2026 |
Impact of facility timing and coordination for next-generation gravitational-wave detectors |
1 |
2 |
2 |
| 127 |
Tornotti |
2025 |
Bayesian luminosity function estimation in multidepth datasets with selection effects: a case study for \(3<z<5\) Lyman \(\alpha\) emitters |
2 |
1 |
2 |
| 128 |
Gerosa |
2018 |
Reanalysis of LIGO black-hole coalescences with alternative prior assumptions |
2 |
2 |
2 |
| 129 |
Dossena |
2026 |
Not all spins of black-hole binaries formed in clusters are isotropic and not all spins of black-hole binaries formed in isolation are aligned |
0 |
1 |
1 |
| 130 |
Anselmo |
2026 |
Black-hole ringdown with templates capturing spin precession: a reanalysis of GW190521 |
1 |
1 |
1 |
| 131 |
Loutrel |
2026 |
Probing modified gravitational-wave dispersion with bursts from eccentric black-hole binaries |
1 |
1 |
1 |
| 132 |
Fumagalli |
2026 |
PRECESSION 2.1: black-hole binary spin precession on eccentric orbits |
1 |
1 |
1 |
| 133 |
Gerosa |
2015 |
Rival families: waveforms from resonant black-hole binaries as probes of their astrophysical formation history |
0 |
1 |
1 |
| 134 |
Plunkett |
2026 |
Spinformation: do gravitational-wave events carry information beyond effective spins? |
0 |
0 |
0 |
| 135 |
Owen |
2026 |
Population-level correlations in Bayesian statistics: an illustrative model for gravitational-wave astronomy |
0 |
0 |
0 |
| 136 |
Leto di Priolo |
2026 |
Targeting black holes from metal-poor progenitors with next-generation gravitational-wave detectors |
0 |
0 |
0 |
| 137 |
Gerosa |
2025 |
Coincident morphological transitions in precessing black-hole binaries |
0 |
0 |
0 |
| 138 |
Gerosa |
2016 |
Source modelling at the dawn of gravitational-wave astronomy |
0 |
0 |
0 |
| 139 |
Gerosa |
2014 |
Spin alignment effects in black hole binaries |
0 |
0 |
0 |
