Skip to content

Commit 2dde7c2

Browse files
committed
Generic update
1 parent 585db81 commit 2dde7c2

File tree

4 files changed

+25
-25
lines changed

4 files changed

+25
-25
lines changed

_citations.md

Lines changed: 22 additions & 22 deletions
Original file line numberDiff line numberDiff line change
@@ -1,49 +1,49 @@
11
## Citation Summary
22

3-
- **Total ADS citations**: 9732
3+
- **Total ADS citations**: 9747
44
- **Total INSPIRE citations**: 10604
5-
- **Total MAX citations**: 10684
5+
- **Total MAX citations**: 10686
66
- **h-index**: 47
77

88
## Paper list sorted by citation count
99

1010
| # | Author | Year | Title | ADS | INSPIRE | MAX |
1111
|---|--------|------|-------|-----|---------|-----|
12-
| **1** | Berti | 2015 | Testing general relativity with present and future astrophysical observations | 1421 | 1589 | 1589 |
12+
| **1** | Berti | 2015 | Testing general relativity with present and future astrophysical observations | 1422 | 1589 | 1589 |
1313
| **2** | Barack | 2019 | Black holes, gravitational waves and fundamental physics: a roadmap | 842 | 930 | 930 |
1414
| **3** | Amaro-Seoane | 2022 | Astrophysics with the Laser Interferometer Space Antenna | 742 | 692 | 742 |
1515
| **4** | Belczynski | 2020 | Evolutionary roads leading to low effective spins, high black hole masses, and O1/O2 rates for LIGO/Virgo binary black holes | 456 | 473 | 473 |
1616
| **5** | Varma | 2019 | Surrogate models for precessing binary black hole simulations with unequal masses | 433 | 450 | 450 |
1717
| **6** | Barausse | 2020 | Prospects for fundamental physics with LISA | 390 | 439 | 439 |
1818
| **7** | Arun | 2022 | New horizons for fundamental physics with LISA | 305 | 355 | 355 |
1919
| **8** | Gerosa | 2017 | Are merging black holes born from stellar collapse or previous mergers? | 331 | 355 | 355 |
20-
| **9** | Gerosa | 2021 | Hierarchical mergers of stellar-mass black holes and their gravitational-wave signatures | 264 | 282 | 282 |
20+
| **9** | Gerosa | 2021 | Hierarchical mergers of stellar-mass black holes and their gravitational-wave signatures | 265 | 282 | 282 |
2121
| **10** | Gerosa | 2018 | Spin orientations of merging black holes formed from the evolution of stellar binaries | 215 | 236 | 236 |
2222
| **11** | Afshordi | 2025 | Waveform modelling for the Laser Interferometer Space Antenna | 144 | 174 | 174 |
2323
| **12** | Gerosa | 2015 | Multi-timescale analysis of phase transitions in precessing black-hole binaries | 139 | 162 | 162 |
2424
| **13** | Varma | 2019 | High-accuracy mass, spin, and recoil predictions of generic black-hole merger remnants | 142 | 159 | 159 |
2525
| **14** | Gerosa | 2013 | Resonant-plane locking and spin alignment in stellar-mass black-hole binaries: a diagnostic of compact-binary formation | 143 | 158 | 158 |
26-
| **15** | Islam | 2021 | Eccentric binary black hole surrogate models for the gravitational waveform and remnant properties: comparable mass, nonspinning case | 127 | 139 | 139 |
27-
| **16** | Vitale | 2020 | Inferring the properties of a population of compact binaries in presence of selection effects | 129 | 138 | 138 |
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+
| **16** | Vitale | 2020 | Inferring the properties of a population of compact binaries in presence of selection effects | 130 | 138 | 138 |
2828
| **17** | Kesden | 2015 | Effective potentials and morphological transitions for binary black-hole spin precession | 115 | 137 | 137 |
2929
| **18** | Ng | 2018 | Gravitational-wave astrophysics with effective-spin measurements: asymmetries and selection biases | 115 | 127 | 127 |
3030
| **19** | Baibhav | 2019 | Gravitational-wave detection rates for compact binaries formed in isolation: LIGO/Virgo O3 and beyond | 108 | 125 | 125 |
31-
| **20** | Gerosa | 2019 | Multiband gravitational-wave event rates and stellar physics | 109 | 121 | 121 |
31+
| **20** | Gerosa | 2019 | Multiband gravitational-wave event rates and stellar physics | 110 | 121 | 121 |
3232
| **21** | Gerosa | 2019 | Escape speed of stellar clusters from multiple-generation black-hole mergers in the upper mass gap | 110 | 119 | 119 |
33-
| **22** | Gerosa | 2016 | PRECESSION: Dynamics of spinning black-hole binaries with python | 92 | 102 | 102 |
33+
| **22** | Gerosa | 2016 | PRECESSION: Dynamics of spinning black-hole binaries with python | 93 | 102 | 102 |
3434
| **23** | Moore | 2019 | Are stellar-mass black-hole binaries too quiet for LISA? | 89 | 101 | 101 |
35-
| **24** | Wysocki | 2018 | Explaining LIGO's observations via isolated binary evolution with natal kicks | 96 | 101 | 101 |
35+
| **24** | Wysocki | 2018 | Explaining LIGO's observations via isolated binary evolution with natal kicks | 97 | 101 | 101 |
3636
| **25** | Vitale | 2017 | Impact of Bayesian priors on the characterization of binary black hole coalescences | 86 | 99 | 99 |
3737
| **26** | Taylor | 2018 | Mining gravitational-wave catalogs to understand binary stellar evolution: a new hierarchical bayesian framework | 92 | 97 | 97 |
3838
| **27** | Romero-Shaw | 2023 | Eccentricity or spin precession? Distinguishing subdominant effects in gravitational-wave data | 82 | 96 | 96 |
39-
| **28** | Baibhav | 2020 | The mass gap, the spin gap, and the origin of merging binary black holes | 79 | 92 | 92 |
39+
| **28** | Baibhav | 2020 | The mass gap, the spin gap, and the origin of merging binary black holes | 80 | 92 | 92 |
4040
| **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 |
4141
| **30** | Gerosa | 2021 | A generalized precession parameter $$\chi_\mathrm{p}$$ to interpret gravitational-wave data | 68 | 79 | 79 |
4242
| **31** | Bouffanais | 2019 | Constraining the fraction of binary black holes formed in isolation and young star clusters with gravitational-wave data | 76 | 78 | 78 |
4343
| **32** | Korol | 2020 | Populations of double white dwarfs in Milky Way satellites and their detectability with LISA | 76 | 76 | 76 |
4444
| **33** | Horbatsch | 2015 | Tensor-multi-scalar theories: relativistic stars and 3+1 decomposition | 70 | 74 | 74 |
4545
| **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 | 61 | 67 | 67 |
46+
| **35** | Gerosa | 2016 | Black-hole kicks as new gravitational-wave observables | 62 | 67 | 67 |
4747
| **36** | Buscicchio | 2021 | Bayesian parameter estimation of stellar-mass black-hole binaries with LISA | 55 | 64 | 64 |
4848
| **37** | Gupta | 2020 | Black holes in the low mass gap: Implications for gravitational wave observations | 59 | 64 | 64 |
4949
| **38** | Gerosa | 2018 | Black-hole kicks from numerical-relativity surrogate models | 56 | 62 | 62 |
@@ -53,12 +53,12 @@
5353
| **42** | Gerosa | 2014 | Distinguishing black-hole spin-orbit resonances by their gravitational-wave signatures | 47 | 57 | 57 |
5454
| **43** | Mould | 2022 | Deep learning and Bayesian inference of gravitational-wave populations: hierarchical black-hole mergers | 52 | 56 | 56 |
5555
| **44** | Gerosa | 2015 | Spin alignment and differential accretion in merging black hole binaries | 55 | 50 | 55 |
56-
| **45** | Mould | 2022 | Which black hole formed first? Mass-ratio reversal in massive binary stars from gravitational-wave data | 46 | 53 | 53 |
56+
| **45** | Mould | 2022 | Which black hole formed first? Mass-ratio reversal in massive binary stars from gravitational-wave data | 47 | 53 | 53 |
5757
| **46** | Roebber | 2020 | Milky Way satellites shining bright in gravitational waves | 44 | 50 | 50 |
5858
| **47** | Sperhake | 2017 | Long-lived inverse chirp signals from core collapse in massive scalar-tensor gravity | 43 | 50 | 50 |
5959
| **48** | Gerosa | 2015 | Missing black holes in brightest cluster galaxies as evidence for the occurrence of superkicks in nature | 41 | 47 | 47 |
6060
| **49** | Moore | 2021 | Testing general relativity with gravitational-wave catalogs: the insidious nature of waveform systematics | 41 | 46 | 46 |
61-
| **50** | Gangardt | 2024 | pAGN: the one-stop solution for AGN disc modeling | 43 | 45 | 45 |
61+
| **50** | Gangardt | 2024 | pAGN: the one-stop solution for AGN disc modeling | 44 | 45 | 45 |
6262
| **51** | Tso | 2019 | Optimizing LIGO with LISA forewarnings to improve black-hole spectroscopy | 37 | 43 | 43 |
6363
| **52** | Trifiro' | 2016 | Distinguishing black-hole spin-orbit resonances by their gravitational wave signatures. II: Full parameter estimation | 34 | 42 | 42 |
6464
| **53** | Gerosa | 2020 | Gravitational-wave selection effects using neural-network classifiers | 37 | 41 | 41 |
@@ -70,17 +70,17 @@
7070
| **59** | Sayeb | 2021 | Massive black hole binary inspiral and spin evolution in a cosmological framework | 31 | 29 | 31 |
7171
| **60** | Mould | 2022 | Gravitational-wave population inference at past time infinity | 26 | 30 | 30 |
7272
| **61** | Wong | 2019 | Machine-learning interpolation of population-synthesis simulations to interpret gravitational-wave observations: a case study | 25 | 30 | 30 |
73-
| **62** | Spadaro | 2023 | Glitch systematics on the observation of massive black-hole binaries with LISA | 25 | 28 | 28 |
74-
| **63** | Baibhav | 2021 | Looking for the parents of LIGO's black holes | 28 | 28 | 28 |
75-
| **64** | Chamberlain | 2019 | Frequency-domain waveform approximants capturing Doppler shifts | 26 | 28 | 28 |
76-
| **65** | Fumagalli | 2024 | Residual eccentricity as a systematic uncertainty on the formation channels of binary black holes | 27 | 27 | 27 |
73+
| **62** | Fumagalli | 2024 | Residual eccentricity as a systematic uncertainty on the formation channels of binary black holes | 28 | 27 | 28 |
74+
| **63** | Spadaro | 2023 | Glitch systematics on the observation of massive black-hole binaries with LISA | 25 | 28 | 28 |
75+
| **64** | Baibhav | 2021 | Looking for the parents of LIGO's black holes | 28 | 28 | 28 |
76+
| **65** | Chamberlain | 2019 | Frequency-domain waveform approximants capturing Doppler shifts | 26 | 28 | 28 |
7777
| **66** | Rosca-Mead | 2020 | Structure of neutron stars in massive scalar-tensor gravity | 23 | 26 | 26 |
78-
| **67** | Pacilio | 2024 | Flexible mapping of ringdown amplitudes for nonprecessing binary black holes | 21 | 25 | 25 |
79-
| **68** | Fumagalli | 2023 | Spin-eccentricity interplay in merging binary black holes | 22 | 25 | 25 |
80-
| **69** | Croon | 2025 | Can GW231123 have a stellar origin? | 24 | 23 | 24 |
78+
| **67** | Croon | 2025 | Can GW231123 have a stellar origin? | 25 | 23 | 25 |
79+
| **68** | Pacilio | 2024 | Flexible mapping of ringdown amplitudes for nonprecessing binary black holes | 21 | 25 | 25 |
80+
| **69** | Fumagalli | 2023 | Spin-eccentricity interplay in merging binary black holes | 23 | 25 | 25 |
8181
| **70** | Boschini | 2025 | Orbital eccentricity in general relativity from catastrophe theory | 22 | 24 | 24 |
8282
| **71** | Moore | 2021 | Population-informed priors in gravitational-wave astronomy | 24 | 23 | 24 |
83-
| **72** | Sperhake | 2020 | Amplification of superkicks in black-hole binaries through orbital eccentricity | 21 | 23 | 23 |
83+
| **72** | Sperhake | 2020 | Amplification of superkicks in black-hole binaries through orbital eccentricity | 22 | 23 | 23 |
8484
| **73** | Zhao | 2017 | Nutational resonances, transitional precession, and precession-averaged evolution in binary black-hole systems | 21 | 23 | 23 |
8585
| **74** | Gerosa | 2017 | On the equal-mass limit of precessing black-hole binaries | 19 | 23 | 23 |
8686
| **75** | Mould | 2020 | Endpoint of the up-down instability in precessing binary black holes | 18 | 22 | 22 |
@@ -203,4 +203,4 @@
203203

204204

205205
<br><br>
206-
*Last updated: 2026-02-08 01:01:21 UTC*
206+
*Last updated: 2026-02-09 01:01:32 UTC*

_group.md

Lines changed: 1 addition & 1 deletion
Original file line numberDiff line numberDiff line change
@@ -259,4 +259,4 @@ Here are the amazing students who are currently completing research projects wit
259259

260260

261261
<br><br>
262-
*Last updated: 2026-02-08 01:01:21 UTC*
262+
*Last updated: 2026-02-09 01:01:32 UTC*

_publications.md

Lines changed: 1 addition & 1 deletion
Original file line numberDiff line numberDiff line change
@@ -690,4 +690,4 @@ E. Berti, et al. (53 authors incl. **D. Gerosa**).\
690690

691691

692692
<br><br>
693-
*Last updated: 2026-02-08 01:01:21 UTC*
693+
*Last updated: 2026-02-09 01:01:32 UTC*

_talks.md

Lines changed: 1 addition & 1 deletion
Original file line numberDiff line numberDiff line change
@@ -549,4 +549,4 @@ Liceo Candia and Liceo Frassati, Seregno, Italy, Jan 2018.
549549

550550

551551
<br><br>
552-
*Last updated: 2026-02-08 01:01:21 UTC*
552+
*Last updated: 2026-02-09 01:01:32 UTC*

0 commit comments

Comments
 (0)