Generic update

Author: dgerosa

_citations.md

@@ -1,49 +1,49 @@
 ## Citation Summary
 
-- **Total ADS citations**: 9704
-- **Total INSPIRE citations**: 10588
-- **Total MAX citations**: 10667
+- **Total ADS citations**: 9713
+- **Total INSPIRE citations**: 10594
+- **Total MAX citations**: 10675
 - **h-index**: 47
 
 ## Paper list sorted by citation count
 
 | # | Author | Year | Title | ADS | INSPIRE | MAX |
 |---|--------|------|-------|-----|---------|-----|
-| **1** | Berti | 2015 | Testing general relativity with present and future astrophysical observations | 1415 | 1588 | 1588 |
-| **2** | Barack | 2019 | Black holes, gravitational waves and fundamental physics: a roadmap | 838 | 928 | 928 |
-| **3** | Amaro-Seoane | 2022 | Astrophysics with the Laser Interferometer Space Antenna | 740 | 692 | 740 |
+| **1** | Berti | 2015 | Testing general relativity with present and future astrophysical observations | 1417 | 1588 | 1588 |
+| **2** | Barack | 2019 | Black holes, gravitational waves and fundamental physics: a roadmap | 839 | 928 | 928 |
+| **3** | Amaro-Seoane | 2022 | Astrophysics with the Laser Interferometer Space Antenna | 741 | 692 | 741 |
 | **4** | Belczynski | 2020 | Evolutionary roads leading to low effective spins, high black hole masses, and O1/O2 rates for LIGO/Virgo binary black holes | 455 | 473 | 473 |
-| **5** | Varma | 2019 | Surrogate models for precessing binary black hole simulations with unequal masses | 430 | 450 | 450 |
+| **5** | Varma | 2019 | Surrogate models for precessing binary black hole simulations with unequal masses | 432 | 450 | 450 |
 | **6** | Barausse | 2020 | Prospects for fundamental physics with LISA | 389 | 439 | 439 |
 | **7** | Gerosa | 2017 | Are merging black holes born from stellar collapse or previous mergers? | 331 | 355 | 355 |
-| **8** | Arun | 2022 | New horizons for fundamental physics with LISA | 301 | 354 | 354 |
-| **9** | Gerosa | 2021 | Hierarchical mergers of stellar-mass black holes and their gravitational-wave signatures | 263 | 280 | 280 |
+| **8** | Arun | 2022 | New horizons for fundamental physics with LISA | 302 | 354 | 354 |
+| **9** | Gerosa | 2021 | Hierarchical mergers of stellar-mass black holes and their gravitational-wave signatures | 264 | 281 | 281 |
 | **10** | Gerosa | 2018 | Spin orientations of merging black holes formed from the evolution of stellar binaries | 214 | 235 | 235 |
 | **11** | Afshordi | 2025 | Waveform modelling for the Laser Interferometer Space Antenna | 144 | 174 | 174 |
 | **12** | Gerosa | 2015 | Multi-timescale analysis of phase transitions in precessing black-hole binaries | 139 | 162 | 162 |
 | **13** | Varma | 2019 | High-accuracy mass, spin, and recoil predictions of generic black-hole merger remnants | 142 | 159 | 159 |
 | **14** | Gerosa | 2013 | Resonant-plane locking and spin alignment in stellar-mass black-hole binaries: a diagnostic of compact-binary formation | 143 | 158 | 158 |
-| **15** | Islam | 2021 | Eccentric binary black hole surrogate models for the gravitational waveform and remnant properties: comparable mass, nonspinning case | 127 | 138 | 138 |
+| **15** | Islam | 2021 | Eccentric binary black hole surrogate models for the gravitational waveform and remnant properties: comparable mass, nonspinning case | 127 | 139 | 139 |
 | **16** | Vitale | 2020 | Inferring the properties of a population of compact binaries in presence of selection effects | 129 | 138 | 138 |
 | **17** | Kesden | 2015 | Effective potentials and morphological transitions for binary black-hole spin precession | 115 | 137 | 137 |
 | **18** | Ng | 2018 | Gravitational-wave astrophysics with effective-spin measurements: asymmetries and selection biases | 115 | 127 | 127 |
 | **19** | Baibhav | 2019 | Gravitational-wave detection rates for compact binaries formed in isolation: LIGO/Virgo O3 and beyond | 108 | 125 | 125 |
 | **20** | Gerosa | 2019 | Multiband gravitational-wave event rates and stellar physics | 109 | 120 | 120 |
 | **21** | Gerosa | 2019 | Escape speed of stellar clusters from multiple-generation black-hole mergers in the upper mass gap | 110 | 119 | 119 |
-| **22** | Moore | 2019 | Are stellar-mass black-hole binaries too quiet for LISA? | 89 | 101 | 101 |
-| **23** | Wysocki | 2018 | Explaining LIGO's observations via isolated binary evolution with natal kicks | 96 | 101 | 101 |
-| **24** | Gerosa | 2016 | PRECESSION: Dynamics of spinning black-hole binaries with python | 92 | 101 | 101 |
+| **22** | Gerosa | 2016 | PRECESSION: Dynamics of spinning black-hole binaries with python | 92 | 102 | 102 |
+| **23** | Moore | 2019 | Are stellar-mass black-hole binaries too quiet for LISA? | 89 | 101 | 101 |
+| **24** | Wysocki | 2018 | Explaining LIGO's observations via isolated binary evolution with natal kicks | 96 | 101 | 101 |
 | **25** | Vitale | 2017 | Impact of Bayesian priors on the characterization of binary black hole coalescences | 86 | 99 | 99 |
 | **26** | Taylor | 2018 | Mining gravitational-wave catalogs to understand binary stellar evolution: a new hierarchical bayesian framework | 92 | 97 | 97 |
 | **27** | Romero-Shaw | 2023 | Eccentricity or spin precession? Distinguishing subdominant effects in gravitational-wave data | 82 | 96 | 96 |
-| **28** | Baibhav | 2020 | The mass gap, the spin gap, and the origin of merging binary black holes | 79 | 91 | 91 |
+| **28** | Baibhav | 2020 | The mass gap, the spin gap, and the origin of merging binary black holes | 79 | 92 | 92 |
 | **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 |
 | **30** | Gerosa | 2021 | A generalized precession parameter $$\chi_\mathrm{p}$$ to interpret gravitational-wave data | 67 | 79 | 79 |
 | **31** | Bouffanais | 2019 | Constraining the fraction of binary black holes formed in isolation and young star clusters with gravitational-wave data | 76 | 78 | 78 |
 | **32** | Korol | 2020 | Populations of double white dwarfs in Milky Way satellites and their detectability with LISA | 76 | 76 | 76 |
 | **33** | Horbatsch | 2015 | Tensor-multi-scalar theories: relativistic stars and 3+1 decomposition | 70 | 74 | 74 |
 | **34** | Klein | 2022 | The last three years: multiband gravitational-wave observations of stellar-mass binary black holes | 61 | 68 | 68 |
-| **35** | Gerosa | 2016 | Black-hole kicks as new gravitational-wave observables | 61 | 66 | 66 |
+| **35** | Gerosa | 2016 | Black-hole kicks as new gravitational-wave observables | 61 | 67 | 67 |
 | **36** | Buscicchio | 2021 | Bayesian parameter estimation of stellar-mass black-hole binaries with LISA | 55 | 64 | 64 |
 | **37** | Gupta | 2020 | Black holes in the low mass gap: Implications for gravitational wave observations | 59 | 64 | 64 |
 | **38** | Gerosa | 2018 | Black-hole kicks from numerical-relativity surrogate models | 56 | 62 | 62 |
@@ -58,7 +58,7 @@
 | **47** | Sperhake | 2017 | Long-lived inverse chirp signals from core collapse in massive scalar-tensor gravity | 43 | 50 | 50 |
 | **48** | Gerosa | 2015 | Missing black holes in brightest cluster galaxies as evidence for the occurrence of superkicks in nature | 41 | 47 | 47 |
 | **49** | Moore | 2021 | Testing general relativity with gravitational-wave catalogs: the insidious nature of waveform systematics | 41 | 46 | 46 |
-| **50** | Gangardt | 2024 | pAGN: the one-stop solution for AGN disc modeling | 43 | 44 | 44 |
+| **50** | Gangardt | 2024 | pAGN: the one-stop solution for AGN disc modeling | 43 | 45 | 45 |
 | **51** | Tso | 2019 | Optimizing LIGO with LISA forewarnings to improve black-hole spectroscopy | 37 | 43 | 43 |
 | **52** | Trifiro' | 2016 | Distinguishing black-hole spin-orbit resonances by their gravitational wave signatures. II: Full parameter estimation | 34 | 42 | 42 |
 | **53** | Gerosa | 2020 | Gravitational-wave selection effects using neural-network classifiers | 37 | 41 | 41 |
@@ -76,14 +76,14 @@
 | **65** | Fumagalli | 2024 | Residual eccentricity as a systematic uncertainty on the formation channels of binary black holes | 27 | 26 | 27 |
 | **66** | Rosca-Mead | 2020 | Structure of neutron stars in massive scalar-tensor gravity | 23 | 26 | 26 |
 | **67** | Pacilio | 2024 | Flexible mapping of ringdown amplitudes for nonprecessing binary black holes | 21 | 25 | 25 |
-| **68** | Croon | 2025 | Can GW231123 have a stellar origin? | 23 | 24 | 24 |
+| **68** | Croon | 2025 | Can GW231123 have a stellar origin? | 24 | 23 | 24 |
 | **69** | Boschini | 2025 | Orbital eccentricity in general relativity from catastrophe theory | 22 | 24 | 24 |
 | **70** | Fumagalli | 2023 | Spin-eccentricity interplay in merging binary black holes | 22 | 24 | 24 |
 | **71** | Moore | 2021 | Population-informed priors in gravitational-wave astronomy | 24 | 23 | 24 |
-| **72** | Zhao | 2017 | Nutational resonances, transitional precession, and precession-averaged evolution in binary black-hole systems | 21 | 23 | 23 |
-| **73** | Gerosa | 2017 | On the equal-mass limit of precessing black-hole binaries | 19 | 23 | 23 |
-| **74** | Mould | 2020 | Endpoint of the up-down instability in precessing binary black holes | 18 | 22 | 22 |
-| **75** | Sperhake | 2020 | Amplification of superkicks in black-hole binaries through orbital eccentricity | 21 | 22 | 22 |
+| **72** | Sperhake | 2020 | Amplification of superkicks in black-hole binaries through orbital eccentricity | 21 | 23 | 23 |
+| **73** | Zhao | 2017 | Nutational resonances, transitional precession, and precession-averaged evolution in binary black-hole systems | 21 | 23 | 23 |
+| **74** | Gerosa | 2017 | On the equal-mass limit of precessing black-hole binaries | 19 | 23 | 23 |
+| **75** | Mould | 2020 | Endpoint of the up-down instability in precessing binary black holes | 18 | 22 | 22 |
 | **76** | Gerosa | 2019 | Wide nutation: binary black-hole spins repeatedly oscillating from full alignment to full anti-alignment | 20 | 22 | 22 |
 | **77** | Romero-Shaw | 2025 | GW200208_222617 as an eccentric black-hole binary merger: properties and astrophysical implications | 21 | 20 | 21 |
 | **78** | Mancarella | 2023 | Inferring, not just detecting: metrics for high-redshift sources observed with third-generation gravitational-wave detectors | 16 | 21 | 21 |
@@ -203,4 +203,4 @@
 
 
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-*Last updated: 2026-02-05 01:01:12 UTC*
+*Last updated: 2026-02-06 01:01:10 UTC*

_group.md

@@ -259,4 +259,4 @@ Here are the amazing students who are currently completing research projects wit
 
 
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-*Last updated: 2026-02-05 01:01:12 UTC*
+*Last updated: 2026-02-06 01:01:10 UTC*

_publications.md

@@ -690,4 +690,4 @@ E. Berti, et al. (53 authors incl. **D. Gerosa**).\
 
 
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-*Last updated: 2026-02-05 01:01:12 UTC*
+*Last updated: 2026-02-06 01:01:10 UTC*

_talks.md

@@ -549,4 +549,4 @@ Liceo Candia and Liceo Frassati, Seregno, Italy, Jan 2018.
 
 
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-*Last updated: 2026-02-05 01:01:12 UTC*
+*Last updated: 2026-02-06 01:01:10 UTC*