IM
Ian G. McCarthy
astro-ph.COastro-ph.GAastro-phastro-ph.HEhep-exastro-ph.IMcosmology: theorygalaxies: clusters: generalgalaxies: formationlarge-scale structure of Universe
On Valency
published · living versionsW_536mjbss·v1 · currentpublished
Quantifying the effect of baryon physics on weak lensing tomography
with Elisabetta Semboloni, Henk Hoekstra, Joop Schaye, Marcel P. van Daalen
1 version
Preprints & journals
179 papers in the corpus · 2001–2026Cosmological constraining power of the redshifts, heights, and angular clustering of weak gravitational lensing peaks2607.29128v2 · Jeger C. Broxterman, Matthieu Schaller, Ian G. McCarthy et al.2026 · 0 citationsarXiv
Evidence for a thermal pressure deficit in galaxy groups from the tSZ effect and weak lensing2608.00164v1 · Jared Siegel, Alexandra Amon, Jenny E. Greene et al.2026 · 0 citationsarXiv
FLAMINGO: The thermal history of the Universe from tSZ effect cross-correlations and its dependencies on cosmology and baryon physics2605.11083v2 · Jaime Salcido, Tianyi Yang, Ian G. McCarthy et al.2026 · 0 citationsarXiv
The FLAMINGO simulations data release2604.24324v3 · John C. Helly, Robert J. McGibbon, Joop Schaye et al.2026 · 3 citationsarXiv
Revealing the neutrino mass through persistent homology of the cosmic web2604.02300v1 · Jiaqi Wang, Willem Elbers, Carlos S. Frenk et al.2026 · 0 citationsarXiv
Implications of a contracted dark matter halo for the Milky Way's inferred virial mass2603.13516v1 · Diego Dado (Durham-ICC), Shaun T. Brown, Stockholm-OKC et al.2026 · 0 citationsarXiv
Impact and interplay of CDM analysis choices for LSST cosmic shear2602.21863v3 · N. C. Robertson, C. Heymans, J. Zuntz et al.2026 · 0 citationsarXiv
The suppression of the matter power spectrum: strong feedback from X-ray gas mass fractions, kSZ effect profiles, and galaxy-galaxy lensing2512.02954v1 · Jared Siegel, Leah Bigwood, Alexandra Amon et al.2025 · 8 citationsMon Not R Astron Soc (2026)
Constraining baryonic feedback and cosmology from DES Y3 and Planck PR4 6$\times$2pt data. I. CDM models2510.25596v2 · Jiachuan Xu, Tim Eifler, Elisabeth Krause et al.2025 · 2 citationsarXiv
FLAMINGO: Tracing the co-evolution of hot gas and black holes in galaxy groups and clusters2510.17980v2 · Emily E. Costello, Ian G. McCarthy, Jaime Salcido et al.2025 · 3 citationsMon Not R Astron Soc (2026)
The kinetic Sunyaev Zeldovich effect as a benchmark for AGN feedback models in hydrodynamical simulations: insights from DESI + ACT2510.15822v1 · Leah Bigwood, Masaya Yamamoto, Jared Siegel et al.2025 · 5 citationsarXiv
Joint X-ray, kinetic Sunyaev-Zeldovich, and weak lensing measurements: toward a consensus picture of efficient gas expulsion from groups and clusters2509.10455v1 · Jared Siegel, Alexandra Amon, Ian G. McCarthy et al.2025 · 9 citationsarXiv
The impact of galaxy bias on cross-correlation tomography2508.05319v2 · Sara Maleubre, Matteo Zennaro, David Alonso et al.2025 · 0 citationsarXiv
Entropy plateaus can emerge from gas replacement at a characteristic halo mass in simulated groups and clusters of galaxies2505.05675v2 · Edoardo Altamura, Scott T. Kay, Joop Schaye et al.2025 · 1 citationMon Not R Astron Soc (2025) 3367-3387
FLAMINGO: Galaxy formation and feedback effects on the gas density and velocity fields2412.09526v1 · Lurdes Ondaro-Mallea, Raul E. Angulo, Giovanni Arico et al.2024 · 3 citationsA&A 697, A63 (2025)
FLAMINGO: combining kinetic SZ effect and galaxy-galaxy lensing measurements to gauge the impact of feedback on large-scale structure2410.19905v2 · Ian G. McCarthy, Alexandra Amon, Joop Schaye et al.2024 · 29 citationsarXiv
Implications of feedback solutions to the tension for the baryon fractions of galaxy groups and clusters2409.05716v3 · Jaime Salcido, Ian G. McCarthy2024 · 6 citationsarXiv
The FLAMINGO Project: A comparison of galaxy cluster samples selected on mass, X-ray luminosity, Compton-Y parameter, or galaxy richness2406.03180v2 · Roi Kugel, Joop Schaye, Matthieu Schaller et al.2024 · 7 citationsarXiv
Applying machine learning to Galactic Archaeology: how well can we recover the origin of stars in Milky Way-like galaxies?2405.00102v2 · Andrea Sante, Andreea S. Font, Sandra Ortega-Martorell et al.2024 · 4 citationsarXiv
Weak lensing combined with the kinetic Sunyaev Zel'dovich effect: A study of baryonic feedback2404.06098v1 · L. Bigwood, A. Amon, A. Schneider et al.2024 · 70 citationsarXiv
The FLAMINGO project: the coupling between baryonic feedback and cosmology in light of the tension2403.12967v2 · Willem Elbers, Carlos S. Frenk, Adrian Jenkins et al.2024 · 21 citationsarXiv
ARTEMIS emulator: exploring the effect of cosmology and galaxy formation physics on Milky Way-mass haloes and their satellites2403.11692v2 · Shaun T. Brown, Azadeh Fattahi, Ian G. McCarthy et al.2024 · 8 citationsMNRAS, 532, 1223-1240 (2024)
GODMAX: Modeling gas thermodynamics and matter distribution using JAX2401.18072v1 · Shivam Pandey, Jaime Salcido, Chun-Hao To et al.2024 · 0 citationsarXiv
The FLAMINGO Project: Galaxy clusters in comparison to X-ray observations2312.08277v2 · Joey Braspenning, Joop Schaye, Matthieu Schaller et al.2023 · 36 citationsarXiv
The FLAMINGO project: Baryonic impact on weak gravitational lensing convergence peak counts2312.08450v3 · Jeger C. Broxterman, Matthieu Schaller, Joop Schaye et al.2023 · 15 citationsMNRAS, Volume 529, Issue 3, April 2024, Pages 2309-2326
Revisiting the effects of baryon physics on small-scale redshift space distortions2312.05009v3 · Juliana Kwan, Ian G. McCarthy, Jaime Salcido2023 · 3 citationsarXiv
Cosmic-Enu: An emulator for the non-linear neutrino power spectrum2311.11240v1 · Amol Upadhye, Juliana Kwan, Ian G. McCarthy et al.2023 · 0 citationsarXiv
FLAMINGO: calibrating large cosmological hydrodynamical simulations with machine learning.37900898 · Kugel, Roi, Schaye, Joop, Schaller, Matthieu et al.2023 · 95 citationsMonthly notices of the Royal Astronomical Society. 2023;526(4):6103-6127
The FLAMINGO project: revisiting the tension and the role of baryonic physics2309.07959v2 · Ian G. McCarthy, Jaime Salcido, Joop Schaye et al.2023 · 39 citationsarXiv
Non-linear CMB lensing with neutrinos and baryons: FLAMINGO simulations vs. fast approximations2308.09755v1 · Amol Upadhye, Juliana Kwan, Ian G. McCarthy et al.2023 · 2 citationsarXiv
The FLAMINGO project: cosmological hydrodynamical simulations for large-scale structure and galaxy cluster surveys2306.04024v3 · Joop Schaye, Roi Kugel, Matthieu Schaller et al.2023 · 274 citations2023, MNRAS, 526, 4978
SP(k) -- A hydrodynamical simulation-based model for the impact of baryon physics on the non-linear matter power spectrum2305.09710v1 · Jaime Salcido, Ian G. McCarthy, Juliana Kwan et al.2023 · 59 citationsarXiv
GOGREEN: a critical assessment of environmental trends in cosmological hydrodynamical simulations at z ~ 12210.10803v1 · Egidijus Kukstas, Michael L. Balogh, Ian G. McCarthy et al.2022 · 21 citationsarXiv
Testing the Collisionless Nature of Dark Matter with the Radial Acceleration Relation in Galaxy Clusters2207.03506v3 · Sut-Ieng Tam, Keiichi Umetsu, Andrew Robertson et al.2022 · 6 citationsApJ, 953, 169 (2023)
Constraints on dark matter self-interaction from the internal density profiles of X-COP galaxy clusters2205.01123v1 · D. Eckert, S. Ettori, A. Robertson et al.2022 · 63 citationsA&A 666, A41 (2022)
High-resolution synthetic UV-submm images for Milky Way-mass simulated galaxies from the ARTEMIS project2203.06078v1 · Peter Camps, Anand Utsav Kapoor, Ana Trcka et al.2022 · 26 citationsarXiv
The halo bispectrum as a sensitive probe of massive neutrinos and baryon physics2202.07680v2 · Victoria Yankelevich, Ian G. McCarthy, Juliana Kwan et al.2022 · 9 citations2023MNRAS.521.1448Y
Intrinsic alignments of the extended radio continuum emission of galaxies in the EAGLE simulations2201.04644v1 · Alexander D. Hill, Robert A. Crain, Ian G. McCarthy et al.2022 · 4 citationsarXiv
HSC-XXL : Baryon budget of the 136 XXL Groups and Clusters2111.10080v2 · Daichi Akino, Dominique Eckert, Nobuhiro Okabe et al.2021 · 1 citationarXiv
Constraining AGN feedback model with SZ profile2111.02088v2 · Hideki Tanimura, Gary Hinshaw, Ian G. McCarthy et al.2021 · 1 citationarXiv
Towards a universal model for the density profiles of dark matter haloes2110.01632v2 · Shaun T. Brown, Ian G. McCarthy, Sam G. Stafford et al.2021 · 10 citationsarXiv
Galaxy Velocity Bias in Cosmological Simulations: Towards Percent-level Calibration2110.01683v2 · Dhayaa Anbajagane, Han Aung, August E. Evrard et al.2021 · 26 citationsarXiv
Merger-induced galaxy transformations in the ARTEMIS simulations2109.13244v2 · Adam M. Dillamore, Vasily Belokurov, Andreea S. Font et al.2021 · 57 citationsMNRAS 513 (2022) 1867-1886
The BAHAMAS project: Evaluating the accuracy of the halo model in predicting the non-linear matter power spectrum2109.11855v2 · Alberto Acuto, Ian G. McCarthy, Juliana Kwan et al.2021 · 11 citationsarXiv
Testing extensions to LCDM on small scales with forthcoming cosmic shear surveys2109.11956v1 · Sam G. Stafford, Ian G McCarthy, Juliana Kwan et al.2021 · 2 citationsarXiv
Quenching of satellite galaxies of Milky Way analogues: reconciling theory and observations2109.06215v2 · Andreea S. Font, Ian G. McCarthy, Vasily Belokurov et al.2021 · 41 citationsarXiv
The GOGREEN survey: Dependence of galaxy properties on halo mass at z > 1 and implications for environmental quenching2107.03425v1 · Andrew M. M. Reeves, Michael L. Balogh, Remco F. J. van der Burg et al.2021 · 27 citationsarXiv
Simulating Groups and the IntraGroup Medium: The Surprisingly Complex and Rich Middle Ground Between Clusters and Galaxies2106.13257v1 · Benjamin D. Oppenheimer, Arif Babul, Yannick Bah'e et al.2021 · 98 citationsarXiv
On the road to percent accuracy V: the non-linear power spectrum beyond CDM with massive neutrinos and baryonic feedback2105.12114v2 · Benjamin Bose, Bill S. Wright, Matteo Cataneo et al.2021 · 41 citationsarXiv
The impact of Self-Interacting Dark Matter on the Intrinsic Alignments of Galaxies2104.02093v2 · David Harvey, Nora Elisa Chisari, Andrew Robertson et al.2021 · 12 citationsarXiv
Career total: 233 works. 179 are in this corpus.Showing the 50 most recent.
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