collaborators

8 papers

astro-ph.CO2026

Evidence for a thermal pressure deficit in galaxy groups from the tSZ effect and weak lensing

Jared Siegel, Alexandra Amon, Jenny E. Greene +3

Measurements of the thermal Sunyaev-Zel'dovich (tSZ) effect have yet to form a consistent picture of the thermodynamic state of the gas in the intracluster medium: their interpreta…

astro-ph.CO2025

Confronting cosmic shear astrophysical uncertainties: DES Year 3 revisited

Leah Bigwood, Jamie McCullough, Jared Siegel +19

Cosmology from weak gravitational lensing has been limited by astrophysical uncertainties in baryonic feedback and intrinsic alignments. By calibrating these effects using external…

astro-ph.CO2025

The suppression of the matter power spectrum: strong feedback from X-ray gas mass fractions, kSZ effect profiles, and galaxy-galaxy lensing

Jared Siegel, Leah Bigwood, Alexandra Amon +6

Baryon feedback redistributes gas relative to the underlying dark matter distribution and suppresses the matter power spectrum on small scales, but the amplitude and scale dependen…

astro-ph.CO2025

The kinetic Sunyaev Zeldovich effect as a benchmark for AGN feedback models in hydrodynamical simulations: insights from DESI + ACT

Leah Bigwood, Masaya Yamamoto, Jared Siegel +7

Baryonic feedback remains one of the largest uncertainties in cosmological hydrodynamical simulations, with different prescriptions producing divergent predictions for the fraction…

astro-ph.CO2025

Prospects for disentangling dark matter with weak lensing

Calvin Preston, Keir K. Rogers, Alexandra Amon +1

We investigate the degeneracy between the effects of ultra-light axion dark matter and baryonic feedback in suppressing the matter power spectrum. We forecast that galaxy shear dat…

astro-ph.CO2025

Joint X-ray, kinetic Sunyaev-Zeldovich, and weak lensing measurements: toward a consensus picture of efficient gas expulsion from groups and clusters

Jared Siegel, Alexandra Amon, Ian G. McCarthy +7

There is no consensus on how baryon feedback shapes the underlying matter distribution from either simulations or observations. We confront the uncertain landscape by jointly analy…