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researcher

S. Borgani

102 papers hereh-index 6128 citations133 works total

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • middle author19
  • last author1

Across the 20 of 102 papers where every author was matched, so the position is known.

fields
  • astro-ph.CO57
  • astro-ph.GA35
  • astro-ph.IM9
  • physics.comp-ph1
same name
  • S. Borgani — 327 papers, h 84
  • S. Borgani — 18 papers, h 8
  • S. Borgani — 8 papers
  • S. Borgani — 3 papers, h 4
  • S. Borgani — 2 papers, h 2

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

activity
20112026
most citedProbing dark energy with the next generation X-ray surveys of galaxy clusters

17 citations · 127 across the 100 of their papers we have counts for

collaborators
Showing 2024Show all

3 papers · 1 filter

astro-ph.CO2024

Euclid preparation: TBD. The impact of line-of-sight projections on the covariance between galaxy cluster multi-wavelength observable properties -- insights from hydrodynamic simulations

Euclid Collaboration, A. Ragagnin, A. Saro +240

Cluster cosmology can benefit from combining multi-wavelength studies, which can benefit from characterising the correlation coefficients between different mass-observable relation…

astro-ph.CO2024★ 4 cited

Euclid preparation. The impact of relativistic redshift-space distortions on two-point clustering statistics from the Euclid wide spectroscopic survey

Euclid Collaboration, M. Y. Elkhashab, D. Bertacca +252

Measurements of galaxy clustering are affected by RSD. Peculiar velocities, gravitational lensing, and other light-cone projection effects modify the observed redshifts, fluxes, an…

astro-ph.CO2024★ 8 cited

Euclid preparation. LIX. Angular power spectra from discrete observations

Euclid Collaboration, N. Tessore, B. Joachimi +266

We present the framework for measuring angular power spectra in the Euclid mission. The observables in galaxy surveys, such as galaxy clustering and cosmic shear, are not continuou…

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Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.