Работы, цитирующие эту работу

Работ: 5

Работа: An Accurate Physical Model for Halo Concentrations

1. SPT clusters with DES and HST weak lensing. I. Cluster lensing and Bayesian population modeling of multiwavelength cluster datasets

   S. Bocquet, S. Grandis, L. E. Bleem +97

   СтатьяGalaxies: Formation, Evolution, PhenomenaPhysical review. D/Physical review. D.2024Цитирований: 1

   ABIABI:AkademIndex/openalex/2024.article.000177

2. <i>Euclid</i> preparation

   Pierluigi Monaco, Gabriele Parimbelli, M.Y Elkhashab +97

   ПрепринтScientific Computing and Data ManagementAstronomy and Astrophysics2025Цитирований: 1

   ABIABI:AkademIndex/openalex/2025.preprint.000004

3. <i>Euclid</i> preparation

   L. Ingoglia, M. Sereno, S. Farrens +97

   СтатьяAstronomy and Astrophysical ResearchAstronomy and Astrophysics2025Цитирований: 0

   ABIABI:AkademIndex/openalex/2025.article.001551

4. XRISM Constraints on Unidentified X-Ray Emission Lines, Including the 3.5 keV Line, in the Stacked Spectrum of 10 Galaxy Clusters

   M. Audard, Hisamitsu Awaki, Ralf Ballhausen +97

   СтатьяGalaxies: Formation, Evolution, PhenomenaThe Astrophysical Journal Letters2025Цитирований: 0

   ABIABI:AkademIndex/openalex/2025.article.002537

5. An emulation-based model for the projected correlation function

   Vetle A. Vikenes, Cheng-Zong Ruan, David F. Mota

   СтатьяSimulation Techniques and ApplicationsAstronomy and Astrophysics2025Цитирований: 0

   ABIABI:AkademIndex/openalex/2025.article.004216