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Pinpointing the cosmic web between massive galaxy clusters I. The incidence of HI and OVI as WHIM tracers
At redshift z<1, the $Λ$CDM paradigm predicts that $\sim$40-50\% of baryons reside in the warm-hot intergalactic medium (WHIM) within cosmic web filaments. Characterizing the physical state and distribution of this dominant baryonic component is crucial for a complete picture of baryon evolution in
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