13 citations · 39 across the 5 of their papers we have counts for
16 papers
Triple-ionised carbon associated with the low-density neutral hydrogen gas at 1.7 < z < 3.3: the integrated N(HI)-N(CIV) relation
Tae-Sun Kim, R. F. Carswell, C. Mongardi +4
From the Voigt profile fitting analysis of 183 intervening CIV systems at 1.7 < z < 3.3 in 23 high-quality UVES/VLT and HIRES/Keck QSO spectra, we find that a majority of CIV syste…
Constraining the baryon fraction in the Warm Hot Intergalactic Medium at low redshifts with PLANCK data
Ricardo Genova-Santos, Fernando Atrio-Barandela, Francisco-Shu Kitaura +1
We cross-correlate foreground cleaned Planck Nominal Cosmic Microwave Background (CMB) maps with two templates constructed from the Two-Micron All-Sky Redshift Survey of galaxies.…
The signature of the Warm Hot Intergalactic Medium in WMAP and the forthcoming PLANCK data
I. Suarez-Velásquez, F. -S. Kitaura, F. Atrio-Barandela +1
We compute the cross-correlation between the Warm-Hot Intergalactic Medium and maps of Cosmic Microwave Background temperature anisotropies using a log-normal probability density f…
Constraints on the Sunyaev-Zel'dovich signal from the Warm Hot Intergalactic Medium from WMAP and SPT data
Ricardo Genova-Santos, Isabel Suarez-Velasquez, Fernando Atrio-Barandela +1
The fraction of ionized gas in the Warm Hot Intergalactic Medium induces temperature anisotropies on the Cosmic Microwave Background similar to those of clusters of galaxies. The S…
The contribution of the Warm-Hot Intergalactic Medium to the CMB anisotropies via the Sunyaev-Zeldovich effect
I. F. Suarez-Velásquez, J. P. Mücket, F. Atrio-Barandela
Cosmological hydrodynamical simulations predict that a large fraction of all baryons reside within mildly non-linear structures with temperatures in the range K. As…
Filaments and sheets of the warm-hot intergalactic medium
J. S. Klar, J. P. Mücket
Filaments, forming in the context of cosmological structure formation, are not only supposed to host the majority of the baryons at low redshifts in the form of the WHIM, but also…