325 citations · 1.2k across the 43 of their papers we have counts for
39 papers
A comparative test of different pressure profile models in clusters of galaxies using recent ACT data
Denis Tramonte
Context. The electron pressure profile is a convenient tool to characterize the thermodynamical state of a galaxy cluster, with several studies adopting a "universal" functional fo…
FAST drift scan survey for HI intensity mapping: simulation on hunting HI filament with pairwise stacking
Diyang Liu, Yichao Li, Denis Tramonte +5
Filaments stand as pivotal structures within the cosmic web. However, direct detection of the cold gas content of the filaments remains challenging due to its inherent low brightne…
QUIJOTE scientific results -- XVIII. New constraints on the polarization of the Anomalous Microwave Emission in bright Galactic regions: \,Ophiuchi, Perseus and W43
R. González-González, R. T. Génova-Santos, J. A. Rubiño-Martín +24
This work focuses on the study of the AME, an important emission mechanism between 10 and 60 GHz whose polarization properties are not yet fully understood, and is therefore a pote…
Cross-correlation of cosmic voids with thermal Sunyaev-Zel'dovich data
Gang Li, Yin-Zhe Ma, Denis Tramonte +1
We provide a measurement of the deficit in the Sunyaev-Zel'dovich Compton- signal towards cosmic voids, by stacking a catalogue of 97,090 voids constructed with BOSS-DR12 data,…
Cross-correlation between the thermal Sunyaev-Zeldovich effect and the Integrated Sachs-Wolfe effect
Ayodeji Ibitoye, Wei-Ming Dai, Yin-Zhe Ma +5
We present a joint cosmological analysis of the power spectra measurement of the Planck Compton parameter and the integrated Sachs-Wolfe (ISW) maps. We detect the statistical corre…
QUIJOTE scientific results -- XIII. Intensity and polarization study of supernova remnants in the QUIJOTE-MFI wide survey: CTB 80, Cygnus Loop, HB 21, CTA 1, Tycho and HB 9
Carlos Hugo López-Caraballo, Beatriz Ruiz-Granados, Ricardo Genova Santos +21
We use the new QUIJOTE-MFI wide survey (11, 13, 17 and 19 GHz) to produce spectral energy distributions (SEDs), on an angular scale of 1 deg, of the supernova remnants (SNRs) CTB 8…