activity
20152023
most citedPlanck 2015 results. XXII. A map of the thermal Sunyaev-Zeldovich effect

178 citations · 345 across the 5 of their papers we have counts for

collaborators

5 papers

astro-ph.GA2023★ 6 cited

Star forming brightest cluster galaxies at in KiDS. Further studies of cold gas and stellar properties

G. Castignani, M. Radovich, F. Combes +10

Brightest cluster galaxies (BCGs) are among the most massive galaxies in the Universe. Their star formation (SF) history and stellar mass assembly are debated. Recent studies sugge…

astro-ph.CO2023★ 19 cited

QUIJOTE scientific results -- VIII. Diffuse polarized foregrounds from component separation with QUIJOTE-MFI

E. de la Hoz, R. B. Barreiro, P. Vielva +23

We derive linearly polarized astrophysical component maps in the Northern Sky from the QUIJOTE-MFI data at 11 and 13 GHz in combination with the WMAP K and Ka bands (23 and 33 GHz)…

astro-ph.GA2016★ 66 cited

QUIJOTE Scientific Results. II. Polarisation Measurements of the Microwave Emission in the Galactic molecular complexes W43 and W47 and supernova remnant W44

R. Génova-Santos, J. A. Rubiño-Martín, A. Peláez-Santos +11

We present Q-U-I JOint TEnerife (QUIJOTE) intensity and polarisation maps at 10-20 GHz covering a region along the Galactic plane 24<l<45 deg, |b|<8 deg. These maps result from 210…

astro-ph.CO2015★ 178 cited

Planck 2015 results. XXII. A map of the thermal Sunyaev-Zeldovich effect

Planck Collaboration, N. Aghanim, M. Arnaud +199

We have constructed all-sky y-maps of the thermal Sunyaev-Zeldovich (tSZ) effect by applying specifically tailored component separation algorithms to the 30 to 857 GHz frequency ch…

astro-ph.GA2015★ 76 cited

Measurements of the Intensity and Polarization of the Anomalous Microwave Emission in the Perseus molecular complex with QUIJOTE

R. Génova-Santos, J. A. Rubiño-Martín, R. Rebolo +27

Anomalous microwave emission (AME) has been observed in numerous sky regions, in the frequency range ~10-60 GHz. One of the most scrutinized regions is G159.6-18.5, located within…