PANNELLA, MAURILIO

PANNELLA, MAURILIO  

Dipartimento di Fisica  

Settore FIS/05 - Astronomia e Astrofisica  

Assegnisti  

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Risultati 1 - 13 di 13 (tempo di esecuzione: 0.015 secondi).
Titolo Data di pubblicazione Autori File
A GIANT LY alpha NEBULA IN THE CORE OF AN X-RAY CLUSTER AT Z=1.99: IMPLICATIONS FOR EARLY ENERGY INJECTION 1-gen-2016 Strazzullo VPannella M +
Constraining radio mode feedback in galaxy clusters with the cluster radio AGNs properties to z ∼ 1 1-gen-2020 Pannella, M.Costanzi, M.Saro, A.Strazzullo, V. +
Deciphering the Activity and Quiescence of High-redshift Cluster Environments: ALMA Observations of Cl J1449+0856 at z = 2 1-gen-2018 Strazzullo, V.Pannella, M.Renzini, A. +
DISCOVERY OF A GALAXY CLUSTER WITH A VIOLENTLY STARBURSTING CORE AT z=2.506 1-gen-2016 Strazzullo VPannella M +
Galaxy populations in the most distant SPT-SZ clusters. I. Environmental quenching in massive clusters at 1.4 ≲ z ≲ 1.7 1-gen-2019 Strazzullo, V.Pannella, M.Saro, A. +
GOODS-HERSCHEL: STAR FORMATION, DUST ATTENUATION, AND THE FIR-RADIO CORRELATION ON THE MAIN SEQUENCE OF STAR-FORMING GALAXIES UP TO z similar or equal to 4 1-gen-2015 Pannella MStrazzullo V +
Merger-driven star formation activity in Cl J1449+0856 at z = 1.99 as seen by ALMA and JVLA 1-gen-2018 V StrazzulloM PannellaA Renzini +
Satellite content and quenching of star formation in galaxy groups at z similar to 1.8 1-gen-2015 Pannella MStrazzullo V +
The 700 ks Chandra Spiderweb Field 1-gen-2022 M. PannellaM. NoninoV. StrazzulloS. BorganiL. Di MascoloE. RasiaA. Saro +
The 700 ks Chandra Spiderweb Field 1-gen-2022 S. BorganiL. Di MascoloA. SaroM. PannellaE. RasiaM. Nonino +
THE RED SEQUENCE AT BIRTH IN THE GALAXY CLUSTER Cl J1449+0856 AT z=2 1-gen-2016 Strazzullo VPannella M +
The Spiderweb Protocluster is Being Magnetized by Its Central Radio Jet 1-gen-2022 S. BorganiLuca Di MascoloMaurilio PannellaA. Saro +
X-Ray Emission from the Jets and Lobes of the Spiderweb 1-gen-2022 Maurilio PannellaS. BorganiA. SaroM. NoninoL. Di Mascolo +