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20072026
most citedEuclid. I. Overview of the Euclid mission

550 citations · 11.3k across the 180 of their papers we have counts for

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Showing 2018Show all

8 papers · 1 filter

astro-ph.GA2018★ 26 cited

Quantifying the suppression of the (un)-obscured star formation in galaxy cluster cores at 0.20.9

L. Rodríguez-Muñoz, G. Rodighiero, C. Mancini +21

We quantify the star formation (SF) in the inner cores (/0.3) of 24 massive galaxy clusters at 0.20.9 observed by the …

astro-ph.GA2018★ 115 cited

Massive Star cluster formation under the microscope at z=6

E. Vanzella, F. Calura, M. Meneghetti +12

We report on a superdense star-forming region with an effective radius (R_e) smaller than 13 pc identified at z=6.143 and showing a star-formation rate density Σ_SFR~1000 Msun/yr/k…

astro-ph.GA2018★ 53 cited

Dissection of the collisional and collisionless mass components in a mini sample of CLASH and HFF massive galaxy clusters at

M. Bonamigo, C. Grillo, S. Ettori +7

We present a multi-wavelength study of the massive (-) galaxy clusters RXC J2248.74431, MACS J0416.12403, and MACS J120…

astro-ph.GA2018★ 8 cited

LBT/ARGOS adaptive optics observations of z lensed galaxies

M. Perna, M. Curti, G. Cresci +24

Gravitationally lensed systems allow a detailed view of galaxies at high redshift. High spatial- and spectral-resolution measurements of arc-like structures can offer unique constr…

astro-ph.GA2018★ 69 cited

Unveiling the dynamical state of massive clusters through the ICL fraction

Y. Jiménez-Teja, R. Dupke, N. Benítez +34

We have selected a sample of eleven massive clusters of galaxies observed by the Hubble Space Telescope in order to study the impact of the dynamical state on the IntraCluster Ligh…

astro-ph.GA2018★ 26 cited

The Kormendy Relation of Galaxies in the Frontier Fields Clusters: Abell S1063 and MACS J1149.5+2223

Luca Tortorelli, Amata Mercurio, Maurizio Paolillo +12

We analyse the Kormendy relations (KRs) of the two Frontier Fields clusters, Abell S1063, at z = 0.348, and MACS J1149.5+2223, at z = 0.542, exploiting very deep Hubble Space Teles…