134 citations · 462 across the 9 of their papers we have counts for
12 papers
A Highly Magnified Star at Redshift 6.2
Brian Welch, Dan Coe, Jose M. Diego +26
Galaxy clusters magnify background objects through strong gravitational lensing. Typical magnifications for lensed galaxies are factors of a few but can also be as high as tens or…
Coincidence between morphology and star-formation activity through cosmic time: the impact of the bulge growth
Paola Dimauro, Emanuele Daddi, Francesco Shankar +10
The origin of the quenching in galaxies is still highly debated. Different scenarios and processes are proposed. We use multi-band (400-1600 nm) bulge-disc decompositions of massiv…
The bending of the star-forming main sequence traces the cold- to hot-accretion transition mass over 0<z<4
E. Daddi, I. Delvecchio, P. Dimauro +8
We analyse measurements of the evolving stellar mass (M0) at which the bending of the star-forming main sequence (MS) occurs over 0<z<4. We find M0~10^10Msun over 0<z<1, then M0 ri…
Photometric and Morphological Analysis of Fornax Galaxies through S-PLUS
A. V. Smith Castelli, A. R. Lopes, A. Cortesi +10
The photometric and morphological analysis of galaxies in clusters provides invaluable information regarding the evolutionary stage of the cluster itself. In addition, it helps to…
From naked spheroids to disky galaxies: how do massive disk galaxies shape their morphology?
L. Costantin, P. G. Pérez-González, J. Méndez-Abreu +9
We investigate the assembly history of massive disk galaxies and describe how they shape their morphology through cosmic time. Using SHARDS and HST data, we modeled the surface bri…
Extending the evolution of the stellar mass-size relation at to low stellar mass galaxies from HFF and CANDELS
Kalina V. Nedkova, Boris Häußler, Danilo Marchesini +23
We reliably extend the stellar mass-size relation over to low stellar mass galaxies by combining the depth of Hubble Frontier Fields (HFF) with the large volume c…