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Infrared color selection of massive galaxies at z > 3
T. Wang, D. Elbaz, C. Schreiber +29
We introduce a new color-selection technique to identify high-redshift, massive galaxies that are systematically missed by Lyman-break selection. The new selection is based on the…
Chandra counterparts of CANDELS GOODS-S sources
N. Cappelluti, A. Comastri, A. Fontana +18
Improving the capabilities of detecting faint X-ray sources is fundamental to increase the statistics on faint high-z AGN and star-forming galaxies. We performed a simultaneous Max…
The Grism Lens-Amplified Survey from Space (GLASS). III. A census of Lyα Emission at 7 from HST Spectroscopy
K. B. Schmidt, T. Treu, M. Bradač +15
[abbreviated] We present a census of Lyα emission at utilizing deep near infrared HST grism spectroscopy from the first six completed clusters of the Grism Lens-Amplifi…
The Grism Lens-Amplified Survey from Space (GLASS). V. Extent and spatial distribution of star formation in z~0.5 cluster galaxies
Benedetta Vulcani, Tommaso Treu, Kasper B. Schmidt +14
We present the first study of the spatial distribution of star formation in z~0.5 cluster galaxies. The analysis is based on data taken with the Wide Field Camera 3 as part of the…
The evolution of the equivalent width of the Ha emission line and specific star-formation rate in star-forming galaxies at 1<z<5
E. Marmol-Queralto, R. J. McLure, F. Cullen +3
We present the results of a study which uses spectral energy distribution (SED) fitting to investigate the evolution of the equivalent width (EW) of the Halpha emission line in sta…
The Lyman Continuum escape fraction of galaxies at z=3.3 in the VUDS-LBC/COSMOS field
A. Grazian, E. Giallongo, R. Gerbasi +52
The Lyman continuum (LyC) flux escaping from high-z galaxies into the IGM is a fundamental quantity to understand the physical processes involved in the reionization epoch. We have…