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1st Roman Young Researchers Meeting Proceedings
E. Cannuccia, M. Migliaccio, D. Pietrobon +29
During the last few decades scientists have been able to test the bases of the physics paradigms, where the quantum mechanics has to match the cosmological scales. Between the extr…
Mid- and Far-infrared Luminosity Functions and Galaxy Evolution from Multiwavelength Spitzer Observations up to z~2.5
G. Rodighiero, M. Vaccari, A. Franceschini +25
[Abridged]We exploit a large homogeneous dataset to derive a self-consistent picture of IR emission based on the time-dependent 24, 15, 12 and 8micron monochromatic and bolometric…
Black hole growth and starburst activity at z = 0.6-4 in the Chandra Deep Field South. Host galaxies properties of obscured AGN
M. Brusa, F. Fiore, P. Santini +8
The co-evolution of host galaxies and the active black holes which reside in their centre is one of the most important topics in modern observational cosmology. Here we present a s…
Evidence for a fast evolution of the UV luminosity function beyond redshift 6 from a deep HAWK-I survey of the GOODS-S field
M. Castellano, A. Fontana, K. Boutsia +21
We perform a deep search for galaxies in the redshift range 6.5<z<7.5, to measure the evolution of the number density of luminous galaxies in this redshift range and derive useful…
Star formation and mass assembly in high redshift galaxies
P. Santini, A. Fontana, A. Grazian +14
We study the star formation and the mass assembly process of 0.3<=z<2.5 galaxies using their IR emission from MIPS 24um band. We used an updated version of the GOODS-MUSIC catalog,…
Subdegree Sunyaev-Zel'dovich Signal from Multifrequency BOOMERanG observations
M. Veneziani, A. Amblard, A. Cooray +36
The Sunyaev-Zel'dovich (SZ) effect is the inverse Compton-scattering of cosmic microwave background (CMB) photons by hot electrons in the intervening gas throughout the universe. T…