Effects of Dust at High Redshift Dusty Star-Forming Galaxies
2023.05.24 12:09 - udgov_hsHYBRID-SEMINAR
Online: https://www.gotomeet.me/NCBJmeetings/phd-seminar
In-person: room 207, Pasteura 7
Date: Thursday, 25 May, 9:15
Abstract:
HYBRID-SEMINAR
Online: https://www.gotomeet.me/NCBJmeetings/phd-seminar
In-person: room 207, Pasteura 7
Date: Thursday, 25 May, 9:15
Abstract:
One very promising observable to study gluon saturation effects at high energy is photon+jet production at forward rapidity in proton-nucleus collisions. Since the produced photon does not rescatter on the target, this observable provides a clean environment to study the interaction of the quark probe with the dense target.
The chemical evolution of galaxies is the direct product of the whole history of star formation. This relation is encoded in the so-called "fundamental metallicity relation'' (FMR), a three-dimensional relation that connects stellar mass, star formation rate, and metallicity. The FMR is mainly studied for star-forming galaxies at low redshift, z~0 with the Sloan Digital Sky Survey (SDSS). Very low statistics are available at higher redshift but the FMR shows no evolution with cosmic time.