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Fitting pseudo-Srsic(Spergel) light profiles to galaxies in interferometric data: the excellence of the -plane
Qing-Hua Tan, Emanuele Daddi, Victor de Souza Magalhães +11
Modern (sub)millimeter interferometers, such as ALMA and NOEMA, offer high angular resolution and unprecedented sensitivity. This provides the possibility to characterize the morph…
ACOSMOS: Dissecting the gas content of star-forming galaxies across the main sequence at 1.2 < 1.6
Tsan-Ming Wang, Benjamin Magnelli, Eva Schinnerer +5
We aim to understand the physical mechanisms that drive star formation in a sample of mass-complete (>10) star-forming galaxies (SFGs) at 1.2 < 1.6. We se…
Measuring the gas reservoirs in M M galaxies at
Rosa M. Mérida, Carlos Gómez-Guijarro, Pablo G. Pérez-González +7
Understanding the gas content in galaxies, its consumption and replenishment, remains pivotal in our comprehension of the evolution of the Universe. Numerous studies have addressed…
CEERS: 7.7 m PAH Star Formation Rate Calibration with JWST MIRI
Kaila Ronayne, Casey Papovich, Guang Yang +33
We test the relationship between UV-derived star formation rates (SFRs) and the 7.7 m polycyclic aromatic hydrocarbon (PAH) luminosities from the integrated emission of galaxies…
Noema formIng Cluster survEy (NICE): Discovery of a starbursting galaxy group with a radio-luminous core at z=3.95
Luwenjia Zhou, Tao Wang, Emanuele Daddi +34
The study of distant galaxy groups and clusters at the peak epoch of star formation is limited by the lack of a statistically and homogeneously selected and spectroscopically confi…
Identification of a transition from stochastic to secular star formation around with JWST
L. Ciesla, D. Elbaz, O. Ilbert +6
Star formation histories (SFH) of early (612) galaxies have been found to be highly stochastic in both simulations and observations, while at 6 the presence of a ma…