December 17, 2025
Facultad de Ciencias Físicas
Europe/Madrid timezone

Unveiling the nature of a representative sample of Extreme Emission Line Galaxies at intermediate redshift

Dec 17, 2025, 10:11 AM
8m
00.xx.0 - Aula Magna M2 (Facultad de Ciencias Físicas)

00.xx.0 - Aula Magna M2

Facultad de Ciencias Físicas

100

Speaker

María Delgado Mancheño (Universidad Complutense de Madrid)

Description

Studies of early galaxy formation are crucial for understanding the processes that have shaped the current Universe. Galaxies with intense star formation at z $>$ 6 are key to events such as reionization, but their faintness limits detailed studies. At lower redshifts (z $\sim$ 1), analogous galaxies allow for better characterization. Extreme Emission Line Galaxies (EELGs) stand out due to their high equivalent widths ($\sim$1000 Å), high specific star formation rates, low metallicities, and low masses. We aim to characterize the physical properties of a sample of 122 EELGs at 0.7 $<$ z $<$ 2, photometrically selected from the Extended Groth Strip catalog, obtaining results consistent with previous studies (Van Der Wel et al. 2011).

Author

María Delgado Mancheño (Universidad Complutense de Madrid)

Co-authors

Dr Jesús Gallego Maestro (Universidad Complutense de Madrid) Dr Sergio Pascual Ramírez (Universidad Complutense de Madrid)

Presentation materials