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Tracing the evolution of the cool gas in CGM and IGM environments through Mg II absorption from redshift z=0.75 to z=1.65 using DESI-Y1 data

Fuente: arXiv

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Bibliographic Details
Main Authors:	Wu, X., Cai, Z., Lan, T. -W., Zou, S., Anand, A., Dey, Biprateep, Li, Z., Aguilar, J., Ahlen, S., Brooks, D., Claybaugh, T., de la Macorra, A., Doel, P., Ferraro, S., Forero-Romero, J. E., Gontcho, S. Gontcho A, Honscheid, K., Juneau, S., Kehoe, R., Kisner, T., Lambert, A., Landriau, M., Guillou, L. Le, Manera, M., Meisner, A., Miquel, R., Moustakas, J., Newman, J. A., Prada, F., Rossi, G., Sanchez, E., Schlegel, D., Schubnell, M., Siudek, M., Sprayberry, D., Tarlé, G., Weaver, B. A., Zou, H.
Format:	Preprint
Published:	2024
Subjects:	Astrophysics of Galaxies
Online Access:	Acceder al recurso
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Internet

https://arxiv.org/abs/2407.17809