IRAM 30-meter millimeter follow-up of deep OSIRIS-GTC optical surveys

IRAM 30-meter millimeter follow-up of deep OSIRIS-GTC optical surveys

It is broadly accepted that CO is a reliable tracer of H2 in massive IR (LIR ≳ 109 L⊙) galaxies, and that there are clear correlations between LIR and L’CO that are qualitatively independent of environment and even redshift. We present two tales on the search for 12CO emission from dusty star-formin...

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Bibliographic Details
Main Authors: Sánchez-Portal M., Bongiovanni A., Cepa J., González-Serrano J.I., González J.J., González-Otero M., Padilla-Torres C.P., Pérez García A.M., Pintos-Castro I., Pérez-Martínez R.M., Cruz-González I., Negrete A., Beyoro-Amado Z., Pović M.
Format: Article
Language:English
Published: EDP Sciences 2024-01-01
Series:EPJ Web of Conferences
Online Access:https://www.epj-conferences.org/articles/epjconf/pdf/2024/03/epjconf_mmUniverse2023_00047.pdf

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https://www.epj-conferences.org/articles/epjconf/pdf/2024/03/epjconf_mmUniverse2023_00047.pdf

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