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astro-ph.GA2024

Baryonic Ecosystem in Galaxies (BEINGMgII). Host Galaxies of Ultra-strong MgII Absorbers in Subaru Hyper Suprime-Cam Survey

Ravi Joshi, Sarbeswar Das, Michele Fumagalli +5

We study the galaxies hosting ultra-strong MgII (USMgII) absorbers at small impact parameters of 2" (5 - 20 kpc), spanning a redshift range of , using deep…

astro-ph.GA2024

Atomic and molecular gas as traced by [C II] emission

Benedetta Casavecchia, Umberto Maio, Céline Péroux +1

The latest ALMA and JWST observations provide new information on the birth and evolution of galaxies in the early Universe, at the epoch of reionization. Of particular importance a…

astro-ph.GA2024

The Multi-Scale Multi-Phase Circumgalactic Medium: Observed and Simulated

Celine Peroux, Dylan Nelson

These are exciting times for studies of galaxy formation and the growth of structures. New observatories and advanced simulations are revolutionising our understanding of the cycli…

astro-ph.GA2024

Baryonic Ecosystem in Galaxies (BEINGMgII) -- II. Unveiling the Nature of Galaxies Harboring Cool Gas Reservoirs

S. Das, R. Joshi, R. Chaudhary +4

We search for the galaxies associated with the intervening MgII absorbers over a redshift range of using imaging data from DESI Legacy Imaging Surveys and measu…

astro-ph.GA2024

ALMACAL XII. Data characterisation and products

Victoria Bollo, Martin Zwaan, Celine Peroux +5

The ALMACAL survey is based on a database of reprocessed ALMA calibration scans suitable for scientific analysis, observed as part of regular PI observations. We present all the da…

astro-ph.GA2024

Metal line emission around z<1 galaxies

Rajeshwari Dutta, Michele Fumagalli, Matteo Fossati +7

We characterize, for the first time, the average extended emission in multiple lines ([OII], [OIII], and Hbeta) around a statistical sample of 560 galaxies at z~0.25-0.85. By stack…