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20012026
most citedThe ALPINE-ALMA [CII] Survey: data processing, catalogs, and statistical source properties

245 citations · 7.2k across the 176 of their papers we have counts for

collaborators

180 papers

astro-ph.GA2026

SCALES. II. The Internal Composition of Giant Star-Forming Clumps at

Boris S. Kalita, Adélaïde Claeyssens, Luis C. Ho +12

Star-forming structures of scale , dubbed 'giant' star-forming clumps, are routinely detected in unlensed surveys of galaxies. Two scenarios are us…

astro-ph.GA2026

SCALES. I. Bridging Lensed Clump - Giant Clump Scales in Lensed Galaxies at

Boris S. Kalita, Adélaïde Claeyssens, Luis C. Ho +12

Dense star-forming regions in galaxies, often termed 'clumps', have been studied across two distinct regimes of telescope resolution, each motivating interpretations in tensi…

astro-ph.GA2026

The ALPINE-CRISTAL-JWST Survey: Investigating the role of interstellar dust, gas and stars in high-z galaxies at kpc-scales

F. Lopez, M. Relano, I. De Looze +37

A comprehensive understanding of galaxy evolution requires a detailed analysis of gas and dust, their distribution, and evolution within galaxies. We analyse spatially resolved (~k…

astro-ph.GA2026

Multi-tracer exploration of molecular gas in main sequence galaxies at z~4.5

M. Dessauges-Zavadsky, M. Béthermin, M. Ginolfi +15

Molecular gas masses in high-z galaxies are inferred from indirect tracers, whose respective reliability remains poorly constrained. In particular, the bright [CII] 158m line is…

astro-ph.GA2026

A Census of the 200 Most Massive Galaxies Spectroscopically Observed with JWST at zspec 3-15

Mengyuan Xiao, Pascal A. Oesch, Longji Bing +26

Massive galaxies provide strong tests of galaxy formation models, yet a comprehensive spectroscopic view of their properties and demographics in the early Universe has remained elu…

astro-ph.GA2026

A Glimpse of the Low-Mass End of the Direct Mass-Metallicity Relation at

Tiger Yu-Yang Hsiao, John Chisholm, Danielle A. Berg +22

The competition between metal synthesis and feedback from massive stars establishes the mass-metallicity relation (MZR) at low-redshifts. Examining this relation at higher redshift…