activity
20162024
most citedCOALAS: I. ATCA CO(1-0) survey and luminosity function in the Spiderweb protocluster at z=2.16

48 citations · 92 across the 8 of their papers we have counts for

collaborators

8 papers

astro-ph.GA2024★ 10 cited

COALAS III: The ATCA CO(1-0) look at the growth and death of H emitters in the Spiderweb protocluster at z=2.16

J. M. Pérez-Martínez, H. Dannerbauer, B. H. C. Emonts +26

We obtain CO(1-0) molecular gas measurements with ATCA on a sample of 43 spectroscopically confirmed H emitters in the Spiderweb protocluster at and investigate the rel…

astro-ph.GA2022★ 22 cited

ALMA Observation of a Galaxy Candidate Discovered with JWST

Ilsang Yoon, Christopher L. Carilli, Seiji Fujimoto +12

We report the ALMA observation of a galaxy candidate (GHZ1) discovered from the GLASS-JWST Early Release Science Program. Our ALMA program aims to detect the [OIII] em…

astro-ph.GA2021★ 11 cited

Early Science with the Large Millimeter Telescope: a 1.1 mm AzTEC Survey of Red- dusty star-forming galaxies

A. Montaña, J. A. Zavala, I. Aretxaga +32

We present LMT/AzTEC 1.1mm observations of luminous high-redshift dusty star-forming galaxy candidates from the sq.deg -ATLAS survey, selected on the…

astro-ph.GA2021★ 48 cited

COALAS: I. ATCA CO(1-0) survey and luminosity function in the Spiderweb protocluster at z=2.16

S. Jin, H. Dannerbauer, B. Emonts +25

We report a detailed CO(1-0) survey of a galaxy protocluster field at , based on 475 hours of observations with the Australia Telescope Compact Array. We constructed a larg…

astro-ph.GA2018

Science with an ngVLA. Cold gas in High-z Galaxies: The dense ISM

R. Decarli, C. Carilli, C. Casey +7

The goal of this science case is to study physical conditions of the interstellar medium (ISM) in distant galaxies. In particular, its densest component is associated with the inne…

astro-ph.GA2018★ 1 cited

Science with an ngVLA. Cold gas in High-z Galaxies: The molecular gas budget

R. Decarli, C. Carilli, C. Casey +7

The goal of this science case is to accurately pin down the molecular gas content of high redshift galaxies. By targeting the CO ground transition, we circumvent uncertainties rela…