activity
20152026
most citedStrong FUV fields drive the [CII]/FIR deficit in z~3 dusty, star-forming galaxies

71 citations · 159 across the 23 of their papers we have counts for

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Showing astro-ph.GAShow all

25 papers · 1 filter

astro-ph.GA20261 cited

Direct detection of cool molecular gas in a star-forming galaxy at

Karin Cescon, Jacqueline A. Hodge, Leindert A. Boogaard +21

We investigate the molecular gas content and interstellar medium (ISM) conditions of REBELS-25, a massive, star-forming galaxy at . Deep VLA Q-band and ALMA Band 3 observat…

astro-ph.GA20261 cited

Investigating the role of turbulence in the interstellar medium in dusty star-forming galaxies using kpc-resolution ALMA dust and gas maps

B. A. Westoby, J. A. Hodge, P. Sharda +28

We present ALMA high-resolution (0.25/2 kpc) CO(5-4) and CO(4-3) observations of three submillimetre-selected dusty galaxies from the ALESS survey.…

astro-ph.GA20261 cited

ALESS--JWST: Dust-driven Morphologies and Hidden Stellar Mass in Sub-millimeter Galaxies

J. Li, E. da Cunha, J. A. Hodge +17

We present JWST/NIRCam and MIRI observations of twelve sub-millimeter galaxies (SMGs) from the ALESS survey, combined with high-resolution () ALMA 870m i…

astro-ph.GA2025

The molecular diversity of the ISM in galaxies across cosmic time

Mathilde Bouvier, Yiqing Song, Michael Romano +7

Submillimetre molecular lines (e.g., CO, HCN, SiO) provide a uniquely powerful view of the physical and chemical processes that govern star formation (SF) and galaxy evolution. Yet…

astro-ph.GA20254 cited

PRUSSIC III -- ALMA and NOEMA survey of dense gas in high-redshift star-forming galaxies

Matus Rybak, G. Sallaberry, J. A. Hodge +7

Characterising the relationship between dense gas and star formation is critical for understanding the assembly of galaxies throughout cosmic history. However, due to the faintness…

astro-ph.GA20255 cited

Detection of millimeter-wave coronal emission in a quasar at cosmological distance using microlensing

M. Rybak, D. Sluse, K. K. Gupta +5

Determining the nature of emission processes at the heart of quasars is critical for understanding environments of supermassive black holes. One of the key open questions is the or…