collaborators

6 papers

astro-ph.GA2025

REBELS-IFU: Steeply rising star formation histories and the importance of dust obscuration in massive galaxies revealed by multi-wavelength observations

R. Fisher, R. A. A. Bowler, R. K. Cochrane +15

Reliable star formation rate (SFR) measurements are essential for understanding early galaxy evolution, yet derived values rely on several assumptions. To address this problem, we…

astro-ph.GA2025

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.GA2025

The ALMA REBELS survey: [OIII] line scans of UV-bright galaxies

I. F. van Leeuwen, R. J. Bouwens, J. A. Hodge +17

We present the [OIII] spectral scan results from the ALMA Large Program REBELS (Reionization Era Bright Emission Line Survey). The generally high luminosity of [OI…

astro-ph.GA2025

Avoiding (photo-) Catastrophe

A. J. Battisti, E. da Cunha, S. Jin +1

Spectral modeling codes that estimate photometric redshifts (photo-) are a powerful and often reliable method for determining redshifts of galaxies. However, there are notable i…

astro-ph.GA2025

CO(1--0) imaging reveals 10-kiloparsec molecular gas reservoirs around star-forming galaxies at high redshift

Matus Rybak, J. T. Jansen, M. Frias Castillo +15

Massive, intensely star-forming galaxies at high redshift require a supply of molecular gas from their gas reservoirs, replenished by infall from the surrounding circumgalactic med…

astro-ph.GA2025

The ALMA-CRISTAL survey: Gas, dust, and stars in star-forming galaxies when the Universe was ~1 Gyr old I. Survey overview and case studies

R. Herrera-Camus, J. González-López, N. Förster Schreiber +44

We present the ALMA-CRISTAL survey, an ALMA Cycle 8 Large Program designed to investigate the physical properties of star-forming galaxies at through spat…