20 citations · 97 across the 16 of their papers we have counts for
6 papers · 1 filter
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.…
The MeerKAT Massive Distant Clusters Survey: a search for diffuse radio emission in 30 massive SZ-selected clusters at
Dakalo G. Phuravhathu, M. Hilton, S. P. Sikhosana +10
We present the results of a search for diffuse radio emission in a uniformly selected sample of 30 of the most massive Sunyaev-Zel'dovich selected galaxy clusters at , provi…
The MeerKAT Massive Distant Clusters Survey: detection of diffuse radio emission in galaxy clusters at
Dakalo G. Phuravhathu, M. Hilton, S. P. Sikhosana +11
Diffuse, low surface-brightness radio emission in merging galaxy clusters provides insights into cosmic structure formation, the growth of magnetic fields, and turbulence. This pap…
PRUSSIC II -- ALMA imaging of dense-gas tracers in SDP.81: Evidence for low mechanical heating and a sub-solar metallicity in a z=3.04 dusty galaxy
M. Rybak, J. van Marrewijk, J. A. Hodge +6
We present deep ALMA Band 3 observations of the HCN, HCO+, and HNC (4-3) emission in SDP.81, a well-studied z = 3.042 strongly lensed galaxy. These lines trace the high-density gas…
To see or not to see a galaxy, that is the question
Melanie Kaasinen, Joshiwa van Marrewijk, Gergö Popping +7
Determining when the first galaxies formed remains an outstanding goal of modern observational astronomy. Theory and current stellar population models imply that the first galaxies…
PRUSSIC I - a JVLA survey of HCN/HCO+/HNC (1-0) emission in z3 dusty galaxies: Low dense-gas fractions in high-redshift star-forming galaxies
M. Rybak, J. A. Hodge, T. R. Greve +6
Dusty star-forming galaxies (DSFGs) at redshift z1 are among the most vigorously star-forming galaxies in the Universe. However, their dense (10 cm ) gas pha…