Number of items: 2.
The dust and [CII] morphologies of redshift ~4.5 sub-millimeter galaxies at ~200pc resolution : The Absence of Large Clumps in the Interstellar Medium at High-redshift. (2018)
B. Gullberg,
A. M. Swinbank,
I. Smail,
A. D. Biggs,
F. Bertoldi,
C. De Breuck,
S. C. Chapman,
C. -C. Chen,
E. A. Cooke,
K. E. K. Coppin,
P. Cox,
H. Dannerbauer,
J. S. Dunlop,
A. C. Edge,
D. Farrah,
J. E. Geach,
T. R. Greve,
J. Hodge,
E. Ibar,
R. J. Ivison,
A. Karim,
E. Schinnerer,
D. Scott,
J. M. Simpson,
S. M. Stach,
A. P. Thomson,
P. van der Werf,
F. Walter,
J. L. Wardlow
and
A. Weiss
Why z > 1 radio-loud galaxies are commonly located in protoclusters. (2014)
N. A. Hatch,
D. Wylezalek,
J. D. Kurk,
D. Stern,
C. De Breuck,
M.J. Jarvis,
A. Galametz,
A. H. Gonzalez,
W. G. Hartley,
A. Mortlock,
N. Seymour
and
J. A. Stevens
grid_on
This list was generated on Sun Apr 19 01:24:46 2026 BST.