133 citations · 332 across the 11 of their papers we have counts for
7 papers · 1 filter
Measuring gravitational lens time delays using low-resolution radio monitoring observations
G. Gurkan, N. Jackson, L. V. E. Koopmans +2
Obtaining lensing time delay measurements requires long-term monitoring campaigns with a high enough resolution (< 1 arcsec) to separate the multiple images. In the radio, a limite…
Discovery of "Warm Dust" Galaxies in Clusters at z~0.3: Evidence for Stripping of Cool Dust in the Dense Environment?
T. D. Rawle, M. Rex, E. Egami +15
Using far-infrared imaging from the "Herschel Lensing Survey", we derive dust properties of spectroscopically-confirmed cluster member galaxies within two massive systems at z~0.3:…
A bright z=5.2 lensed submillimeter galaxy in the field of Abell 773: HLSJ091828.6+514223
F. Combes, M. Rex, T. D. Rawle +20
During our Herschel Lensing Survey (HLS) of massive galaxy clusters, we have discovered an exceptionally bright source behind the z=0.22 cluster Abell 773, which appears to be a st…
Water vapor emission reveals a highly obscured, star forming nuclear region in the QSO host galaxy APM08279+5255 at z=3.9
Paul P. van der Werf, Alicia Berciano Alba, Marco Spaans +6
We present the detection of four rotational emission lines of water vapor, from energy levels Eu/k= 101 - 454 K, in the gravitationally lensed z=3.9 QSO host galaxy APM08279+5255.…
A new perspective on the submillimetre galaxy MM 18423+5938 at redshift 3.9296 from radio continuum imaging
J. P. McKean, A. Berciano Alba, F. Volino +5
The bright submillimetre (sub-mm) galaxy MM 18423+5938 at redshift 3.9296 has been predicted from mid-infrared and millimetre photometry to have an exceptionally large total infrar…
Radio counterpart of the lensed sub-mm emission in the cluster MS0451.6-0305: new evidence for the merger scenario
A. Berciano Alba, L. V. E. Koopmans, M. A. Garrett +2
SMM J04542-0301 is an extended (~1 arcmin) sub-mm source located near the core of the cluster MS0451.6-0305. It has been suggested that part of its emission arises from the interac…