activity
20062017
most citedA bright z=5.2 lensed submillimeter galaxy in the field of Abell 773: HLSJ091828.6+514223

133 citations · 332 across the 11 of their papers we have counts for

collaborators

10 papers

astro-ph.GA2017★ 55 cited

Gravitational lensing reveals extreme dust-obscured star formation in quasar host galaxies

H. R. Stacey, J. P. McKean, N. C. Robertson +8

We have observed 104 gravitationally-lensed quasars at with Herschel/SPIRE, the largest such sample ever studied. By targeting gravitational lenses, we probe intrinsic f…

astro-ph.CO2014★ 8 cited

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…

astro-ph.CO2012★ 21 cited

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:…

astro-ph.CO2012★ 133 cited

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…

astro-ph.CO2011★ 65 cited

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.…

astro-ph.CO2011★ 9 cited

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…