125 citations · 125 across the 2 of their papers we have counts for
19 papers
High resolution observations of HCN and HCO+ J=3-2 in the disk and outflow of Mrk231 -Detection of vibrationally excited HCN in the warped nucleus
S. Aalto, S. Garcia-Burillo, S. Muller +6
We obtained high resolution (0."25 to 0."90) observations of HCN and HCO+ J=3-2 of the ultraluminous QSO galaxy Mrk231 with the IRAM Plateau de Bure Interferometer. We find luminou…
The IRAM M33 CO(2-1) Survey - A complete census of the molecular gas out to 7 kpc
C. Druard, J. Braine, K. F. Schuster +11
In order to study the ISM and the interplay between the atomic and molecular components in a low-metallicity environment, we present a complete high angular and spectral resolution…
The SCUBA-2 Cosmology Legacy Survey: Ultraluminous star-forming galaxies in a z=1.6 cluster
Ian Smail, J. E. Geach, A. M. Swinbank +23
We analyse new SCUBA-2 submillimeter and archival SPIRE far-infrared imaging of a z=1.62 cluster, Cl0218.3-0510, which lies in the UKIDSS/UDS field of the SCUBA-2 Cosmology Legacy…
Gravitational Lens Models Based on Submillimeter Array Imaging of Herschel-selected Strongly Lensed Sub-millimeter Galaxies at z>1.5
R. S. Bussmann, I. Perez-Fournon, S. Amber +46
Strong gravitational lenses are now being routinely discovered in wide-field surveys at (sub)millimeter wavelengths. We present Submillimeter Array (SMA) high-spatial resolution im…
[CII] and 12CO(1-0) Emission Maps in HLSJ091828.6+514223: A Strongly Lensed Interacting System at z=5.24
T. D. Rawle, E. Egami, R. S. Bussmann +25
We present Submillimeter Array (SMA) [CII] 158um and Jansky Very Large Array (JVLA) CO(1-0) line emission maps for the bright, lensed, submillimeter source at beh…
Herschel-ATLAS: a binary HyLIRG pinpointing a cluster of starbursting proto-ellipticals
R. J. Ivison, A. M. Swinbank, Ian Smail +48
Panchromatic observations of the best candidate HyLIRG from the widest Herschel extragalactic imaging survey have led to the discovery of at least four intrinsically luminous z=2.4…