NewEvery arXiv paper, its researchers & institutions — mapped.
papers

Publications (27)

astro-ph.CO2014

Herschel-ATLAS/GAMA:How does the far-IR luminosity function depend on galaxy group properties?

Qi Guo, Cedric Lacey, Peder Norberg +14

astro-ph.CO2010

Which halos host Herschel-ATLAS galaxies in the local Universe?

Qi Guo, Shaun Cole, Cedric G. Lacey +40

astro-ph.CO2011

Herschel-ATLAS: Rapid evolution of dust in galaxies in the last 5 billion years

L. Dunne, H. Gomez, E. da Cunha +38

astro-ph.CO2010

Herschel-ATLAS: Dust temperature and redshift distribution of SPIRE and PACS detected sources using submillimetre colours

A. Amblard, A. Cooray, P. Serra +69

astro-ph.CO2010

The Detection of a Population of Submillimeter-Bright, Strongly-Lensed Galaxies

Mattia Negrello, R. Hopwood, G. De Zotti +86

astro-ph.GA2018

GAMA/H-ATLAS: The Local Dust Mass Function and Cosmic Density as a Function of Galaxy Type - A Benchmark for Models of Galaxy Evolution

R. A. Beeston, A. H. Wright, S. Maddox +22

astro-ph.CO2012

Herschel-ATLAS/GAMA: spatial clustering of low-redshift sub-mm galaxies

E. van Kampen, D. J. B. Smith, S. Maddox +44

astro-ph.CO2013

Galaxy And Mass Assembly (GAMA): Linking Star Formation Histories and Stellar Mass Growth

Amanda E. Bauer, A. M. Hopkins, M. Gunawardhana +23

astro-ph.CO2012

Herschel-ATLAS: VISTA VIKING near-IR counterparts in the Phase 1 GAMA 9h data

S. Fleuren, W. Sutherland, L. Dunne +38

astro-ph2007

The Shapes of Galaxy Groups

A. Robotham, S. Phillipps, R. de Propris

astro-ph.GA2019

On the observability of individual Population III stars and their stellar-mass black hole accretion disks through cluster caustic transits

Rogier A. Windhorst, M. Alpaslan, S. Andrews +44

astro-ph.CO2012

Galaxy And Mass Assembly (GAMA): The M-Z relation for galaxy groups

M. A. Lara-Lopez, A. M. Hopkins, A. Robotham +7

astro-ph.GA2018

The SAMI Galaxy Survey: Stellar and gas misalignments and the origin of gas in nearby galaxies

J. J. Bryant, S. M. Croom, J. van de Sande +16

astro-ph.CO2010

The Herschel-ATLAS: Evolution of the 250um luminosity function out to z=0.5

S. Dye, L. Dunne, S. Eales +65

astro-ph.CO2012

Herschel-ATLAS: Multi-wavelength SEDs and physical properties of 250 micron-selected galaxies at z < 0.5

D. J. B. Smith, L. Dunne, E. da Cunha +38

astro-ph.GA2018

The XXL Survey: XXVII. The 3XLSS point source catalogue

L. Chiappetti, S. Fotopoulou, C. Lidman +35

astro-ph.CO2011

H-ATLAS/GAMA: Dusty early-type galaxies and passive spirals

K. Rowlands, L. Dunne, S. Maddox +38

astro-ph.CO2010

Herschel-ATLAS: The far-infrared--radio correlation at z<0.5

Matt J. Jarvis, D. J. B. Smith, D. G. Bonfield +44

astro-ph.CO2018

The XXL Survey XX: The 365 cluster catalogue

C. Adami, P. Giles, E. Koulouridis +54

astro-ph.GA2015

H-ATLAS/GAMA: The nature and characteristics of optically red galaxies detected at submillimetre wavelengths

A. Dariush, S. Dib, S. Hony +39

astro-ph.GA2017

Galaxy and Mass Assembly (GAMA): Probing the merger histories of massive galaxies via stellar populations

I. Ferreras, A. M. Hopkins, M. L. P. Gunawardhana +13

astro-ph.GA2014

Herschel-ATLAS: Properties of dusty massive galaxies at low and high redshifts

K. Rowlands, L. Dunne, S. Dye +16

astro-ph.CO2017

The XXL Survey: XXIII. The Mass Scale of XXL Clusters from Ensemble Spectroscopy

A. Farahi, V. Guglielmo, A. E. Evrard +34

astro-ph.CO2013

GAMA/H-ATLAS: Linking the Properties of Sub-mm Detected and Undetected Early-Type Galaxies: I. z$\le$0.06 Sample

N. K. Agius, A. E. Sansom, C. C. Popescu +34

astro-ph.CO2011

Herschel-ATLAS: counterparts from the UV--NIR in the science demonstration phase catalogue

D. J. B. Smith, L. Dunne, S. J. Maddox +45

astro-ph.GA2017

The XXL Survey: XXII. The XXL-North spectrophotometric sample and galaxy stellar mass function in X-ray detected groups and clusters

V. Guglielmo, B. M. Poggianti, B. Vulcani +42

astro-ph.GA2018

The XXL Survey: XXX. Characterisation of the XLSSsC N01 supercluster and analysis of the galaxy stellar populations

V. Guglielmo, B. M. Poggianti, B. Vulcani +34