We have measured the clustering properties of low-redshift (z \u3c 0.3) submm galaxies detected at 250 μm in the Herschel-ATLAS science demonstration phase field. We selected a sample for which we have high-quality spectroscopic redshifts, obtained from reliably matching the 250-μm sources to a complete (for r \u3c 19.4) sample of galaxies from the GAMA data base. Both the angular and spatial clustering strength are measured for all z \u3c 0.3 sources as well as for five redshift slices with thickness Δz = 0.05 in the range 0.05 \u3c z \u3c 0.3. Our measured spatial clustering length r0 is comparable to that of optically selected, moderately star-forming (blue) galaxies: we find values around 5 Mpc. One of the redshift bins contains an inte...
We present measurements of the angular correlation function of galaxies selected from the first fiel...
We use the Herschel-ATLAS survey to conduct the first large-scale statistical study of the sub-mm pr...
We measure the two-point angular correlation function of a sample of 4289 223 galaxies with r < 19.4...
We have measured the clustering properties of low-redshift (z \u3c 0.3) submm galaxies detected at 2...
We have measured the clustering properties of low-redshift (z < 0.3) submm galaxies detected at 250 ...
We have measured the clustering properties of low-redshift (z < 0.3) submm galaxies detected at 250 ...
We have measured the clustering properties of low-redshift (z < 0.3) submm galaxies detected at 250 ...
We have measured the clustering properties of low-redshift (z <0.3) submm galaxies detected at 25...
We have measured the clustering properties of low-redshift (z < 0.3) submm galaxies detected at 250 ...
We present measurements of the angular correlation function of sub- millimetre (sub-mm) galaxies (SM...
We present measurements of the angular correlation function of sub-millimeter (sub-mm) galaxies (SMG...
We have measured the clustering properties of low-redshift (z Herschel-ATLAS science demonstration p...
We present measurements of the angular correlation function of galaxies selected from the first fiel...
We present measurements of the angular correlation function of galaxies selected from the first fiel...
We present measurements of the angular correlation function of galaxies selected from the first fiel...
We present measurements of the angular correlation function of galaxies selected from the first fiel...
We use the Herschel-ATLAS survey to conduct the first large-scale statistical study of the sub-mm pr...
We measure the two-point angular correlation function of a sample of 4289 223 galaxies with r < 19.4...
We have measured the clustering properties of low-redshift (z \u3c 0.3) submm galaxies detected at 2...
We have measured the clustering properties of low-redshift (z < 0.3) submm galaxies detected at 250 ...
We have measured the clustering properties of low-redshift (z < 0.3) submm galaxies detected at 250 ...
We have measured the clustering properties of low-redshift (z < 0.3) submm galaxies detected at 250 ...
We have measured the clustering properties of low-redshift (z <0.3) submm galaxies detected at 25...
We have measured the clustering properties of low-redshift (z < 0.3) submm galaxies detected at 250 ...
We present measurements of the angular correlation function of sub- millimetre (sub-mm) galaxies (SM...
We present measurements of the angular correlation function of sub-millimeter (sub-mm) galaxies (SMG...
We have measured the clustering properties of low-redshift (z Herschel-ATLAS science demonstration p...
We present measurements of the angular correlation function of galaxies selected from the first fiel...
We present measurements of the angular correlation function of galaxies selected from the first fiel...
We present measurements of the angular correlation function of galaxies selected from the first fiel...
We present measurements of the angular correlation function of galaxies selected from the first fiel...
We use the Herschel-ATLAS survey to conduct the first large-scale statistical study of the sub-mm pr...
We measure the two-point angular correlation function of a sample of 4289 223 galaxies with r < 19.4...