activity
19992007
most citedClustering of galaxies at 3.6 microns in the Spitzer Wide-area Infrared Extragalactic legacy survey

13 citations · 13 across the 6 of their papers we have counts for

collaborators
Showing 2007Show all

7 papers · 1 filter

astro-ph200755 cited

Galaxy Counts at 24 Microns in the SWIRE Fields

David L. Shupe, Michael Rowan-Robinson, Carol J. Lonsdale +21

This paper presents galaxy source counts at 24 microns in the six Spitzer Wide-field InfraRed Extragalactic (SWIRE) fields. The source counts are compared to counts in other fields…

astro-ph200713 cited

Clustering of galaxies at 3.6 microns in the Spitzer Wide-area Infrared Extragalactic legacy survey

I. Waddington, S. J. Oliver, T. S. R. Babbedge +11

We investigate the clustering of galaxies selected in the 3.6 micron band of the Spitzer Wide-area Infrared Extragalactic (SWIRE) legacy survey. The angular two-point correlation f…

astro-ph200775 cited

High-Redshift QSOs in the SWIRE Survey and the z~3 QSO Luminosity Function

Brian Siana, Maria del Carmen Polletta, Harding E. Smith +10

We use a simple optical/infrared (IR) photometric selection of high-redshift QSOs that identifies a Lyman Break in the optical photometry and requires a red IR color to distinguish…

astro-ph200721 cited

The contribution of very massive high-redshift SWIRE galaxies to the stellar mass function

S. Berta, C. J. Lonsdale, M. Polletta +18

(Abridged) We selected high-z massive galaxies at 5.8 microns, in the SWIRE ELAIS-S1 field (1 sq. deg.). Galaxies with the 1.6 microns stellar peak redshifted into the IRAC bands (…

astro-ph2007

Ultraluminous Infrared Galaxies at 1.5<z<3 occupy dark matter haloes of mass ~6x10^13 solar masses

D. Farrah, C. J. Lonsdale, C. Borys +9

We present measurements of the spatial clustering of ultraluminous infrared galaxies in two redshift intervals, 1.5<z<2.0 and 2<z<3. Both samples cluster strongly, with r_0=14.40+/…

astro-ph200742 cited

Obscured and unobscured AGN populations in a hard-X-ray selected sample of the XMDS survey

M. Tajer, M. Polletta, L. Chiappetti +16

Our goal is to probe the populations of obscured and unobscured AGN investigating their optical-IR and X-ray properties as a function of X-ray flux, luminosity and redshift within…