activity
20092017
most citedThe Second Data Release of the INT Photometric H-Alpha Survey of the Northern Galactic Plane (IPHAS DR2)

177 citations · 736 across the 13 of their papers we have counts for

collaborators

13 papers

astro-ph.IM2017★ 146 cited

The VISTA ZYJHKs Photometric System: Calibration from 2MASS

Carlos González-Fernández, Simon T. Hodgkin, Michael J. Irwin +7

In this paper we describe the routine photometric calibration of data taken with the VIRCAM instrument on the ESO VISTA telescope. The broadband ZYJHKs data are directly calibrated…

astro-ph.GA2016★ 29 cited

The 2QDES Pilot : The luminosity and redshift dependence of quasar clustering

Ben Chehade, T. Shanks, J. Findlay +10

We present a new redshift survey, the 2dF Quasar Dark Energy Survey pilot (2QDESp), which consists of quasars from deg of the southern sky, base…

astro-ph.GA2016★ 5 cited

Calibrated and completeness-corrected optical stellar density maps of the Northern Galactic Plane

H. J. Farnhill, J. E. Drew, G. Barentsen +1

Following on from the second release of calibrated photometry from IPHAS, the INT/WFC Photometric H-alpha Survey of the Northern Galactic Plane, we present incompleteness-corrected…

astro-ph.GA2015★ 23 cited

The shell game: a panoramic view of Fornax

N. F. Bate, B. McMonigal, G. F. Lewis +4

We present a panoramic study of the Fornax dwarf spheroidal galaxy, using data obtained as part of the VLT Survey Telescope (VST) ATLAS Survey. The data presented here -- a subset…

astro-ph.GA2015★ 88 cited

Two bright z > 6 quasars from VST ATLAS and a new method of optical plus mid-infra-red colour selection

A. C. Carnall, T. Shanks, B. Chehade +6

We present the discovery of two z > 6 quasars, selected as i band dropouts in the VST ATLAS survey. Our first quasar has redshift, z = 6.31 \pm 0.03, z band magnitude, z_AB = 19.63…

astro-ph.SR2014★ 80 cited

The Gaia-ESO Survey: Stellar content and elemental abundances in the massive cluster NGC 6705

T. Cantat-Gaudin, A. Vallenari, S. Zaggia +52

Chemically inhomogeneous populations are observed in most globular clusters, but not in open clusters. Cluster mass seems to play a key role in the existence of multiple population…