activity
19972025
most citedThe XMM-Newton Optical/UV Monitor Telescope

685 citations · 1.9k across the 24 of their papers we have counts for

collaborators

24 papers

astro-ph.GA2025

The ultraviolet luminosity function of star-forming galaxies between redshifts of 0.4 and 0.6

M. J. Page, T. Dwelly, I. McHardy +7

We combine ultraviolet imaging of the 13H survey field, taken with the XMM-Newton Optical Monitor telescope (XMM-OM) and the Neil Gehrels Swift Observatory Ultraviolet and Optical…

astro-ph.GA2021★ 11 cited

The ultraviolet luminosity function of star-forming galaxies between redshifts of 0.6 and 1.2

M. J. Page, T. Dwelly, I. McHardy +11

We use ultraviolet imaging taken with the XMM-Newton Optical Monitor telescope (XMM-OM), covering 280 square arcminutes in the UVW1 band (effective wavelength 2910 Angstroms) to me…

astro-ph2006★ 11 cited

A Search for EUV Emission from Comets with the Cosmic Hot Interstellar Plasma Spectrometer (CHIPS)

T. P. Sasseen, M. Hurwitz, C. M. Lisse +5

We have obtained EUV spectra between 90 and 255 Åof the cometsC/2002 T7 (LINEAR), C/2001 Q4 (NEAT), and C/2004 Q2 (Machholz) near their perihelion passages in 2004 with the Cosmic…

astro-ph2006★ 39 cited

X-ray spectra of sources in the 13H XMM-Newton / Chandra deep field

M. J. Page, N. S. Loaring, T. Dwelly +8

We present the X-ray spectra of 86 optically-identified sources in the 13H XMM-Newton/Chandra deep field which have >70 X-ray counts. The sample consists of 50 broad line AGN, 25 n…

astro-ph2005★ 29 cited

XMM-Newton 13H Deep field - I. X-ray sources

N. S. Loaring, T. Dwelly, M. J. Page +10

We present the results of a deep X-ray survey conducted with XMM-Newton, centred on the UK ROSAT 13H deep field area. This region covers 0.18 deg^2 and is the first of two areas co…

astro-ph2005★ 18 cited

Constraints on the distribution of absorption in the X-ray selected AGN population found in the 13H XMM-Newton/Chandra deep field

T. Dwelly, M. J. Page, N. S. Loaring +4

We present an analysis of the X-ray properties of sources detected in the 13H XMM-Newton deep (200ks) field. In order to constrain the absorbed AGN population, we use extensive Mon…