800 citations · 8.7k across the 102 of their papers we have counts for
101 papers
On the Dust properties of the UV galaxies in the redshift range
M. Sharma, M. J. Page, M. Symeonidis +1
Far-infrared observations from the \textit{Herschel Space Observatory} are used to estimate the infrared (IR) properties of ultraviolet-selected galaxies. We stack the PACS (100, 1…
ACOSMOS: the infrared luminosity function and dust-obscured star formation rate density at
A. Traina, C. Gruppioni, I. Delvecchio +16
Aims: We leverage the largest available Atacama Large Millimetre/submillimetre Array (ALMA) survey from the archive (ACOSMOS) to study to study infrared luminosity function and…
The star-formation rates of QSOs
M. Symeonidis, N. Maddox, M. J. Jarvis +13
We examine the far-IR properties of a sample of 5391 optically selected QSOs in the 0.5<z<2.65 redshift range down to log[nuLnu,2500 (erg/s)]>44.7, using SPIRE data from Herschel-A…
On the intrinsic AGN emission in far-infrared/sub-mm
M. Symeonidis
Far-infrared (far-IR)/sub-mm emission linked to AGN-heated dust has been a topic of contention for many years. Results have been diverse and various views have been presented. The…
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…
Photoionisation Modelling of the X-ray Emission Line Regions within the Seyfert 2 AGN NGC 1068
S. Grafton-Waters, G. Branduardi-Raymont, M. Mehdipour +4
We investigate the photoionised X-ray emission line regions (ELRs) within the Seyfert 2 galaxy NGC 1068, to determine if there are any characteristic changes between observations t…