MESMER: MeerKAT Search for Molecules in the Epoch of Reionization
ArXiv e-prints (2011)
DETECTING COLD GAS AT z=3 WITH THE ATACAMA LARGE MILLIMETER/SUBMILLIMETER ARRAY AND THE SQUARE KILOMETER ARRAY
ASTROPHYSICAL JOURNAL 743:1 (2011) ARTN 84
Further observations of the intermediate mass black hole candidate ESO 243-49 HLX-1
AIP Conference Proceedings 1248 (2010) 93-96
Abstract:
The brightest Ultra-Luminous X-ray source HLX-1 in the galaxy ESO 243-49 currently provides strong evidence for the existence of intermediate mass black holes. Here we present the latest multi-wavelength results on this intriguing source in X-ray, UV and radio bands. We have refined the X-ray position to sub-arcsecond accuracy. We also report the detection of UV emission that could indicate ongoing star formation in the region around HLX-1. The lack of detectable radio emission at the X-ray position strengthens the argument against a background AGN. © 2010 American Institute of Physics.Goonhilly: A new site for e-MERLIN and the EVN
Proceedings of Science 125 (2010)