The discovery of a type II quasar at z = 1.65 with integral-field spectroscopy
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 358:1 (2005) L11-L15
What can we learn from neutron star X-ray binaries’ jets?
Chapter in Astrophysics and Space Science, Springer Nature (2005) 197-209
Precise measurement of CMB polarisation from Dome-C: the BRAIN and CLOVER experiments
ArXiv astro-ph/0412590 (2004)
Source subtraction for the extended Very Small Array and 33-GHz source count estimates
ArXiv astro-ph/0412605 (2004)
Abstract:
We describe the source subtraction strategy and observations for the extended Very Small Array, a CMB interferometer operating at 33 GHz. A total of 453 sources were monitored at 33 GHz using a dedicated source subtraction baseline. 131 sources brighter than 20 mJy were directly subtracted from the VSA visibility data. Some characteristics of the subtracted sources, such as spectra and variability, are discussed. The 33-GHz source counts are estimated from a sample selected at 15 GHz. The selection of VSA fields in order to avoid bright sources introduces a bias into the observed counts. This bias is corrected and the resulting source count is estimated to be complete in the flux-density range 20-114 mJy. The 33-GHz source counts are used to calculate a correction to the VSA power spectrum for sources below the subtraction limit.On the Origin of Radio Emission in the X-Ray States of XTE J1650–500 during the 2001-2002 Outburst
The Astrophysical Journal American Astronomical Society 617:2 (2004) 1272-1283