Candidate Isolated Neutron Stars and Other Optically Blank X-Ray Fields Identified from the ROSAT All-Sky and Sloan Digital Sky Surveys**Includes observations obtained with the Apache Point Observatory 3.5 m telescope, which is owned and operated by the Astrophysical Research Consortium.
The Astronomical Journal American Astronomical Society 131:3 (2006) 1740-1749
Adapting and expanding interferometric arrays
ArXiv astro-ph/0602578 (2006)
Abstract:
We outline here a simple yet efficient method for finding optimized configurations of the elements of radio-astronomical interferometers with fixed pad locations. The method can be successfully applied, as we demonstrate, to define new configurations when changes to the array take place. This may include the addition of new pads or new antennas, or the loss of pads or antennas. Our method is based on identifying which placement of elements provides the most appropriate uv plane sampling for astronomical imaging.Jets in neutron star X-ray binaries: a comparison with black holes
Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 366:1 (2006) 79-91
Opening angles, Lorentz factors and confinement of X-ray binary jets
(2006)