On the peak radio and X-ray emission from neutron star and black hole candidate X-ray transients
(2001)
A 350GHz radial-probe SIS mixer for astronomical imaging arrays
International Journal of Infrared and Millimeter Waves 22:9 (2001) 1305-1312
Abstract:
We have developed a 330-370GHz SIS mixer for small-format, heterodyne, astronomical imaging arrays. Fixed-tuned broadband operation is achieved by means of a superconducting radial waveguide probe. A horn-reflector antenna provides high-efficiency optical coupling. Using a variable-temperature cryogenic noise source, we measured a DSB system noise temperature of 32±1K. The mixer contributes 3±3K, supporting the theoretically-predicted result that the noise temperature of a DSB mixer can be less than (Latin small letter hwith stroke)ω/2k (8.6K). © 2001 Plenum Publishing Corporation.Energetics of jets from X-ray binaries
Astrophysics and Space Science Springer Nature 276:Suppl 1 (2001) 69-77
Jets in XRB Low/Hard States: Models of XTE J1118+480 Suggest a Strong Signature from Radio through X-Ray
Astrophysics and Space Science Springer Nature 276:Suppl 1 (2001) 289-290
The 1997 Hard State Outburst of the X-Ray Transient GS 1354-64 / BW CIR
Astrophysics and Space Science Springer Nature 276:Suppl 1 (2001) 117-120