The radio galaxy K-z relation to z ~ 4.5
ArXiv astro-ph/0103364 (2001)
Abstract:
Using a new radio sample, 6C* designed to find radio galaxies at z > 4 along with the complete 3CRR and 6CE sample we extend the radio galaxy K-z relation to z~4.5. The 6C* K-z data significantly improve delineation of the K-z relation for radio galaxies at high redshift (z > 2). Accounting for non-stellar contamination, and for correlations between radio luminosity and estimates of stellar mass, we find little support for previous claims that the underlying scatter in the stellar luminosity of radio galaxies increases significantly at z > 2. This indicates that we are not probing into the formation epoch until at least z > 3.Cygnus X-3 with ISO: investigating the wind
Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 322:1 (2001) 177-186
Powerful jets from black hole X-ray binaries in low/hard X-ray states
Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 322:1 (2001) 31-42
X-ray states and radio emission in the black hole candidate XTE J1550-564
(2001)
Correlated X-Ray Spectral and Timing Behavior of the Black Hole Candidate XTE J1550–564: A New Interpretation of Black Hole States
The Astrophysical Journal Supplement Series American Astronomical Society 132:2 (2001) 377-402