We review how the recent increase in X-ray and radio data from black hole and neutron star
binaries can be merged together with theoretical advances to give a coherent picture of the …

RNA-seq is now the technology of choice for genome-wide differential gene expression
experiments, but it is not clear how many biological replicates are needed to ensure valid …

We systematically analyse all publicly available XMM–Newton spectra of radio-quiet PG
quasars. The soft X-ray excess in these objects is well modelled by an additional, cool, …

… 3 ml 0.25 m sucrose, 10 mm MgCl 2, and layered over 3 ml 0.35 m sucrose, 0.5 mm MgCl 2
… The clean, pelleted nuclei were resuspended in 3 ml 0.35 m sucrose, 0.5 mm MgCl 2 , and …

We present X-ray/γ-ray spectra of Cyg X-1 observed during the transition from the hard to
the soft state and in the soft state by ASCA, RXTE and CGRO/OSSE in 1996 May and June. …

Active galactic nuclei and quasars are thought to be scaled-up versions of Galactic black hole
binaries, powered by accretion onto supermassive black holes with masses of 10 6 –10 9 , …

… Each labeled probe, 150 ng, was precipitated in ethanol and 0.3 M sodium acetate
together with 10 μg COT1 carrier DNA (Invitrogen) and dissolved in 10 μl hybridization buffer (…

… , we consider masses between M= 1.0 M ⊙ and 1.6 M ⊙ . Masses in the range of 1.4–1.6 …
of the compact object M≲ 1.6 M ⊙ . We also put the lower limit of M≳ 1.2 M ⊙ on the stellar …

… There are no constraints for mass or distance for this source and we assume that M= 10 M⊙…
There are no constraints for mass or distance for this source and we assume that M= 10 M ⊙ …

We build a simple model of the optical/ultraviolet (UV) emission from irradiation of the outer
disc by the inner disc and coronal emission in black hole binaries. We apply this to the broad-…