THE NuSTAR EXTRAGALACTIC SURVEY: A FIRST SENSITIVE LOOK AT THE HIGH ENERGY COSMIC X RAY BACKGROUND POPULATION

Roughly 50% of the PNe observed by Chandra harbor X-ray-luminous CSPNe, while soft, diffuse X-ray emission tracing shocks—in most cases, “hot bubbles”—formed by energetic

We remind the data were taken during 10 different observing sessions spanned in an orbital cycle in August/September 1992 simultaneously with 6 cm and X-ray data of the source

Upon viewing each work, I took the measurements of the matrix (image), overall sheet size (as measured), photographed it and categorized it in the following ways: as an

The cation distribution and magnetic properties of electrosynthetized cobalt ferrite nanoparticles have been studied by means of X-Ray Absortion and Mössbauer spectroscopy,

The three Cycle 14 X-ray point source detections (HbDs1, NGC 6337, Sp 1) continue the trend, noted in Paper I, that soft (∼0.6–1.0 keV) X-ray sources likely indicate the presence

We used a large set of numerically simulated clusters for which the X-ray and the lensing properties were previously investi- gated, and compared their Einstein ring sizes

Energy-dispersive X-ray microanalysis showed the cell walls to be the main area of Cu binding in the inner and outer cortex and infected zone of white lupin

The time selection for the following sources is based entirely on their X-ray behaviour, by taking into account the disk-jet coupling just described. Only periods of hard X-ray