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Roger Blandford

Researcher at Stanford University

Publications -  716
Citations -  97353

Roger Blandford is an academic researcher from Stanford University. The author has contributed to research in topics: Galaxy & Fermi Gamma-ray Space Telescope. The author has an hindex of 156, co-authored 704 publications receiving 90181 citations. Previous affiliations of Roger Blandford include SLAC National Accelerator Laboratory & Max Planck Society.

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Intrinsic and Extrinsic Galaxy Alignment

TL;DR: In this article, the authors show that the assumption of uncorrelated intrinsic ellipticities of target sources that is usually made in searches for weak gravitational lensing due to large-scale mass inhomogeneities (''field lensing'') is unwarranted.
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Electromagnetic Models of Compact Radio Sources and Circular Polarisation

TL;DR: In this paper, an electromagnetic model of relativistic jets is proposed and it is suggested that these jets are interpreted as current flows and that they owe their persistence and collimation to the pinching action of the magnetic field.

UV-optical from space

TL;DR: In this article, the authors discuss the science program (star formation and origins of planetary systems, structure and evolution of the interstellar medium, stellar population, the galactic and extragalactic distance scale, nature of galaxy nuclei, AGNs, and QSOs), formation of galaxies at high redshifts, and cosmology).
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On The Jets Associated with Galactic Superluminal Sources

TL;DR: In this article, the physical conditions within these Galactic sources, their interaction with their environment, their possible formation, and contrast them with their extragalactic counterparts are examined, and constraints on particle acceleration in the jets are imposed using X-ray and radio observations, the $\gamma$-ray flux from e$+$-e$^-$ jets expected at EGRET energies and the flux in infrared lines from an e-p jet are estimated.
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Hydromagnetic Wind Model for the Broad-Line Region of NGC 5548

TL;DR: A hydromagnetic wind model from a dusty molecular disk (Emmering, Blandford, & Shlosman 1992) was applied to the BLR in NGC 5548 and produced synthetic C IV line profiles as a function of time as discussed by the authors.