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The Innuos PULSAR addresses power isolation in a thorough and thoughtful manner. The PULSAR contains three independent power rails, one for the USB reclocker, one for the main board and one for the SSD. It’s an incredibly quiet box, adding to that illusion of a solid billet–the PULSAR ma...
where polarization can exceed 60% at the leading edge—approaching the theoretical limit of what can be produced by synchrotron emission. We infer that, in contrast with the case of the supernova remnant, the electrons in the pulsar wind nebula are accelerated with little or no turbulence in ...
Since it appears PTAs are approaching a detection, typically the scaling law is presumed to be the following [179], [211]: (1)S/N∝NTACσ3/13,where S/N is the signal-to-noise ratio of the GWB in the data, N is the number of pulsars in the array, T is the timing baseline of...
The small radial extent and nearly round shape\nof the putative PWN can be explained if the pulsar is receding (or approaching)\nin the direction close to the line of sight. The very soft spectrum of the\nextended emission ($\\Gamma\\sim 8$), much softer than those of typical PWNe,\...
Pulsar's growth has skyrocketed globally since it became a top-level Apache Project inSeptember 2018. According to Docker Hub,Apache Pulsar has more than 10 million downloads.On Github, the project is approaching 7,000 stars and currently has over 330 contributors. ...
discovery the system's orbital period had decreased by about 76 millionths of a second per year - this means that the pulsar was approaching its maximum separation more than a second earlier than it would have if the orbit had remained the same. Subsequent observations continue to show this ...
The small radial extent and nearly round shape of the putative PWN can be explained if the pulsar is receding (or approaching) in the direction close to the line of sight. The very soft spectrum of the extended emission ($\\\Gamma\\\sim 8$), much softer than those of typical PWNe, ...
In strong shocks, particles in either the preshock or postshock fluid have scattering centers such that they experience only approaching collisions. This allows energy gains of first-order as particles cross the shock front, with a spectrum that depends only on the shock compression ratio as expla...
As Nvidia and other manufacturers develop technology to cater to new displays, the Video Electronics Standards Association (VESA) has made changes to how it’s approaching the future of monitors. At the beginning of January 2024, VESA announced updates to its Adaptive-Sync Display Compliance Test ...