'Phase bins' diaporamas de présentation

SKA Central Signal Processor Architecture

SKA Central Signal Processor Architecture. SKA CSP LMC Peer Review 11.April , 2016, Madrid. Sonja Vrcic. SKA CSP LMC Sub-element Lead. List of topics to address as a part of this review. CSP Architecture CSP Control Context Detail CSP Monitor and Control Architecture

925 views • 51 slides

X-RAY IMAGING PRACTICUM

X-RAY IMAGING PRACTICUM. Brian Dennis, GSFC Gordon Hurford, UCB. X-RAY IMAGING PRACTICUM. Objectives Intuitive perspective on RMC imaging Introduction to some real-world hardware and design considerations

568 views • 43 slides

Introduction to Visibilities

231 views • 23 slides

The Stacker

The Stacker. Gordon Hurford, Ed Schmahl, Richard Schwartz 18-April-2005. What is the Stacker?. Current imaging algorithms based on time-binned event lists Time bins must be very short (~1-100ms) to preserve modulation Few events per bin (statistics, display, Forward Fit issues)

575 views • 18 slides

Problem with VELA light curve

Dave reported that the pulsar light curves look ragged. Try to reproduce the seen effect: I downloaded VELA data from GSSC > Select all photons within a 1 deg radius around VELA I corrected the photon arrival times with gtbary I computed the pulsar phase with gtpphase

169 views • 2 slides