<--- Back to Details
First PageDocument Content
Space / Matter / Radio astronomy / Rotating radio transient / Allen Telescope Array / Neutron star / Dispersion / Pulse-width modulation / Analog-to-digital converter / Astronomy / Star types / Pulsars
Date: 2011-09-13 20:56:36
Space
Matter
Radio astronomy
Rotating radio transient
Allen Telescope Array
Neutron star
Dispersion
Pulse-width modulation
Analog-to-digital converter
Astronomy
Star types
Pulsars

The Allen Telescope Array Fly’s Eye Survey for Fast Radio Transients Andrew P.V. Siemion1 , Geoffrey C. Bower1 , Griffin Foster2 , Peter L. McMahon3 , Mark I. Wagner1 , Dan Werthimer1 , Don Backer1 , Jim Cordes4 , Joer

Add to Reading List

Source URL: arxiv.org

Download Document from Source Website

File Size: 2,74 MB

Share Document on Facebook

Similar Documents

Origin of the Heavy Elements in a Neutron Star Merger Daniel Kasen (UC Berkeley/Lawrence Berkeley Laboratory) The Origin of the Elements Big

Origin of the Heavy Elements in a Neutron Star Merger Daniel Kasen (UC Berkeley/Lawrence Berkeley Laboratory) The Origin of the Elements Big

DocID: 1vlp7 - View Document

RIKEN-RESCEU joint seminar Contribution of Neutron-Star Merger to the R-process Chemical Evolution

RIKEN-RESCEU joint seminar Contribution of Neutron-Star Merger to the R-process Chemical Evolution

DocID: 1vdNt - View Document

Heavy Element Production and Neutrino-Driven Jets in Neutron-Star Merger Oliver Just Max-Planck-Institut für Astrophysik, Garching, Germany

Heavy Element Production and Neutrino-Driven Jets in Neutron-Star Merger Oliver Just Max-Planck-Institut für Astrophysik, Garching, Germany

DocID: 1v3mB - View Document

THE MEASUREMENT OF THE NEUTRON STAR RADIUS

THE MEASUREMENT OF THE NEUTRON STAR RADIUS

DocID: 1v0Aq - View Document

Nuclear Waffles in Neutron Star Crust Objectives  Use large scale GPU computing to perform detailed MD simulations of dense neutron rich matter.  Explore complex nuclear pasta phases in the crust of neutron stars.

Nuclear Waffles in Neutron Star Crust Objectives  Use large scale GPU computing to perform detailed MD simulations of dense neutron rich matter.  Explore complex nuclear pasta phases in the crust of neutron stars.

DocID: 1uSGG - View Document