PPT-Pulsar broadening measurements

at low frequencies with LOFAR Kimon Zagkouris University of Oxford In collaboration with the LOFAR Pulsar Working Group Ierapetra June 2014 Image Credit David A Aguilar CfA NASA ESA. Staff Workshop. Introduction. Discussion Groups/Feedback. curriculum.leeds.ac.uk. Broadening Strand Definition . A Broadening Strand is:. ‘A co-ordinated and structured series of related elective modules allowing sustained exploration of a specific subject, issue or skill which lies beyond the primary disciplinary content of a student’s programme.’. Megan . DeCesar (UWM). In collaboration with Scott Ransom (NRAO), Paul Ray (NRL), Paul Demorest (NRAO), David Kaplan (UWM), and the . Fermi. LAT Collaboration. Discovery of a Highly Eccentric Binary Millisecond Pulsar. High Energy & Cosmic Ray Research Ctr.. North Bengal University. TeV Neutrinos and Gamma rays from Pulsars/Magnetars. Introduction. The energy spectrum of cosmic rays extends to extremely high energies, values exceeding 10. The Pulsar Search Collaboratory. Questions We Will Answer. What is a . pulsar. ?. Why do astronomers study pulsars?. What is the . PSC. ?. How can . you. get involved?. What is a pulsar?. A pulsar is a . Shockingly Bright Pulsar. Developed by the . NuSTAR. EPO Group. at. Sonoma State University. 0. Topic: . Pulsars, X-rays, black holes. Concepts: . multi-wavelength observations, galactic and stellar . PULSAR PROPERTIES:. High Space Velocity . Rapid Spin Rate. Super Dense. Strong Gravitational Field. Strong Magnetic Field . Jocelyn Bell. “Little Green Men” Theory. Chandrasekhar Mass Limit. 1.4 solar masses =. is a supernova remnant which is a super dense, . rapidly spinning neutron star which emits . dipole electromagnetic . radiation and features a strong magnetic and gravitational . field and also high space velocity. . overview. Caroline Campbell (Languages and Cross-Cultural Understanding). Fiona Douglas (Media, Culture and Creativity). Rafe. Hallett (Personal and Professional Development). Bonnie Meekums (Mind and Body). with a Pulsar . T. iming Array. Lindley . Lentati. Cambridge University . Gravitational Waves. Fluctuations in curvature that propagate at the speed of light. Experiment . in the lab:. Using an accurate clock, record when you measure ticks. . S. R. Kulkarni. Supernova . remnan. . The blue emission is X-ray and arises. from relativistic electrons. Red (. Xray. ). Green Forbidden Optical Line. Guitar nebula: Pulsar traveling at 2000 km/s. Charge exchange!. w. eb . Ryan Shannon, . ICRAR-Curtin/. ATNF (. Vikram. Ravi, Swinburne . Pulsar . Group). Outline. Fast radio bursts (. FRBs) . Exciting times!. FRB 131104 . The . (improbable/real-time) . discovery of an FRB to the Carina dwarf spheroidal. Monoxide and Nitrous Oxide Measured by Terahertz Time-Domain Spectroscopy. Presentation to the 11. th. HITRAN Database Conference, 2010, Cambridge, MA, USA. 16 June, 2010. Weston Aenchbacher. 1. , Mira Naftaly. Jelle Kaastra. with. . Ton . Raassen. , . Liyi. . Gu. , . Junjie. Mao, . Igone. . Urdampilleta. , . Missagh. . Mehdipour. SRON & Leiden University. Introduction. X-ray emitting plasmas everywhere:. In the vibrant city of Bangalore, where the roads are alive with the buzz of motorcycles weaving through traffic, owning a reliable two-wheeler is often a necessity. Among the popular choices for commuters and bike enthusiasts alike is the Bajaj Pulsar 150, known for its robust performance, sleek design, and affordable price tag. If you\'re in the market for a used Bajaj Pulsar 150 in Bangalore, this comprehensive guide will walk you through everything you need to know to make an informed purchase decision.