Add to ORKGAbstract. The study of supernova remnants and pulsar wind nebulae was one of the Key Science Projects for the first two years of VERITAS ob-servations. VERITAS is an array of four imaging Cherenkov telescopes located at the Whipple Ob-servatory in southern Arizona. Supernova remnants are widely considered to be the strongest candidate for the source of cosmic rays below the knee at around 1015 eV. Pulsar wind nebulae are synchrotron nebulae powered by the spin-down of energetic young pulsars, and comprise one of the most populous very-high-energy gamma-ray source classes. This poster will summarize the results of this observation program
University of Minnesota Ph.D. dissertation. October 2009. Major: Astrophysics. Advisors: Charles E. ...
We present evidence that the very high energy (VHE, E > 100 GeV) gamma-ray emission coinciden...
Recent advances in very-high-energy (VHE) gamma-ray astronomy have opened a new observational window...
Abstract: Shell-type supernova remnants (SNRs) accelerate particles at the shock front between the e...
International audienceIn the past few years, gamma-ray astronomy has entered a golden age thanks to ...
The nature and source of cosmic rays has been at the core of particle astrophysics since their disco...
Observations of TeV gamma rays enable investigation of extreme, high-energy astrophysical environmen...
AbstractVERITAS is a ground-based gamma-ray observatory consisting of an array of four atmospheric C...
Pulsars have been known to exist for over forty years now, but the nature of their emission througho...
Pulsars are known to power winds of relativistic particles that can produce bright nebulae by intera...
The VERITAS observatory is an imaging atmospheric Cherenkov telescope array located in southern Ariz...
Abstract. VERITAS is an imaging atmospheric Cherenkov telescope array carrying out observations of t...
The VERITAS telescope array has been operating smoothly since 2007, and has detected gamma-ray emiss...
The role pulsar wind nebulae play in producing our locally observed cosmic ray spectrum remains murk...
The Very Energetic Radiation Imaging Telescope Array System (VERITAS) is the major next generation i...
University of Minnesota Ph.D. dissertation. October 2009. Major: Astrophysics. Advisors: Charles E. ...
We present evidence that the very high energy (VHE, E > 100 GeV) gamma-ray emission coinciden...
Recent advances in very-high-energy (VHE) gamma-ray astronomy have opened a new observational window...
Abstract: Shell-type supernova remnants (SNRs) accelerate particles at the shock front between the e...
International audienceIn the past few years, gamma-ray astronomy has entered a golden age thanks to ...
The nature and source of cosmic rays has been at the core of particle astrophysics since their disco...
Observations of TeV gamma rays enable investigation of extreme, high-energy astrophysical environmen...
AbstractVERITAS is a ground-based gamma-ray observatory consisting of an array of four atmospheric C...
Pulsars have been known to exist for over forty years now, but the nature of their emission througho...
Pulsars are known to power winds of relativistic particles that can produce bright nebulae by intera...
The VERITAS observatory is an imaging atmospheric Cherenkov telescope array located in southern Ariz...
Abstract. VERITAS is an imaging atmospheric Cherenkov telescope array carrying out observations of t...
The VERITAS telescope array has been operating smoothly since 2007, and has detected gamma-ray emiss...
The role pulsar wind nebulae play in producing our locally observed cosmic ray spectrum remains murk...
The Very Energetic Radiation Imaging Telescope Array System (VERITAS) is the major next generation i...
University of Minnesota Ph.D. dissertation. October 2009. Major: Astrophysics. Advisors: Charles E. ...
We present evidence that the very high energy (VHE, E > 100 GeV) gamma-ray emission coinciden...
Recent advances in very-high-energy (VHE) gamma-ray astronomy have opened a new observational window...