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MULTIWAVELENGTH BEHAVIOUR OF THE BLAZAR OJ 248 FROM RADIO TO γ− RAYS M. I. Carnerero1,2, C. M. Raiteri1, M. Villata1, J. A. Acosta-Pulido2, V. M. Larionov3 for the GASP-WEBT collaboration 1 2
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Document Date: 2015-05-26 01:48:08


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City

Lulin / Lowell / Crimean / Steward / St. Petersburg / Calar Alto / San Pedro Martir / /

Company

SMA / IRAM / Loral / /

Country

Russia / Italy / Spain / /

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Event

M&A / /

Facility

Isaac Newton Institute of Chile / Steward Observatory / Pulkovo Observatory / /

IndustryTerm

gas velocity / energy range / gas clouds / energy density / low-energy / high-energy data / /

MusicGroup

X-ray / /

OperatingSystem

Fermi / /

Organization

Universidad de La Laguna / Instituto de Astrofisica de Canarias / St.-Petersburg State Univ. / Isaac Newton Institute of Chile / /

Person

Campo Imperatore / Teide / Massimo Villata / /

Position

WEBT President / /

RadioStation

WEBT / /

Technology

alpha / radiation / broadband / X-ray / SPECTROSCOPY / /

URL

http /

SocialTag