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First year results of the High Altitude Water Cherenkov observatory Alberto Carramiñana - for the HAWC Collaboration Instituto Nacional de Astrof́ısica, Óptica y Electrónica,…
The structure of radio pulsars with interpulses malov@praoru maggika@mailru IF Malov EB Nikitina Pushchino Radio Astronomy Observatory Physical Institute of the Russian Academy…
Multi-wavelength multi-site Monitoring of Gamma-Ray Burst-associated Supernovae 19 July 2012 Burst-associated Supernovae Elena Pian INAF-Trieste Astronomical Observatory…
Slide 1 The DDO photometric system1 It was developed at the David Dunlap Observatory near Toronto by McClure & van den Bergh (1968) It was developed at the David Dunlap…
Daya Bay II: Jiangmen Underground Neutrino Observatory JUNO Xiaonan Li Institute of High Energy Physics 1 Windows on the Universe August 11-17 2013 Guy Nhon Vietnam Outline…
1 of 33 Twin Universes Cosmology Jean-Pierre Petit Marseille Observatory France Astrophysics and Space Science 226 273-307 1995 Abstract Starting from the field equation…
Continuing the Legacy of NASA’s Great Observatories The Wide Field Infrared Survey Telescope Roman Space Telescope Spectroscopic Capabilities Field of View sq deg Wavelength…
RADIATIVE PROCESSES in HIGH ENERGY ASTROPHYSICS Juri Poutanen (Tuorla Observatory, University of Turku, Finland) Zelenogorsk, Russia 2014 1 1. Introduction 2. Kinetic…
Continuing the Legacy of NASA’s Great Observatories The Wide Field Infrared Survey Telescope WFIRST Spectroscopic Capabilities Field of View sq deg Wavelength µm Resolution…
The James Webb Space Telescope JWST is a 6.5-meter-aperture observatory optimized for infrared astronomy 0.6 - 28 μm. JWST is the first infrared space telescope to employ…
Solar Neutrino Results from Phase III of the Sudbury Neutrino Observatory Alan Poon Berkeley Lab Solar Neutrinos Bahcall et al Solar Neutrino Problem ~Y2K • Deficits were…
Thirteenth Synthesis Imaging Workshop 2012 May 29– June 5 Low-frequency Interferometry Lincoln Greenhill ➢ Key science drivers at low frequencies: - Dark Ages (spin decoupling)…
Draft version November 9, 2018 Preprint typeset using LATEX style emulateapj v. 12/16/11 TESS DISCOVERY OF A TRANSITING SUPER-EARTH IN THE π MENSAE SYSTEM Chelsea X. Huang1,2,…
Solar Neutrino Results from Phase III of the Sudbury Neutrino Observatory Alan Poon Berkeley Lab Solar Neutrinos Bahcall et al Solar Neutrino Problem ~Y2K • Deficits were…
Future of US-China Pulsar Work Scott Ransom National Radio Astronomy Observatory University of Virginia What are pulsar radio properties • Continuum point sources • Quite…
ΕΛΛΗΝΙΚΗ ∆ΗΜΟΚΡΑΤΙΑ Α .∆ Ι .Π . ΑΡΧΗ ∆ΙΑΣΦΑΛΙΣΗΣ ΠΟΙΟΤΗΤΑΣ ΑΝΩΤΑΤΗΣ ΕΚΠΑΙ∆ΕΥΣΗΣ HELLENIC REPUBLIC H…
Our place in the Universe The Universe is very very big Earth radius 6378 km Sun Earth radius of sun x 109 orbit of earth around sun x 214 orbit of Pluto x 39 Pluto Nearby…
1 Class 23 : Dark Matter Halos n This class l Dark matter halos the “skeleton” of a galaxy l Halo over-density factor ΔV l Applications of Virial Theorem…