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FOREBYGGELSESPAKKE Fysisk Aktivitet FOREBYGGELSESPAKKE – FYSISK AKTIVITET 3 INDholDsfortegNelse fakta 4 FOREKOMST 5 TABTE LEVEÅR SOM FØLGE AF FYSISK InAKTIVITET 6 BRuG…
An ultrahigh-speed digitizer for the Harvard College Observatory astronomical plates R.J. Simcoe ξ 1, J.E. Grindlay1, E.J. Los1, A.Doane1, S.G. Laycock1, D.J.Mink2, G. Champine1,…
The Characterising Exoplanets Satellite ExoPAG22 • 18 June 2020 David Ehrenreich the CHEOPS Mission Consortium 70-cm telescope Geneva Observatory January 2020 CH EO PS…
FanCam infrared parallax program is feasible •Resulting astrometric precision overall •x α: 1.3±0.7 µm 0.04”±0.02” •y δ: 1.3±0.8 µm 0.04”±0.02” •xy-averaged:…
The triple system AT Mic AB + AU Mic in the β Pictoris Association Sergio Messina1, Giuseppe Leto1, Isabella Pagano1 INAF- Catania Astrophysical Observatory, via S.Sofia,…
Simulation of the second half of the 20th Century using the MGO AGCM P.V. Sporyshev, V.P. Meleshko, T.V. Pavlova Voeikov Main Geophysical Observatory, St.Petersburg, Russia…
1 Planning for Transit in the World‟s Most Livable City: What Portland and the Rest of North America Can Learn From Vancouver Alan Jones – Director Steer Davies Gleave…
MNRAS 000 1– 2019 Preprint 7 November 2019 Compiled using MNRAS LATEX style file v30 H0LiCOW XIII A 24% measurement of H0 from lensed quasars: 53σ tension between early…
SD - Obscured AGN – June 8th 2007 OBSERVATIONS OF AGN WITH FUTURE VLT AND E-ELT INSTRUMENTS λλ 03-20 μm Sandro D’Odorico European Southern Observatory Paranal Observatory…
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…
Draft version April 22 2020 Typeset using LATEX twocolumn style in AASTeX63 The Origin and Evolution of Lyman-α Blobs in Cosmological Galaxy Formation Simulations Benjamin…
Draft version January 17, 2017 Preprint typeset using LATEX style AASTeX6 v. 1.0 AN ALTERNATIVE TO THE ΛCDM MODEL: THE CASE OF SCALE INVARIANCE Andre Maeder Geneva Observatory,…
AGN spectral lines SMBH Luka Č. Popović Astronomical Observatory, Belgrade, Serbia Bonn, June 24, 2010, MP0905 QSOs AGN emit radiation at a range of wavelengths from the…
ar X iv :a st ro -p h 04 05 58 7v 1 2 8 M ay 2 00 4 – 1 – Address for Correspondence: Nancy R. Evans Smithsonian Astrophysical Observatory MS 4, 60 Garden St., Cambridge,…
1 Super-Kamiokande Results Neutrino Oscillations Outline of the talk:Outline of the talk: • Brief introductionhistory • What we have learnt – Atmospheric neutrinos…
Slide 1Evolution of the comoving infrared energy density up to z~1 * Emeric Le Floch, Casey Papovich, Eiichi Egami, George Rieke & the MIPS team (Steward Observatory,…
A Deep Ocean Anti-Neutrino Observatory An Introduction to the Science Potential of Hanohano Presented by Steve Dye University of Hawaii at Manoa Hawaii Pacific University…
RESPONDING TO THE UNEMPLOYMENT CHALLENGE: A JOB GUARANTEE PROPOSAL FOR GREECE Observatory of Economic and Social Developments, Labour Institute, Greek General Confederation…
Lithium in the globular clusters ω Centauri & M4 Lorenzo Monaco ESO – European Southern Observatory / Santiago (Chile) [email protected] Collaborators: P. Bonifacio,…
Slide 1 Starbursts from z~3 to 7-10 Starbursts from z~3 to 7-10 Daniel Schaerer (Geneva Observatory, OMP Toulouse) Stellar populations: ages, star formation histories, masses,…