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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…
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,…
RESPONDING TO THE UNEMPLOYMENT CHALLENGE: A JOB GUARANTEE PROPOSAL FOR GREECE Observatory of Economic and Social Developments, Labour Institute, Greek General Confederation…
HIPPARCHOSHIPPARCHOS The Hellenic Astronomical Society Newsletter Volume 2, Issue 6 ISSN: 1790-9252 9o Ελληνικό Αστρονομικό Συνέδριο Αθήνα…
Extragalactic HydrogenExtragalactic Hydrogen Screenshot from first of 21,490 entries in the All Digital HI catalog in the Extragalactic Distance Database (https://edd.ifa.Hawaii.edu)