Riunione Avanzamento 1 ASI – Roma 11 Novembre 2008 INAF IFSI IRA OAFI OACT UNIRM1 UNIRM2 UNILE 1 SWG3: Evolution of Young Stellar Objects Goals Establish.
D EBRIS DISKS WITH H ERSCHEL : AN OVERVIEW OF THE DUNES MODELING ACTIVITIES Jean-Charles Augereau, Steve Ertel, Alexander Krivov, Jérémy Lebreton, Torsten.
ExoZodiacal Emission and Challenge and Opportunity for The Detection of ExoPlanets C. Beichman Friday, March 26, 2010 5 AU Workshop With lots of help from.
Cold dust in the Galactic halo: first detection of dust emission in a high-velocity cloud : Francois Boulanger et Marc-Antoine Miville-Deschênes Miville.
Emil-Christensen-SASP-2014
Visible Light and Beyond “White light” is made up of a rainbow of colors, each with a different wavelength.
SN 1987A the excitement continues Bruno Leibundgut ESO.
Basic Detection Techniques Front-end Detectors for the Submm Wolfgang Wild Lecture on 21 Sep 2006.
PENERAPAN PROSEDUR K3 DAN PENGAPLIKASIANNYA DI INDUSTRI PERHOTELAN Pertemuan 13 Matakuliah: V0152 / Hygiene, Keamanan & Keselamatan Tahun : 2008.
The SED of the nearby, HI-massive, LIRG HIZOA J0836-43: from the NIR to the radio domain Renée C. Kraan-Korteweg Astronomy Department Centre for Astrophysics.
Past, Present and Future Star Formation in High Redshift Radio Galaxies Nick Seymour (MSSL/UCL) 22 nd Nov 2009 - Powerful Radio Galaxies.
[email protected]. Last Version: DR3.5 Released June 2012 Pipeline: Optimised De- glitcher BriGAdE Allow Dark Pixel drift removal.