Bruce Partridge, Haverford College, USA ([email protected])[email protected] Outline: - CMB studiesEtudes CMB - Radio TechniquesTechniques de.
The Patent Chemistry “Big Bang” In Pubchem
Understand Galaxy Evolution with IR Surveys: Comparison between ISOCAM 15- m and Spitzer 24- m Source Counts as a Tool Carlotta Gruppioni – INAF OAB.
Science with SKA:. The SKA will provide continuous frequency coverage from 50 MHz to 14 GHz in the first two phases of its construction. A third phase.
Cumulative Deviation of data & model scaled to 0.3 99% 90% 95% HD 36861J (rp200200a01) 0.829 Probability of Variability A Large ROSAT Survey.
Introduction to the X-ray background Chandra Deep Field-North data Source Redshifts Diversity of X-ray selected sources Constraints on AGN evolution AGNs.
Star formation in Deep Radio Surveys
ASTRONOMY BROWN BAG SEMINAR SWIRE S pitzer W ide – area I nfra R ed E xtragalactic survey
Obscured AGN and XRB models
Bill Reach 2009 May 14 Greater IPAC Technology Symposium.
80x Bandwidth (8 GHz, full stokes), with 4000 channels Full frequency coverage (1 to 50 GHz)
Everything you wanted to know about the X-ray background …
