Slide 1 6. Really Basic Optics Sample Prep Instrument Out put Signal (Data) Select light Sample interaction source select Turn off/diminish intensity detect Polychromatic…

Introduction Most of what you have heard about so far has applied to a single spectral channel with some frequency width, dn Many astronomical problems require many channels…

Mid-IR selection of Ultra-Luminous Far-IR Galaxies Starburst and AGN tracers in z~2 ULIRGs continuum & CO mm emission, radio and PAH Alain Omont (IAP, CNRS and Université…

Hyper ULX Sean Farrell XMM-Newton Survey Science Centre University of Leicester, UK (soon to be University of Sydney, Australia) In collaboration with… D. Barret, S. Corbel,…

Astronomical Spectroscopy Astronomical Spectroscopy Astronomical spectroscopy is done by attaching a spectrometer to a telescope A spectrometer is a device separates the…

Large-Scale Galactic Stokes-I Continuum Science Chris Salter (NAIC/Arecibo Observatory) General Points: Arecibo can cover about 32% of the full sky. The 305-m telescope offers…

Science with continuum data ALMA continuum observations: Physical, chemical properties and evolution of dust, SFR, SED, circumstellar discs, accretion discs Effects of dust…

Paul M. Harveya George H. Riekeb Daniel F. Lestera Dominic J. Benfordc aUniversity of Texas bUniversity of Arizona cGoddard Space Flight Center SAFIR Single Aperture Far-Infrared…

Redshifted far-IR Lines and the Cornell Caltech Atacama Telescope: CCAT A joint project of Cornell University, the California Institute of Technology and the Jet Propulsion…

Lecture: April 8, 2003 Continuum Emission in AGN UV-Optical Continuum Infrared Continuum High Energy Continuum Radio Continuum - Jets and superluminal motion Goal: The foundation…