Table of Contents
Michael R. Rosa
Agenda
Very Large Telescope 4 * 8m @ Cerro Paranal
HST
Historical Perspective
The Observational Information Loop
Travelling the Info Loop
Software Models of Instruments
Definitions & Examples
Demonstration of Requirements & Solutions
Classical Methods Dispersion Relations
Classical Methods Dispersion Relations
Classical Methods Dispersion Relations
FOS Dispersion Model Physical Principle
FOS Dispersion Model Solve for fcam and sgrating
FOS Dispersion Model Grating - Only
FOS Dispersion Model Grating only results
FOS Scattered Light
FOS - Solution to Scattered Light
Grating - Interference
Grating - Diffraction
IF * DF
Line Profile - IF *DF only
Line Profile - obs vs theory
Line Profile - obs vs theory (2)
Line Profile - obs vs theory (3)
Grating Scatter - Hot Target
Grating Scatter - Cool Target
FOS Scatter Model Test on Data
FOS Scatter Model Prediction for Blaze
Lesson from FOS Scattered Light
Reminder: Observation Information Loop
Generic Spectrograph Why - Multi-mode STIS
Generic Spectrograph Why - Multi-mode STIS
Generic Spectrograph Why - Multi-mode STIS
Generic Spectrograph Echelle Scatter
Generic Spectrograph STIS MAMA ghosts
Generic Spectrograph STIS Data Extraction
Generic Spectrograph First Principle Physics
Generic Spectrograph Optimizing Configurations
Generic Spectrograph Results CASPEC
Generic Spectrograph STIS Auto Wave-Cals
Generic Spectrograph Auto Wave-Cal E 140H
Generic Spectrograph STIS CCD Fringing
Generic Spectrograph Results CASPEC
Generic Spectrographs QED and Monte Carlo
We are almost there in the Observation Information
Loop
Closing the loop |