Video cameras and photometry Dave Herald. Background Occultations are usually step events When video introduced, it overcame issues of Personal Equation,
European Space Astronomy Centre (ESAC) Villafranca del Castillo, MADRID (SPAIN) Alberto Micol ISO & CharDM IVOA Cambridge, 2007-09-27 The Characterisation.
Star formation histories and environment Bianca M. Poggianti INAF – Osservatorio Astronomico di Padova WE ARE ALL AFTER THE BIG PICTURE: 1)To what extent,
Definitions for polarimetry Frans Snik Sterrewacht Leiden.
Light Visible electromagnetic radiation Power spectrum Polarization Photon (quantum effects) Wave (interference, diffraction) From London and Upton.
Hinode / EIS Solar 24, Dec 2008 Dr Peter Young, NRL/GMU Active Region Diagnostics with EIS Dr Peter Young Dr Peter Young Naval Research Laboratory George.
Photometry & Virtual Observatory Gijs Verdoes Kleijn Kapteyn Institute, room 147 [email protected] 050-3638326.
NGAO Report February 18, 2009 Waimea NGAO Report February 18, 2009 Waimea P. Wizinowich for the NGAO Team.
Photometry. Measuring Energy Photometry measures the energy from a source using a narrow range of wavelengths. –Visual wavelengths from 400-700 nm –Narrower.
30 March 2006Birmingham workshop1 The Gaia Mission A stereoscopic census of our Galaxy.
R Ophiuchi, A Mira- Type Variable Star Vikas Agtey Emily Berryman Caroline Fletcher Linda Gong Aaron McNeely Dan Walsh University of Notre Dame QuarkNet.
ALTAIR: Precision Photometric Calibration via Low-Cost Artificial Light Sources Above the Atmosphere Divya Bhatnagar Univ. of Victoria.
