Physics – Physics and Society
Scientist
Physics
Physics and Society
Scientist
ESA
ESA-VILSPA, Spain
and 32 others
ESA-VILSPA, Madrid, Spain
European Space Agency, Vilspa, Spain
University Coll., London
Technion - Israel Institute of Technology, Haifa
International Ultraviolet Explorer Observatory, Madrid, Spain
European Southern Observatory, La Silla, Chile
European Southern Observatory, Santiago, Chile
ESO
ESA IUE Obs.
IUE Observatory, Madrid, Spain
VILSPA
European Southern Observatory, Santiago, Chile; ESA, Villafranca Satellite Tracking Station, Madrid, Spain
ESA, Villafranca Satellite Tracking Station, Madrid, Spain
Ministerio de Educacion, Instituto Isaac Newton; European Southern Observatory, Santiago, Chile
ESA, Astronomy Div., Madrid, Spain
Texas Univ., Austin.
European Space Agency. ESA Tracking Station, Madrid, Spain
ESA IUE Observatory, PO Box 50727, 28080 Madrid, Spain
ESA-IUE Observatory, VILSPA, P.O. Box 50727, E-28080 Madrid, Spain
Wise Observatory, Tel Aviv, Israel
ESA-VILSPA, Apartado 50727, 28080 Madrid, Spain
NASA, Marshall Space Flight Center, Space Sciences Laboratory, Huntsville, Ala.
National Aeronautics and Space Administration. Goddard Space Flight Center, Greenbelt, MD.
SRC, Chilton, England
ESA-IUE Observatory, VILSPA, PO Box 50727, 28080 Madrid, Spain Villafranca del Castillo Satellite Tracking Station, Madrid, Spain
GSFC
ESA IUE Observatory, Villafranca, P.O. Box 50727, 28080 Madrid, Spain
European Southern Observatory, La Serena, Chile
Hamburger Sternwarte G.m.b.H., Germany
INTA / LAEFF, Apartado 50727, 28080 Madrid, Spain
International Center for Physics, Bogota, Columbia
ESA, European Space Research and Technology Centre, Noordwijk, Netherlands; FSA, Villafranca Satellite Tracking Station, Madrid, Spain
Science and Engineering Research Council, Madrid
ESA, Madrid
ESA IUE Observatory, Apartado 50727, 28080-Madrid, Spain and Affiliated to the Astrophysics Divisio
30 years of multi-wavelength observations of 3C 273
A comparison between various UV photometric systems for late-type stars
A Fast Monte Carlo Algorithm Applied the Photometry in the Central Portion of LMC Cluster NGC 121
A model for the variable continuum of the Seyfert 1 galaxy NGC 5548
A near-infrared study of the region L = 305 deg
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