Astronomy and Astrophysics – Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Scientist
Space Science Department, Rutherford Appleton Laboratory, Chilton, Oxon OX11 0QX
ISO Science Operations Centre, Astrophysics Division of ESA, Villafranca, Spain; Queen Mary & Westfield College, University of London, London, UK
The LWS Instrument-Dedicated Team, ISO Science Operations Center, P.O. Box 50727, E-28080 Madrid, Spain
The LWS Instrument-Dedicated Team, ISO Science Operations Centre, PO Box 50727, E-28080 Madrid, Spain
Space Science & Technology Department, Science & Technology Facilities Council, Rutherford Appleton Laboratory, Chilton, Didcot, Oxon, OX11 0QX, UK
Rutherford Appleton Laboratory, Didcot, UK
ISO Science Operations Centre, Astrophysics Division of ESA, Villafranca, Spain
ISO Data Centre, Astrophysics Division, ESA, Villafranca, Spain
School of Physics, University College, Canberra ACT 2600, Australia
Rutherford Appleton Lab., Chilton, Didcot, Oxon OX11 0QX, UK
CSIC. Instituto de Estructura de la Materia. Serrano 121. 28006 Madrid. Spain
ISO-SOC
KAIST, Korea, Republic of
ISO Science Operations Centre, Astrophysics Division of ESA, P.O. Box 50727, E-28080 Madrid, Spain
Space Science and Technology Department, Rutherford Appleton Laboratory, Oxfordshire, OX11 0QX, UK
Space Science Department, Rutherford Appleton Lab., UK
RAL
ISO Science Operations Centre, Space Science Department of ESA, Villafranca, P.O. Box 50727, E-28080, Madrid, Spain
Rutherford Appleton Laboratory
CCLRC, Rutherford Appleton Lab., United Kingdom
"TNOs are Cool": A survey of the trans-Neptunian region I. Results from the Herschel Science Demonstration Phase (SDP)
"TNOs are Cool": A Survey of the Transneptunian Region IV. Size/albedo characterization of 15 scattered disk and detached objects observed with Herschel Space Observatory-PACS
An ISO Long Wavelength Spectrometer detection of CH in NGC 7027 and an HeH^+ upper limit
Aspects of LWS processing
Calibration and performance of the ISO Long-Wavelength Spectrometer.
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