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<DIV ALIGN=CENTER>
<H1><A NAME="SECTION00090000000000000000">List of successful proposals</H1></DIV>
<HR><P>
The review of <I>ISO</I> Supplemental Call proposals has been completed.
The proposals (or parts thereof) with recommended observations are listed
below.
<HR><P>
<TABLE BORDER=3 CELLPADDING=2 CELLSPACING=3 WIDTH="100%">
<TR>
<TH WIDTH="20%">PI</TH><TH WIDTH="30%">Institute</TH><TH WIDTH="50%">Proposal</TH></TR>
<TR>
<TD>Abada-Simon M. </TD>
<TD>Observatoire de Paris-Meudon </TD>
<TD> Extension of AE Aquarii's radio spectrum to the far infrared -
search for the synchrotron spectrum's turnover frequency
<BR>
</TD></TR>
<TR>
<TD>Abergel A. </TD>
<TD>Institut d'Astrophysique Spatiale, Orsay </TD>
<TD> Extinction curve in dense cores
</TD></TR>
<TR>
<TD>Acosta-Pulido J. </TD>
<TD>ISO-SOC, ESA, Vilspa </TD>
<TD> Mid IR imaging of the starburst galaxy NGC 6090
</TD></TR>
<TR>
<TD>Andre P. </TD>
<TD>C.E.A. - Service d'Astrophysique </TD>
<TD> An ISOCAM absorption survey for dense clumps within dark clouds
</TD></TR>
<TR>
<TD>Andre P. </TD>
<TD>C.E.A. - Service d'Astrophysique </TD>
<TD> The spatial structure of protostellar cores - an absorption study
</TD></TR>
<TR>
<TD>Andreani P. </TD>
<TD>Dipartimento di Astronomia, Universita` di Padova </TD>
<TD> Photometry of cluster candidates for the Sunyaev-Zeldovich effect
</TD></TR>
<TR>
<TD>Andreani P. </TD>
<TD>Dipartimento di Astronomia, Universita` di Padova </TD>
<TD> FIR photometry of a complete sample of optically selected bright quasars.
</TD></TR>
<TR>
<TD>Backman D. </TD>
<TD>Franklin and Marshall College, Lancaster, PA </TD>
<TD> Terrestrial-temperature Dust around Cluster `A' Stars
</TD></TR>
<TR>
<TD>Backman D. </TD>
<TD>Franklin and Marshall College, Lancaster, PA </TD>
<TD> Zodiacal Dust in Other Planetary Systems - Search for Hot Dust Around
Planetary-Perturbation Target Stars
<BR>
</TD></TR>
<TR>
<TD>Backman D. </TD>
<TD>Franklin and Marshall College, Lancaster, PA </TD>
<TD> Mapping and Spectroscopy of a Circumbinary Disk -
IR Studies of an Edge-On Disk Discovered via Coronagraphy
<BR>
</TD></TR>
<TR>
<TD>Baluteau J. </TD>
<TD>Laboratoire d'Astronomie Spatiale </TD>
<TD> Complete LWS Spectral Survey at High Resolution
</TD></TR>
<TR>
<TD>Bania T. </TD>
<TD>Department of Astronomy, Boston University </TD>
<TD> Probing the properties of Southern hemisphere galactic HII/PDR/GMC
sources using ISO FIR spectra and ASTRO [CI] measurements
<BR>
</TD></TR>
<TR>
<TD>Bania T. </TD>
<TD>Department of Astronomy, Boston University </TD>
<TD> Southern hemisphere high latitude clouds: constraining the chemistry of
translucent gas
</TD></TR>
<TR>
<TD>Barlow M. </TD>
<TD>University College London </TD>
<TD> FP observations of FAR-IR OH maser pump lines
</TD></TR>
<TR>
<TD>Barlow M. </TD>
<TD>University College London </TD>
<TD> High resolution observations of FAR-IR water lines
</TD></TR>
<TR>
<TD>Barr P. </TD>
<TD>ISO-SOC, ESA, Vilspa </TD>
<TD> Infrared properties of Cygnus X-3; origin of the IR flares and quiescent
emission
</TD></TR>
<TR>
<TD>Barr P. </TD>
<TD>ISO-SOC, ESA, Vilspa </TD>
<TD> Multifrequency monitoring of the enigmatic blazar 3C279
</TD></TR>
<TR>
<TD>Barucci A. </TD>
<TD>Observatoire de Paris-Meudon </TD>
<TD> Dark, volatile rich asteroids : possible relation to comets
</TD></TR>
<TR>
<TD>Barvainis R. </TD>
<TD>MIT Haystack Observatory </TD>
<TD> High Redshift Primeval Galaxies Lensed by Clusters
</TD></TR>
<TR>
<TD>Baudry A. </TD>
<TD>Observatoire de Bordeaux </TD>
<TD> Detection of OD in selected hot molecular cores
</TD></TR>
<TR>
<TD>Baudry A. </TD>
<TD>Observatoire de Bordeaux </TD>
<TD> OH in Compact HII Regions
</TD></TR>
<TR>
<TD>Bechtold J. </TD>
<TD>Steward Observatory </TD>
<TD> The Spectral Energy Distribution of the Protogalaxy Candidate MS1512-cB58
</TD></TR>
<TR>
<TD>Beckwith S. </TD>
<TD>MPI f. Astronomie, Heidelberg </TD>
<TD> Evolution of Circumstellar Disks - A Test of Disk-Regulated Angular Momentum
Evolution
</TD></TR>
<TR>
<TD>Beckwith S. </TD>
<TD>MPI f. Astronomie, Heidelberg </TD>
<TD> Physical Properties of Circumstellar Disks - Spectral Energy Distributions
of Young Stellar Objects
</TD></TR>
<TR>
<TD>Bernard J. </TD>
<TD>Institut d'Astrophysique Spatiale, Orsay </TD>
<TD> Origin of color variations in the ISM
</TD></TR>
<TR>
<TD>Bertoldi F. </TD>
<TD>Max-Planck-Institut f. Extraterrestrische Physik </TD>
<TD> Physical Conditions in Photodissociation Regions
</TD></TR>
<TR>
<TD>Bezard B. </TD>
<TD>Observatoire de Paris, Section de Meudon </TD>
<TD> Search for methyl radical on Neptune and Saturn
</TD></TR>
<TR>
<TD>Bezard B. </TD>
<TD>Observatoire de Paris, Section de Meudon </TD>
<TD> Search for undetected photochemical compounds on Jupiter
</TD></TR>
<TR>
<TD>Bezard B. </TD>
<TD>Observatoire de Paris, Section de Meudon </TD>
<TD> The atmospheric structure of brown dwarf Gliese 229 B
</TD></TR>
<TR>
<TD>Birkinshaw M. </TD>
<TD>Department of Physics, University of Bristol </TD>
<TD> IR properties of the cores of nearby radio galaxies
</TD></TR>
<TR>
<TD>Biviano A. </TD>
<TD>ISO-SOC, ESA, Vilspa </TD>
<TD> Early-type post-starburst galaxies in the Coma cluster
</TD></TR>
<TR>
<TD>Biviano A. </TD>
<TD>ISO-SOC, ESA, Vilspa </TD>
<TD> The Infra-Red Properties of Brightest Cluster Members
</TD></TR>
<TR>
<TD>Blake G. </TD>
<TD>California Instititute of Technology </TD>
<TD> SWS Studies of H <IMG WIDTH=5 HEIGHT=10 ALIGN=MIDDLE ALT="tex2html_wrap_inline136" SRC="imgx.gif" > Rotational Lines from YSO Accretion Disks
</TD></TR>
<TR>
<TD>Blommaert J. </TD>
<TD>ISO-SOC, ESA, Vilspa </TD>
<TD> Evolution and mass loss of AGB stars in the Small Magellanic Cloud
</TD></TR>
<TR>
<TD>Boulanger F. </TD>
<TD>Institut d'Astrophysique Spatiale, Orsay </TD>
<TD> Very Small Dust grains in the Galactic halo - Dust destruction in shocks
</TD></TR>
<TR>
<TD>Braine J. </TD>
<TD>Observatoire de Bordeaux </TD>
<TD> Gas Properties in an old but incomplete merger : NGC 660
A study of gas properties in a polar ring galaxy
<BR>
</TD></TR>
<TR>
<TD>Bregman J. </TD>
<TD>NASA-AMES Research Center </TD>
<TD> Are there hidden supernovae?
</TD></TR>
<TR>
<TD>Bregman J. </TD>
<TD>University of Michigan </TD>
<TD> The Origin of Dust and PAHs in Elliptical Galaxies
</TD></TR>
<TR>
<TD>Bujarrabal V. </TD>
<TD>Observatorio Astronomico Nacional, Alcala de Henares </TD>
<TD> Atomic gas in protoplanetary nebulae, II
</TD></TR>
<TR>
<TD>Carr J. </TD>
<TD>Naval Research Lab </TD>
<TD> Water in Protoplanetary Disks
</TD></TR>
<TR>
<TD>Casali M. </TD>
<TD>Royal Observatory, Edinburgh </TD>
<TD> A search for cool halo emission above NGC5714 and NGC5529
</TD></TR>
<TR>
<TD>Casoli F. </TD>
<TD>Observatoire de Paris </TD>
<TD> Fine-structure line emission in selected regions of M 31
</TD></TR>
<TR>
<TD>Casoli F. </TD>
<TD>Observatoire de Paris </TD>
<TD> CII line emission in isolated galaxies
</TD></TR>
<TR>
<TD>Cassinelli J. </TD>
<TD>University of Wisconsin-Madison </TD>
<TD> IR Diagnostics of Temperature Structure in the - Atmospheres of Early B
Stars
</TD></TR>
<TR>
<TD>Cassinelli J. </TD>
<TD>University of Wisconsin-Madison </TD>
<TD> The Velocity Structure of Wolf-Rayet Winds - from Infrared Line and Continuum
Observations
</TD></TR>
<TR>
<TD>Caux E. </TD>
<TD>Centre d'Etudes Spatiales des Rayonnements </TD>
<TD> Atomic oxygen absorption against bright galactic sources
</TD></TR>
<TR>
<TD>Ceccarelli C. </TD>
<TD>Observatoire de Grenoble </TD>
<TD> Map of C and J type shocks in IRAS16293-2422
</TD></TR>
<TR>
<TD>Cernicharo J. </TD>
<TD>Instituto de Estructura de la Materia. CSIC, Madrid </TD>
<TD> A key spectroscopic study of CRL618 - shocked chemistry in Post-AGB evolution
</TD></TR>
<TR>
<TD>Cernicharo J. </TD>
<TD>Instituto de Estructura de la Materia. CSIC, Madrid </TD>
<TD> A search for C <SUB>3</SUB> , C <SUB>4</SUB> H <IMG WIDTH=5 HEIGHT=10 ALIGN=MIDDLE ALT="tex2html_wrap_inline136" SRC="imgx.gif" > , and C <SUB>6</SUB> H <IMG WIDTH=5 HEIGHT=10 ALIGN=MIDDLE ALT="tex2html_wrap_inline136" SRC="imgx.gif" > in the interstellar medium -
the synthesis of hydrocarbons in the ISM and in the CSM
<BR>
</TD></TR>
<TR>
<TD>Cernicharo J. </TD>
<TD>Instituto de Estructura de la Materia. CSIC, Madrid </TD>
<TD> A study of dust, atomic and molecular emission in cometary globules -
the physics of partially ionized globules in the Trifid
<BR>
</TD></TR>
<TR>
<TD>Cernicharo J. </TD>
<TD>Instituto de Estructura de la Materia. CSIC, Madrid </TD>
<TD> A study of water emission in molecular clouds -
The extent of water vapor emission in galactic molecular clouds
<BR>
</TD></TR>
<TR>
<TD>Cernicharo J. </TD>
<TD>Instituto de Estructura de la Materia. CSIC, Madrid </TD>
<TD> HH Jets and their interaction with their placentary clouds
</TD></TR>
<TR>
<TD>Cernicharo J. </TD>
<TD>Instituto de Estructura de la Materia. CSIC, Madrid </TD>
<TD> The Mid and Far infrared spectrum of keystone molecular clouds -
the molecular content of warm and cold molecular clouds
<BR>
</TD></TR>
<TR>
<TD>Cesarsky C. </TD>
<TD>Service d'Astrophysique. CEA-SACLAY </TD>
<TD> Ultra-deep survey with ISOCAM - search for primeval galaxies and quasars
</TD></TR>
<TR>
<TD>Cesarsky D. </TD>
<TD>Institut d'Astrophysique Spatiale, Orsay </TD>
<TD> Dust emission in reflection nebulae
</TD></TR>
<TR>
<TD>Chini R. </TD>
<TD>Max Planck Institut f. Radioastronomie, Bonn </TD>
<TD> ISO study of protostars
</TD></TR>
<TR>
<TD>Clavel J. </TD>
<TD>ISO-SOC, ESA, Vilspa </TD>
<TD> ISO and mm observations of narrow lines Seyfert 1 galaxies
</TD></TR>
<TR>
<TD>Colangeli L. </TD>
<TD>Osservatorio Astronomico di Capodimonte, Napoli </TD>
<TD> Extended Remote Analysis of Coma and Trails - Analysis of comets also in
preparation to Rosetta
</TD></TR>
<TR>
<TD>Colgan S. </TD>
<TD>SETI Institute/NASA-AMES Research Center </TD>
<TD> Infrared Spectroscopy of Black Hole Candidates
</TD></TR>
<TR>
<TD>Colgan S. </TD>
<TD>SETI Institute/NASA-AMES Research Center </TD>
<TD> The Properties of Narrow Recombination Line HII Regions
</TD></TR>
<TR>
<TD>Combes F. </TD>
<TD>DEMIRM Observatoire de Paris </TD>
<TD> Bars and Tides in Galaxies - Role of Large-scale Dynamics on Star Formation
</TD></TR>
<TR>
<TD>Combes F. </TD>
<TD>DEMIRM Observatoire de Paris </TD>
<TD> Spiral Arm in Messier 31 - Star-formation Processes Across the Arm
</TD></TR>
<TR>
<TD>Comeron F. </TD>
<TD>European Southern Observatory </TD>
<TD> Brown dwarf candidates in the Rho Ophiuchi cluster
</TD></TR>
<TR>
<TD>Comeron F. </TD>
<TD>European Southern Observatory </TD>
<TD> Ultracompact HII regions in the Large Magellanic Cloud
</TD></TR>
<TR>
<TD>Courvoisier T. </TD>
<TD>Integral Science Data Center, Versoix </TD>
<TD> Far-infrared variability of a large sample of quasars
</TD></TR>
<TR>
<TD>Coustenis A. </TD>
<TD>DESPA, Observatoire de Paris </TD>
<TD> Spectroscopy of the 12.2 and 13.4 micron regions on Titan
</TD></TR>
<TR>
<TD>Coustenis A. </TD>
<TD>DESPA, Observatoire de Paris </TD>
<TD> The 3-micron window on Titan
</TD></TR>
<TR>
<TD>Coustenis A. </TD>
<TD>DESPA, Observatoire de Paris </TD>
<TD> The short-wavelength spectrum of Titan
</TD></TR>
<TR>
<TD>Cox C. </TD>
<TD>University of Virginia </TD>
<TD> The distribution and temperature of dust in ABELL 1691
</TD></TR>
<TR>
<TD>Cox P. </TD>
<TD>Institut d'Astrophysique Spatiale, Orsay </TD>
<TD> A study of water vapour absorption in molecular clouds
</TD></TR>
<TR>
<TD>Cox P. </TD>
<TD>Institut d'Astrophysique Spatiale, Orsay </TD>
<TD> The Helix nebula : a case study of a PDR region
</TD></TR>
<TR>
<TD>Crovisier J. </TD>
<TD>Observatoire de Paris-Meudon </TD>
<TD> ToO spectroscopic observations of comets
</TD></TR>
<TR>
<TD>d'Hendecourt L. </TD>
<TD>Institut d'Astrophysique Spatiale, Orsay </TD>
<TD> Spectroscopy of carbon bearing molecules in diffuse ISM
</TD></TR>
<TR>
<TD>d'Hendecourt L. </TD>
<TD>Institut d'Astrophysique Spatiale, Orsay </TD>
<TD> Survey of Solid State Molecular Absorption
</TD></TR>
<TR>
<TD>d'Hendecourt L. </TD>
<TD>Institut d'Astrophysique Spatiale, Orsay </TD>
<TD> Specific search for solid state and gas phase features.
</TD></TR>
<TR>
<TD>Davis G. </TD>
<TD>University of Saskatchewan </TD>
<TD> ISO Spectroscopy of the Martian Atmosphere
</TD></TR>
<TR>
<TD>de Jong T. </TD>
<TD>SRON, Groningen </TD>
<TD> High resolution Observations of HCN and C <IMG WIDTH=5 HEIGHT=10 ALIGN=MIDDLE ALT="tex2html_wrap_inline136" SRC="imgx.gif" > H <IMG WIDTH=5 HEIGHT=10 ALIGN=MIDDLE ALT="tex2html_wrap_inline136" SRC="imgx.gif" > lines in Carbon Stars
</TD></TR>
<TR>
<TD>de Jong T. </TD>
<TD>SRON, Groningen </TD>
<TD> SWS Observations of O-Rich Circumstellar Shell of Late-type Stars with the
13 <IMG WIDTH=10 HEIGHT=12 ALIGN=MIDDLE ALT="tex2html_wrap_inline152" SRC="img5.gif" > m Emission Feature
</TD></TR>
<TR>
<TD>De Zotti G. </TD>
<TD>Osservatorio Astronomico, Padova </TD>
<TD> Far-IR evolution of galaxies : the IRAS deep survey sample
</TD></TR>
<TR>
<TD>Deleuil M. </TD>
<TD>Laboratoire d'Astronomie Spatiale - CNRS </TD>
<TD> Origin of the circumstellar disc around Beta Pictoris
</TD></TR>
<TR>
<TD>Dermott S. </TD>
<TD>University of Florida </TD>
<TD> Probing The Zodiacal Cloud by Observing the Ecliptic Poles
</TD></TR>
<TR>
<TD>Drossart P. </TD>
<TD>DESPA, Observatoire de Meudon </TD>
<TD> Equatorial emissions of hydrocarbons on Jupiter
</TD></TR>
<TR>
<TD>Dunlop J. </TD>
<TD>IFA, University of Edinburgh </TD>
<TD> An infrared comparison of the host galaxies of radio-quiet quasars,
radio-loud quasars and radio galaxies.
</TD></TR>
<TR>
<TD>Dunlop J. </TD>
<TD>IFA, University of Edinburgh </TD>
<TD> The formation and evolution of elliptical galaxies
</TD></TR>
<TR>
<TD>Dwek E. </TD>
<TD>NASA/GSFC </TD>
<TD> A Search for the Infrared Signature of Graphite Grains -
The 11.52 micron Graphitic Absorption Feature Towards the G.C.
<BR>
</TD></TR>
<TR>
<TD>Efstathiou A. </TD>
<TD>Blackett Laboratory, Imperial College </TD>
<TD> Photometry and spectroscopy of AGN with polarized BLR
</TD></TR>
<TR>
<TD>Egami E. </TD>
<TD>Max-Planck-Institut f. Extraterrestrische Physik, Garching </TD>
<TD> SWS Spectroscopy of Molecular Hydrogen Lines in Bright IR Galaxies
</TD></TR>
<TR>
<TD>Egami E. </TD>
<TD>Max-Planck-Institut f. Extraterrestrische Physik, Garching </TD>
<TD> SWS Spectroscopy of a Seyfert2 Warm Ultraluminous Galaxy IRAS 05189-2524
</TD></TR>
<TR>
<TD>Ehrenfreund P. </TD>
<TD>Leiden Observatory </TD>
<TD> Search for interstellar fullerenes
</TD></TR>
<TR>
<TD>Ehrenfreund P. </TD>
<TD>Leiden Observatory </TD>
<TD> Search for solid molecular oxygen and ozone
</TD></TR>
<TR>
<TD>Eisloeffel J. </TD>
<TD>Thueringer Landessternwarte Tautenburg </TD>
<TD> The dusty envelopes of deeply emdedded Class 0 outflow sources
</TD></TR>
<TR>
<TD>Encrenaz T. </TD>
<TD>DESPA, Observatoire de Paris </TD>
<TD> Jupiter: latitudinal variations of atmospheric parameters
</TD></TR>
<TR>
<TD>Engels D. </TD>
<TD>Hamburger Sternwarte </TD>
<TD> The 22 GHz H <IMG WIDTH=5 HEIGHT=10 ALIGN=MIDDLE ALT="tex2html_wrap_inline136" SRC="imgx.gif" > O maser pump in AGB stars
</TD></TR>
<TR>
<TD>Eriksson K. </TD>
<TD>Uppsala Astronomical Observatory </TD>
<TD> Spectra of envelopes around AGB stars
</TD></TR>
<TR>
<TD>Evans N. </TD>
<TD>Astronomy Department, The Univ. of Texas at Austin </TD>
<TD> Photoionization regulated star formation, cloud structure, and tracers of
the neutral ISM
</TD></TR>
<TR>
<TD>Eyres S. </TD>
<TD>Keele University </TD>
<TD> SWS spectroscopy of symbiotic stars
</TD></TR>
<TR>
<TD>Eyres S. </TD>
<TD>Keele University </TD>
<TD> Spectroscopy of Sakurai's object in Sagittarius - the evolution of a final
helium shell flash
</TD></TR>
<TR>
<TD>Fajardo-Acosta S. </TD>
<TD>University of Denver </TD>
<TD> Microscan Mapping of Vega-type Circumstellar Dust
</TD></TR>
<TR>
<TD>Falgarone E. </TD>
<TD>Ecole Normale Superieure </TD>
<TD> Gas spectral diagnostics of the dust emission color - variations in
interstellar clouds
</TD></TR>
<TR>
<TD>Falgarone E. </TD>
<TD>Ecole Normale Superieure </TD>
<TD> Polarization of dust absorption at the edge of a dense core - magnetic field
confinement?
</TD></TR>
<TR>
<TD>Fanti C. </TD>
<TD>Institute of Radioastronomy, Bologna </TD>
<TD> Medium-Far Infrared observations of Compact Steep-spectrum and GHz Peaked
Spectrum radio galaxies
</TD></TR>
<TR>
<TD>Feretti L. </TD>
<TD>Istituto di Radioastronomia, Bologna </TD>
<TD> Elliptical galaxies in rich clusters : dust and stripping
</TD></TR>
<TR>
<TD>Fischer J. </TD>
<TD>Naval Research Laboratory </TD>
<TD> LWS Grating Observations of HD and other molecules in IR Bright Galaxies
</TD></TR>
<TR>
<TD>Franceschini A. </TD>
<TD>Dipartimento di Astronomia, Universita` di Padova </TD>
<TD> ISO observations of candidate primeval dusty galaxies and AGNs - IR
photometry of high redshift galaxies
</TD></TR>
<TR>
<TD>Fuente A. </TD>
<TD>Observatorio Astronomico Nacional, Alcala de Henares </TD>
<TD> A chemical study of the hot and dense molecular gas adjacent to the
photon-dominated region (PDR) associated with NGC 7023
<BR>
</TD></TR>
<TR>
<TD>Fulchignoni M. </TD>
<TD>Observatoire de Paris-Meudon </TD>
<TD> Rosetta target asteroids
</TD></TR>
<TR>
<TD>Fusi Pecci F. </TD>
<TD>Osservatorio Astronomico, Bologna </TD>
<TD> Circumstellar matter in the central region of globular clusters.
</TD></TR>
<TR>
<TD>Garnett D. </TD>
<TD>Astronomy Department, University of Minnesota </TD>
<TD> Composition and Cooling in Extragalactic H II Regions
</TD></TR>
<TR>
<TD>Garzon F. </TD>
<TD>Instituto de Astrofisica de Canarias </TD>
<TD> The Physical Parameters that Control Violent Stellar Bursts
</TD></TR>
<TR>
<TD>Gehrz R. </TD>
<TD>University of Minnesota </TD>
<TD> ToO: ISO spectroscopy of Galactic Novae
</TD></TR>
<TR>
<TD>Gerin M. </TD>
<TD>Dept. Radioastronomie, Ecole Normale Superieure </TD>
<TD> The dust composition in distant galaxies
</TD></TR>
<TR>
<TD>Giard M. </TD>
<TD>CESR/CNRS, Toulouse </TD>
<TD> IR emission of SZ galaxy clusters
</TD></TR>
<TR>
<TD>Giard M. </TD>
<TD>CESR/CNRS, Toulouse </TD>
<TD> Water vapor in warm dusty regions
</TD></TR>
<TR>
<TD>Gilmore G. </TD>
<TD>Institute of Astronomy, Cambridge </TD>
<TD> ISO colours of the halos of normal galaxies
</TD></TR>
<TR>
<TD>Goldschmidt P. </TD>
<TD>Blackett Laboratory, Imperial College </TD>
<TD> The physical causes of quasar evolution
</TD></TR>
<TR>
<TD>Goldschmidt P. </TD>
<TD>Blackett Laboratory, Imperial College </TD>
<TD> Photometry of PG quasars
</TD></TR>
<TR>
<TD>Griffin M. </TD>
<TD>Physics Department, Queen Mary and Westfield College </TD>
<TD> The Far infrared continuum spectra of cold protostellar sources
</TD></TR>
<TR>
<TD>Gruen E. </TD>
<TD>Max-Planck-Institut f. Kernphysik, Heidelberg </TD>
<TD> ToO: ISOPHOT observations of a new comet
</TD></TR>
<TR>
<TD>Guertler J. </TD>
<TD>Universitaets-Sternwarte Jena </TD>
<TD> IR imaging of post-AGB dust envelopes
</TD></TR>
<TR>
<TD>Guertler J. </TD>
<TD>Universitaets-Sternwarte Jena </TD>
<TD> Infrared ice bands towards young stars in Chamaeleon
</TD></TR>
<TR>
<TD>Haas M. </TD>
<TD>Max-Planck-Institut f. Astronomie, Heidelberg </TD>
<TD> Far Infrared Map of the Andromeda Galaxy M31
</TD></TR>
<TR>
<TD>Haas M. </TD>
<TD>Max-Planck-Institut f. Astronomie, Heidelberg </TD>
<TD> Search for cold dust in the normal spiral galaxy M31
</TD></TR>
<TR>
<TD>Haas M. </TD>
<TD>NASA-Ames Research Center </TD>
<TD> A Study of Interstellar Shocks in IC443
</TD></TR>
<TR>
<TD>Haas M. </TD>
<TD>NASA-Ames Research Center </TD>
<TD> Physical Conditions in the Circumstellar Envelopes of Supergiants and
Other Evolved Stars
</TD></TR>
<TR>
<TD>Hammer F. </TD>
<TD>DAEC, Observatoire de Paris-Meudon </TD>
<TD> Infrared studies of distant galaxies in deep optical surveys.
Nature of field galaxies from HST, ISO and deep spectroscopy.
<BR>
</TD></TR>
<TR>
<TD>Helmich F. </TD>
<TD>Sterrewacht Leiden </TD>
<TD> A search for the methyl radical
</TD></TR>
<TR>
<TD>Helou G. </TD>
<TD>IPAC </TD>
<TD> A [OI] survey in high redshift objects
</TD></TR>
<TR>
<TD>Henning T. </TD>
<TD>MPG, Jena </TD>
<TD> Search for the 21 micron emitters
</TD></TR>
<TR>
<TD>Hensler G. </TD>
<TD>Institute of Astronomy and Astrophysics, Kiel </TD>
<TD> Infrared spectroscopy of starburst dwarf galaxies NGC 4449
</TD></TR>
<TR>
<TD>Herbstmeier U. </TD>
<TD>Max-Planck-Institut f. Astronomie, Heidelberg </TD>
<TD> Cirrus Dust Clouds in Hot Plasma G88+36-2
</TD></TR>
<TR>
<TD>Hoare M. </TD>
<TD>Dept. of Physics & Astronomy, University of Leeds </TD>
<TD> Ionized winds from luminous young stellar objects.
</TD></TR>
<TR>
<TD>Hough J. </TD>
<TD>University of Hertfordshire </TD>
<TD> Polarimetry of the nucleus of active galaxies
AGN with hidden broadlines and rising IR polarization
</TD></TR>
<TR>
<TD>Hrivnak B. </TD>
<TD>Valparaiso University </TD>
<TD> Spectroscopy of Additional Visible Proto-Planetary Nebulae
</TD></TR>
<TR>
<TD>Hron J. </TD>
<TD>Institut f. Astronomie, Universitaet Wien </TD>
<TD> Spectral Variability of Long Period Variables - The Relation between
Pulsation, Atmospheric Structure and Dust Formation
<BR>
</TD></TR>
<TR>
<TD>Hurley K. </TD>
<TD>University of California </TD>
<TD> Study of Soft Gamma Repeater Counterparts
</TD></TR>
<TR>
<TD>Ip W. </TD>
<TD>Max-Planck-Institut f. Aeronomie, Katlenburg-Lindau </TD>
<TD> A Survey of Kuiper Belt Candidates
</TD></TR>
<TR>
<TD>Ishii K. </TD>
<TD>Remote Sensing Technology Center of Japan, Tokyo </TD>
<TD> [C II] observations of spiral structures in NGC 300 -
a research on arm-interarm contrast in star-formation efficiency
<BR>
</TD></TR>
<TR>
<TD>Ivison R. </TD>
<TD>Royal Observatory, Edinburgh </TD>
<TD> The far-IR luminosity function of QSOs in the early Universe
</TD></TR>
<TR>
<TD>Izumiura H. </TD>
<TD>Okayama Astrophysical Observatory </TD>
<TD> Extended Dust Shell around the J-type Carbon Star RY Draconis
</TD></TR>
<TR>
<TD>Jackson J. </TD>
<TD>Boston University </TD>
<TD> Infrared Studies of Massive Young Stars and the ISM - The NGC 6334 Star
Formation Region
</TD></TR>
<TR>
<TD>Jackson J. </TD>
<TD>Boston University </TD>
<TD> Low Metallicity PDR Diagnostics in the Infrared - a Study of the Dust-Gas
Interaction
</TD></TR>
<TR>
<TD>Joblin C. </TD>
<TD>Centre d'Etudes Spatiale des Rayonnements </TD>
<TD> IR emission features and interstellar PAH'S - the simple case of the
reflection nebula NGC 1333-SVS3
</TD></TR>
<TR>
<TD>Joseph R. </TD>
<TD>Institute for Astronomy, Honolulu </TD>
<TD> The ISOPHOT Field Galaxy Survey
</TD></TR>
<TR>
<TD>Jourdain de Muizon M. </TD>
<TD>LAEFF - INTA, Madrid </TD>
<TD> Variation of the dust composition through the Taurus cloud -
Infrared spectra of background stars toward the Taurus cloud
<BR>
</TD></TR>
<TR>
<TD>Justtanont K. </TD>
<TD>SRON, Groningen </TD>
<TD> SWS Observation of molecular lines in NML Cyg
</TD></TR>
<TR>
<TD>Kawara K. </TD>
<TD>ISO-SOC, ESA, Vilspa / ISAS </TD>
<TD> ISO Study of Evolution of Quasar Spectra
- Spectral Evolution Separated from Luminosity Effect
</TD></TR>
<TR>
<TD>Keel W. </TD>
<TD>University of Alabama </TD>
<TD> Stellar populations in a cluster of galaxies at z=2.4
</TD></TR>
<TR>
<TD>Kegel W. </TD>
<TD>Inst. f. Theor. Physik, Universitaet Frankfurt/Main </TD>
<TD> OH-megamasers and the velocity field.
</TD></TR>
<TR>
<TD>Kerber F. </TD>
<TD>Institut f. Astronomie, Innsbruck </TD>
<TD> Sakurai's Object : A New Born-Again Nucleus of a Planetary Nebula
</TD></TR>
<TR>
<TD>Kerschbaum F. </TD>
<TD>Institut f. Astronomie, Universitaet Wien </TD>
<TD> Atmospheric structure of o-rich semiregular and irregular
</TD></TR>
<TR>
<TD>Kidger M. </TD>
<TD>Instituto de Astrofisica de Canarias </TD>
<TD> The optical-radio polarisation breakpoint in blazars
</TD></TR>
<TR>
<TD>Knapp G. </TD>
<TD>Princeton University Observatory </TD>
<TD> Origin and Evolution of Dust in Elliptical Galaxies - ISOPHOT
Observations of 10 Galaxies with Nuclear Optical Dust Lanes
<BR>
</TD></TR>
<TR>
<TD>Krugel E. </TD>
<TD>MPI f. Radioastronomie, Bonn </TD>
<TD> Dust emission from radio galaxies at high redshifts
</TD></TR>
<TR>
<TD>Kunze D. </TD>
<TD>Max-Planck-Institut f. Extraterrestrische Physik, Garching </TD>
<TD> Detailed Spectroscopy of the Galactic Center
</TD></TR>
<TR>
<TD>Kwok S. </TD>
<TD>University of Calgary </TD>
<TD> A Detailed Study of the Unidentified 21 micron Emission Feature In Post-AGB
Stars
</TD></TR>
<TR>
<TD>Kwok S. </TD>
<TD>University of Calgary </TD>
<TD> Spectroscopy of Extreme Carbon Stars
</TD></TR>
<TR>
<TD>Lambert D. </TD>
<TD>Univ. of Texas at Austin </TD>
<TD> Testing model atmospheres of cool Dwarf stars with ISO
</TD></TR>
<TR>
<TD>Lamers H. </TD>
<TD>SRON Laboratory for Space Research Utrecht </TD>
<TD> The winds of early type supergiants -
The critical mass loss phase of massive stars.
</TD></TR>
<TR>
<TD>Lamy P. </TD>
<TD>Laboratoire d'Astronomie Spatiale </TD>
<TD> Observation of cometary nuclei
</TD></TR>
<TR>
<TD>Lamy P. </TD>
<TD>Laboratoire d'Astronomie Spatiale </TD>
<TD> ToO: The nucleus of a new bright comet
</TD></TR>
<TR>
<TD>Launhardt R. </TD>
<TD>MPG, Research Unit: Dust in Star-Forming Regions, Jena </TD>
<TD> MIR morphology of a high-mass protostellar core
The case of LBN594-MM
</TD></TR>
<TR>
<TD>Laureijs R. </TD>
<TD>ISO-SOC, ESA, Vilspa </TD>
<TD> Small scale structure and dust properties in cloud cores
</TD></TR>
<TR>
<TD>Lebertre T. </TD>
<TD>Observatoire de Paris </TD>
<TD> Interstellar dust heated by AGB stars
</TD></TR>
<TR>
<TD>Leech K. </TD>
<TD>ISO-SOC, ESA, Vilspa </TD>
<TD> ISO observations of the Pleiades Brown Dwarfs
Teide 1 and Calar 3
</TD></TR>
<TR>
<TD>Leger A. </TD>
<TD>Institut d'Astrophysique Spatiale, Orsay </TD>
<TD> Search for C 60+ bands and long-wavelength PAH features
</TD></TR>
<TR>
<TD>Leinert C. </TD>
<TD>Max-Planck-Institute f. Astronomie, Heidelberg </TD>
<TD> Spectral Energy distribution of binary T Tauri stars, Part 1
</TD></TR>
<TR>
<TD>Lellouch E. </TD>
<TD>Observatoire de Paris, Section de Meudon </TD>
<TD> Deuterium on Jupiter and Saturn
</TD></TR>
<TR>
<TD>Lellouch E. </TD>
<TD>Observatoire de Paris, Section de Meudon </TD>
<TD> The surface temperature of Pluto
</TD></TR>
<TR>
<TD>Lemke D. </TD>
<TD>Max-Planck-Institut f. Astronomie, Heidelberg </TD>
<TD> Search for very cold dust outside the optical disks of galaxies
</TD></TR>
<TR>
<TD>Lequeux J. </TD>
<TD>Observatoire de Paris </TD>
<TD> CAM-CVF observations of the nuclear region of M 31
</TD></TR>
<TR>
<TD>Levine D. </TD>
<TD>ISO-SOC, ESA, Vilspa / IPAC (CalTech / JPL) </TD>
<TD> A Superbubble Surrounding the Quintuplet at the Galactic Center?
</TD></TR>
<TR>
<TD>Lis D. </TD>
<TD>California Institute of Technology </TD>
<TD> Star formation in the galactic center dust ridge - search for embedded FIR
sources
</TD></TR>
<TR>
<TD>Liseau R. </TD>
<TD>Stockholm Observatory </TD>
<TD> LWS spectroscopy of the star forming Rho Ophiuchi cloud
Physical conditions in the condensed `absorption cores'
<BR>
</TD></TR>
<TR>
<TD>Lisse C. </TD>
<TD>University of Maryland </TD>
<TD> Large-Scale Observations of Scattered Sunlight and Thermal Emission
in the Tails of Bright Periodic Comets
<BR>
</TD></TR>
<TR>
<TD>Little L. </TD>
<TD>Electronics Lab., University of Kent at Canterbury </TD>
<TD> C <IMG WIDTH=9 HEIGHT=7 ALIGN=BOTTOM ALT="tex2html_wrap_inline158" SRC="img7.gif" > and O distribution in the molecular cloud G34.3+0.2
</TD></TR>
<TR>
<TD>Liu X. </TD>
<TD>University College London </TD>
<TD> Far-IR fine-structure lines in planetary nebulae -
a key to resolving discrepancies in abundance determinations
<BR>
</TD></TR>
<TR>
<TD>Lo K. </TD>
<TD>Department of Astronomy, University of Illinois </TD>
<TD> Pre-starbursts in Luminous Infrared Galaxies
</TD></TR>
<TR>
<TD>Lu N. </TD>
<TD>IPAC </TD>
<TD> Disentangle the Merging Sequence of Ultraluminous IR Galaxies
</TD></TR>
<TR>
<TD>Lutz D. </TD>
<TD>Max-Planck-Institut f. Extraterrestrische Physik, Garching </TD>
<TD> Infrared [FeVII] lines as Narrow Line Region diagnostics
</TD></TR>
<TR>
<TD>Lutz D. </TD>
<TD>Max-Planck-Institut f. Extraterrestrische Physik, Garching </TD>
<TD> The Mid-infrared Extinction Law towards the Galactic Center
</TD></TR>
<TR>
<TD>Maiolino R. </TD>
<TD>Max-Planck-Institut f. Extraterrestrische Physik, Garching </TD>
<TD> Imaging spectroscopy of the starbursts NGC 4945 and IC342 - disentangling
starforming regions
</TD></TR>
<TR>
<TD>Malhotra S. </TD>
<TD>IPAC </TD>
<TD> Studying Dust in Gravitational Lenses at High Redshift
</TD></TR>
<TR>
<TD>Malkan M. </TD>
<TD>University of California at Los Angeles </TD>
<TD> Dust in Proto-Galaxies - The First Measurements of the Rest-Frame IR
Emission From Young Galaxies
</TD></TR>
<TR>
<TD>Malkan M. </TD>
<TD>University of California at Los Angeles </TD>
<TD> An infrared emission-line search for obscured Active Nuclei - surveying
four subsamples of the strongest candidates
<BR>
</TD></TR>
<TR>
<TD>Mann R. </TD>
<TD>Astrophysics Group, Blackett Lab., Imperial College </TD>
<TD> Morphological disturbance and star formation in IRAS galaxies
</TD></TR>
<TR>
<TD>Martin-Pintado A. </TD>
<TD>Observatorio Astronomico Nacional, Alcala de Henares </TD>
<TD> On the properties of the Giant Molecular Clouds in the Galactic
</TD></TR>
<TR>
<TD>Mattila K. </TD>
<TD>University of Helsinki Observatory </TD>
<TD> Spectrophotometry of diffuse dust emission in the Galaxy -
UIR band carriers, small and large grains.
</TD></TR>
<TR>
<TD>Mattila K. </TD>
<TD>University of Helsinki Observatory </TD>
<TD> UIR bands in the disks of edge-on spiral galaxies
</TD></TR>
<TR>
<TD>Mazzei P. </TD>
<TD>Osservatorio Astronomico, Padova </TD>
<TD> Infrared properties of barred galaxies
</TD></TR>
<TR>
<TD>McBreen B. </TD>
<TD>University College Dublin </TD>
<TD> ISO Observations of Wolf-Rayet Galaxies - HII type Galaxy with an AGN
Signature
</TD></TR>
<TR>
<TD>McMahon R. </TD>
<TD>Institute of Astronomy, Cambridge </TD>
<TD> Dust masses and the FIR properties of the most distant quasars.
</TD></TR>
<TR>
<TD>Megeath S. </TD>
<TD>MIT Haystack Observatory </TD>
<TD> A search for deeply embedded young stellar objects in the NGC 281 west
cluster
</TD></TR>
<TR>
<TD>Meixner M. </TD>
<TD>Dept. of Astronomy, University of Illinois </TD>
<TD> FIR Imaging Dust Halos of Protoplanetary and Planetary Nebulae -
A Study of Mass Loss History
</TD></TR>
<TR>
<TD>Meixner M. </TD>
<TD>Dept. of Astronomy, University of Illinois </TD>
<TD> Spectroscopy of Atomic Fine Structure Lines in Evolved Stars
- A study of Planetary Nebulae Formation.
</TD></TR>
<TR>
<TD>Meixner M. </TD>
<TD>Dept. of Astronomy, University of Illinois </TD>
<TD> Spectroscopy of Atomic Fine Structure Lines in GL 618
</TD></TR>
<TR>
<TD>Mellier Y. </TD>
<TD>Institut d'Astrophysique de Paris. </TD>
<TD> Arclets in three intermediate redshift clusters
</TD></TR>
<TR>
<TD>Mezger P. </TD>
<TD>Max-Planck-Institut f. Radioastronomie, Bonn </TD>
<TD> Observations of the Galactic Centre with ISO
</TD></TR>
<TR>
<TD>Miley G. </TD>
<TD>Leiden Observatory </TD>
<TD> Dust emission in an unbiased sample of 3CR galaxies - Obscured nuclear activity and
star formation at z ;<I>SPMlt</I>; 0.5
<BR>
</TD></TR>
<TR>
<TD>Miley G. </TD>
<TD>Leiden Observatory </TD>
<TD> Dust in the most distant radio galaxies -
Luminosities and spectral enery distributions
</TD></TR>
<TR>
<TD>Mirabel F. </TD>
<TD>SAP CE-Saclay </TD>
<TD> Follow up of FMIRABEL.CAMACTIV - Starburst and Active galaxies
</TD></TR>
<TR>
<TD>Mirabel F. </TD>
<TD>SAP CE-Saclay </TD>
<TD> Continuation OH HEATDUST
</TD></TR>
<TR>
<TD>Mirabel F. </TD>
<TD>SAP CE-Saclay </TD>
<TD> Continuation of the search for clusters of galaxies at early epochs of the
universe
</TD></TR>
<TR>
<TD>Mobasher B. </TD>
<TD>Astrophysics Group, Blackett Lab., Imperial College </TD>
<TD> Photometry of galaxies in Deep radio selected surveys
</TD></TR>
<TR>
<TD>Molinari S. </TD>
<TD>Instituto di Radioastronomia - CNR, Bologna </TD>
<TD> Spectroscopy of Candidate Progenitors of Ultracompact HII Regions
</TD></TR>
<TR>
<TD>Montmerle T. </TD>
<TD>Service d'Astrophysique - CEA </TD>
<TD> Spectral features of X-Ray irradiated dust - follow-up ISOCAM observations
</TD></TR>
<TR>
<TD>Moorwood A. </TD>
<TD>European Southern Observatory </TD>
<TD> Imaging spectroscopy of the Circinus galaxy
AGN versus starburst ring
</TD></TR>
<TR>
<TD>Murakami H. </TD>
<TD>The Institute of Space and Astronautical Science </TD>
<TD> Spectrophotometry of the UIR bands in the IRTS field.
</TD></TR>
<TR>
<TD>Myers P. </TD>
<TD>Smithonian Astrophysical Observatory </TD>
<TD> Warm Dust Imaging of Nearby Young Stellar Objects
</TD></TR>
<TR>
<TD>Nakagawa T. </TD>
<TD>The Institute of Space and Astronautical Science </TD>
<TD> Large-Scale Multi-Line Spectroscopy of the Galactic Center -
Origins of the Far-Infrared [CII] Line Deficit
</TD></TR>
<TR>
<TD>Neufeld D. </TD>
<TD>The Johns Hopkins University </TD>
<TD> Far-Infrared Line Emission from Shock Heated Gas in Cepheus A -
Fabry-Pérot observations of OI and high-J CO emissions
<BR>
</TD></TR>
<TR>
<TD>Neufeld D. </TD>
<TD>The Johns Hopkins University </TD>
<TD> Search for Far-IR Transitions of Interstellar Hydrogen Halides
</TD></TR>
<TR>
<TD>Noll K. </TD>
<TD>Space Telescope Science Institute, Baltimore </TD>
<TD> Titan's lightcurve at 5 micron: A clue to surface composition
</TD></TR>
<TR>
<TD>Noriega-Crespo A. </TD>
<TD>IPAC </TD>
<TD> Instabilities in Bow Shocks around Runaway OB Stars. A PHOT Map at 60
microns.
</TD></TR>
<TR>
<TD>Noriega-Crespo A. </TD>
<TD>IPAC </TD>
<TD> The Star Forming Region around IRAS 05487+0255.
ISOCAM MAPS of Stellar Jets and their Sources.
</TD></TR>
<TR>
<TD>Okumura K. </TD>
<TD>ISO-SOC, ESA, Vilspa </TD>
<TD> Diffuse interstellar medium in the Small Magellanic Cloud -
Are there PAHs in the Small Magellanic Cloud?
</TD></TR>
<TR>
<TD>Oldham P. </TD>
<TD>Queen Mary and Westfield College </TD>
<TD> Saturn: determination of the tropospheric methane abundance profile
</TD></TR>
<TR>
<TD>Oliva E. </TD>
<TD>Arcetri Observatory, Florence </TD>
<TD> IR spectroscopy of the most luminous LMC Supernova remnant
IR spectroscopy of N49
</TD></TR>
<TR>
<TD>Oliver S. </TD>
<TD>Astrophysics Group, Blackett Lab., Imperial College </TD>
<TD> FIR studies of a complete AGN rich sample
from the Point Source Catalog Redshift Survey
</TD></TR>
<TR>
<TD>Oliver S. </TD>
<TD>Astrophysics Group, Blackett Lab., Imperial College </TD>
<TD> Evolution in the SED of ultraluminous IRAS galaxies
</TD></TR>
<TR>
<TD>Omont A. </TD>
<TD>Institut d'Astrophysique de Paris </TD>
<TD> ISOCAM survey of the inner galaxy
Completion of the ISOGAL 7-15 micron survey
</TD></TR>
<TR>
<TD>Onaka T. </TD>
<TD>Department of Astronomy, University of Tokyo </TD>
<TD> Time variation of spectra of circumstellar envelopes
</TD></TR>
<TR>
<TD>Onaka T. </TD>
<TD>Department of Astronomy, University of Tokyo </TD>
<TD> A systematic study of infrared emission from galaxies
- Complemental study to IRTS/MIRS observations
</TD></TR>
<TR>
<TD>Osip D. </TD>
<TD>University of Florida </TD>
<TD> Spectral analysis of ``carbon-chain depleted'' comets.
Spectral studies of P/Wolf-Harrington.
</TD></TR>
<TR>
<TD>Padovani P. </TD>
<TD>Dip. di Fisica, II Universita' di Roma `Tor Vergata' </TD>
<TD> ISO observations of radio-selected BL Lacs
- Observations of the complete 1 Jy sample
</TD></TR>
<TR>
<TD>Penny A. </TD>
<TD>Rutherford Appleton Laboratory </TD>
<TD> Dust in globular clusters
</TD></TR>
<TR>
<TD>Pequignot D. </TD>
<TD>DAEC, Observatoire de Paris-Meudon </TD>
<TD> Far-infrared spectroscopy of nuclearly processed material
in young supernova remnants.
</TD></TR>
<TR>
<TD>Peschke S. </TD>
<TD>Max-Planck-Institut f. Kernphysik, Heidelberg </TD>
<TD> ToO : Cometary comae in the IR
</TD></TR>
<TR>
<TD>Phillips T. </TD>
<TD>California Institute of Technology </TD>
<TD> Oxygen in molecular clouds
</TD></TR>
<TR>
<TD>Pottasch S. </TD>
<TD>Kapteyn Institute, Groningen </TD>
<TD> Determining Planetary Nebulae Central Star Temperatures
</TD></TR>
<TR>
<TD>Prieto A. </TD>
<TD>Max-Planck-Institut f. Extraterrestrische Physik, Garching </TD>
<TD> The CfA sample of Seyfert galaxies
line spectroscopy with SWS
</TD></TR>
<TR>
<TD>Prusti T. </TD>
<TD>ISO-SOC, ESA, Vilspa </TD>
<TD> Star formation in L1251
Spectral energy distribution of young stellar objects
</TD></TR>
<TR>
<TD>Prusti T. </TD>
<TD>ISO-SOC, ESA, Vilspa </TD>
<TD> 200 micron filler survey for IRAS sources
</TD></TR>
<TR>
<TD>Prusti T. </TD>
<TD>ISO-SOC, ESA, Vilspa </TD>
<TD> Bolometric luminosity functions of near by star forming regions
</TD></TR>
<TR>
<TD>Prusti T. </TD>
<TD>ISO-SOC, ESA, Vilspa </TD>
<TD> Circumstellar environment of pre-main-sequence stars
with variable extinction
</TD></TR>
<TR>
<TD>Prusti T. </TD>
<TD>ISO-SOC, ESA, Vilspa </TD>
<TD> Extended infrared emission around young stars
</TD></TR>
<TR>
<TD>Prusti T. </TD>
<TD>ISO-SOC, ESA, Vilspa </TD>
<TD> Search of the comet-like activity in Beta Pic
</TD></TR>
<TR>
<TD>Prusti T. </TD>
<TD>ISO-SOC, ESA, Vilspa </TD>
<TD> ToO: Evolution of the Circumstellar Environment during an FU Ori
or EX Lup outburst
</TD></TR>
<TR>
<TD>Prusti T. </TD>
<TD>ISO-SOC, ESA, Vilspa </TD>
<TD> Variable infrared emission from circumstellar environment of
young intermediate mass stars
</TD></TR>
<TR>
<TD>Puget J. </TD>
<TD>Institut d'Astrophysique Spatiale, Orsay </TD>
<TD> Spectral survey of the cold interstellar medium -
Search for new features from dust, atom clusters
</TD></TR>
<TR>
<TD>Puget J. </TD>
<TD>Institut d'Astrophysique Spatiale, Orsay </TD>
<TD>Structure of the far infrared background
</TD></TR>
<TR>
<TD>Rauer H. </TD>
<TD>Observatoire de Paris-Meudon </TD>
<TD> IR absorption features of extra-solar planets -
Search for an extended enveloppe around 51 Peg B
</TD></TR>
<TR>
<TD>Reach W. </TD>
<TD>Institut d'Astrophysique Spatiale, Orsay </TD>
<TD> Imaging the source of cometary dust trails
</TD></TR>
<TR>
<TD>Reach W. </TD>
<TD>Institut d'Astrophysique Spatiale, Orsay </TD>
<TD> Mapping the interstellar cooling lines in the SMC
</TD></TR>
<TR>
<TD>Reach W. </TD>
<TD>Institut d'Astrophysique Spatiale, Orsay </TD>
<TD> Spectrum of the zodiacal light
</TD></TR>
<TR>
<TD>Reach W. </TD>
<TD>Institut d'Astrophysique Spatiale, Orsay </TD>
<TD> Supernova interactions with molecular clouds
and their influence on X-ray remnant morphology
</TD></TR>
<TR>
<TD>Richards P. </TD>
<TD>The Rutherford Appleton Laboratory </TD>
<TD> Dust in galactic open clusters
</TD></TR>
<TR>
<TD>Rieke G. </TD>
<TD>Steward Observatory </TD>
<TD> Low mass pleiades brown dwarfs
</TD></TR>
<TR>
<TD>Rieke G. </TD>
<TD>Steward Observatory </TD>
<TD> Star Formation and Evolution of Seyfert Nuclei
</TD></TR>
<TR>
<TD>Rieke M. </TD>
<TD>Steward Observatory </TD>
<TD> Mid-Infrared Output of the Quiescent Galaxy NGC3115
</TD></TR>
<TR>
<TD>Rieke M. </TD>
<TD>Steward Observatory </TD>
<TD> The Star Formation Rate in Coma E+A Galaxies
</TD></TR>
<TR>
<TD>Rigopoulou D. </TD>
<TD>Max-Planck-Institut f. Extratterestrische Physik, Garching </TD>
<TD> The nature and radiation field of Ultraluminous IR Galaxies
- A survey using 6-12 <IMG WIDTH=10 HEIGHT=12 ALIGN=MIDDLE ALT="tex2html_wrap_inline152" SRC="img5.gif" > m emission features
</TD></TR>
<TR>
<TD>Rocca-Volmerange B. </TD>
<TD>Institut d'Astrophysique de Paris </TD>
<TD> Galaxy Luminosity Functions by types from the ESO-Sculptor redshift sample
</TD></TR>
<TR>
<TD>Roche P. </TD>
<TD>Oxford University </TD>
<TD> Spectral features in carbon-rich stellar envelopes
</TD></TR>
<TR>
<TD>Rodriguez Espinosa J. </TD>
<TD>Instituto de Astrofisica de Canarias </TD>
<TD> The Spectral Energy Distribution of Seyfert Galaxies
- The Center for Astrophysics Seyfert sample
</TD></TR>
<TR>
<TD>Rouan D. </TD>
<TD>Observatoire de Paris-Meudon </TD>
<TD> ISM in edge-on galaxies : the PAHS/very small grains component
</TD></TR>
<TR>
<TD>Rowan-Robinson M. </TD>
<TD>Astrophysics Group, Blackett Lab., Imperial College </TD>
<TD> Photometric follow-up of the ELAIS survey and extension
of the survey to 6.7 microns
</TD></TR>
<TR>
<TD>Rowan-Robinson M. </TD>
<TD>Astrophysics Group, Blackett Lab., Imperial College </TD>
<TD> An ISO Survey of the Southern Hubble Deep Field
</TD></TR>
<TR>
<TD>Rowan-Robinson M. </TD>
<TD>Astrophysics group, Blackett Lab., Imperial College </TD>
<TD> Photometry of extreme ultraluminous IRAS galaxies - the PSCz sample
</TD></TR>
<TR>
<TD>Rubin R. </TD>
<TD>NASA AMES Research Center (Orion Enterprises) </TD>
<TD> ISO Spectral Analysis of Planetary Nebulae: Densities,
Temperatures, and Abundances
</TD></TR>
<TR>
<TD>Rubin R. </TD>
<TD>NASA AMES Research Center (Orion Enterprises) </TD>
<TD> Iron Abundance in the Orion Nebula - Unique Contributions From
[FeIII] and [FeIV] Lines
</TD></TR>
<TR>
<TD>Salama A. </TD>
<TD>ISO-SOC, ESA, Vilspa </TD>
<TD> ISO observations of old novae
</TD></TR>
<TR>
<TD>Saxton R. </TD>
<TD>ISO-SOC, ESA, Vilspa </TD>
<TD> Determining the timescale of infrared variability in Blazers.
</TD></TR>
<TR>
<TD>Schild H. </TD>
<TD>Institut f. Astronomie, Zuerich </TD>
<TD> Dust in symbiotic binaries
</TD></TR>
<TR>
<TD>Schoenberner D. </TD>
<TD>Astrophysikalisches Institut Potsdam </TD>
<TD> Probing mass loss variations of AGB stars with detached shells -
Differences in mass loss behavior for C- and O-rich AGB stars
<BR>
</TD></TR>
<TR>
<TD>Schutte W. </TD>
<TD>Leiden Observatory </TD>
<TD> The 2.75 micron feature of hydrated silicates
</TD></TR>
<TR>
<TD>Sellgren K. </TD>
<TD>Astronomy Department, Ohio State University </TD>
<TD> Imaging of infrared emission features in reflection nebulae
</TD></TR>
<TR>
<TD>Serra G. </TD>
<TD>CESR/CNRS, Toulouse </TD>
<TD> Dust and gas properties of extended cold cores in the ISM
- A study of dust matter inside cold cores
</TD></TR>
<TR>
<TD>Siebenmorgen R. </TD>
<TD>ISO-SOC, ESA, Vilspa </TD>
<TD> Polarimetry of ultraluminous IRAS galaxies
Starbursts or AGN?
</TD></TR>
<TR>
<TD>Siebenmorgen R. </TD>
<TD>ISO-SOC, ESA, Vilspa </TD>
<TD> The energetics of extended emission around Herbig He/Be stars
</TD></TR>
<TR>
<TD>Skinner C. </TD>
<TD>Space Telescope Science Institute, Baltimore </TD>
<TD> PAHS and chromospheres in M-Supergiants
</TD></TR>
<TR>
<TD>Skinner C. </TD>
<TD>Space Telescope Science Institute, Baltimore </TD>
<TD> Photometry of a New Sample of Candidate Vega-Excess Sources
Properties of Circumstellar Discs
</TD></TR>
<TR>
<TD>Skinner C. </TD>
<TD>Space Telescope Science Institute, Baltimore </TD>
<TD> CO Observations of Mass-Loss in Low-Mass Post-Main Sequence Stars
</TD></TR>
<TR>
<TD>Smith H. </TD>
<TD>Smithsonian Institution </TD>
<TD> A spectroscopic study of OH lines in megamaser galaxies
</TD></TR>
<TR>
<TD>Smith M. </TD>
<TD>Astronomisches Institut, Universitaet Wuerzburg </TD>
<TD> Warm CO in the Youngest Protostellar Outflows
</TD></TR>
<TR>
<TD>Spinoglio L. </TD>
<TD>Istituto di Fisica dello Spazio Interplanetario, Frascati </TD>
<TD> IR energy distributions and imaging of the complete sample of 12 <IMG WIDTH=10 HEIGHT=12 ALIGN=MIDDLE ALT="tex2html_wrap_inline152" SRC="img5.gif" > m active
galaxies - Towards the unification of active galactic nuclei.
<BR>
</TD></TR>
<TR>
<TD>Stacey G. </TD>
<TD>Cornell University </TD>
<TD> LWS molecular line observations of M82 and NGC 253
</TD></TR>
<TR>
<TD>Stark R. </TD>
<TD>Max-Planck-Institut f. Radioastronomie, Bonn </TD>
<TD> FIR line emission from galactic high-latitude clouds
</TD></TR>
<TR>
<TD>Stark R. </TD>
<TD>Max-Planck-Institut f. Radioastronomie, Bonn </TD>
<TD> The UV radiation field illuminating L183
</TD></TR>
<TR>
<TD>Stencel R. </TD>
<TD>University of Denver, Dept. Astronomy </TD>
<TD> PHOT reobservation of VEGA disk stars
</TD></TR>
<TR>
<TD>Sternberg A. </TD>
<TD>MPE, Garching </TD>
<TD> Mid-infrared spectroscopy of LINERS - the AGN connection
</TD></TR>
<TR>
<TD>Stringfellow G. </TD>
<TD>CASA, University of Colorado </TD>
<TD> Replenishment of the Accretion Disk Between Outbursts in EXORs -
Characterizing the Variable Infrared Emission of Accreting YSOs
<BR>
</TD></TR>
<TR>
<TD>Szczerba R. </TD>
<TD>N. Copernicus Astronomical Center, Torun </TD>
<TD> Detailed investigation of the 30 micron band -
Search for the 30 micron emitters
</TD></TR>
<TR>
<TD>Szczerba R. </TD>
<TD>N. Copernicus Astronomical Center, Torun </TD>
<TD> Excitation conditions in shells of post-AGB objects
Search for precursors of planetary nebulae with WR type
</TD></TR>
<TR>
<TD>Takashi T. </TD>
<TD>Institute of Astronomy, The University of Tokyo </TD>
<TD> Dust Formation in the Photospheres of Very Low Mass Stars
- From M dwarfs to brown dwarfs
</TD></TR>
<TR>
<TD>Tanabe T. </TD>
<TD>Institute of Astronomy, The University of Tokyo </TD>
<TD> Mass-Loss in the Late Stages of Stellar Evolution
III. AGB Stars in the Magellanic Clouds Star Clusters II.
</TD></TR>
<TR>
<TD>Tanabe T. </TD>
<TD>Institute of Astronomy, The University of Tokyo </TD>
<TD> Spectrophotometric observations of AGB stars in the Magellanic
Clouds star clusters II
</TD></TR>
<TR>
<TD>Tedesco E. </TD>
<TD>Terra Systems, Inc. </TD>
<TD> Asteroid size-frequency distribution
</TD></TR>
<TR>
<TD>Teixeira T. </TD>
<TD>Dept. of Physics, Queen Mary and Westfield College </TD>
<TD> Deuteration in Grain Mantles
The Missing Link
</TD></TR>
<TR>
<TD>Thuan T. </TD>
<TD>University of Virginia Department of astronomy </TD>
<TD> The interstellar medium in the young galaxy system
SBS 0335-052 and its companion
</TD></TR>
<TR>
<TD>Thum C. </TD>
<TD>IRAM, St Martin d`Heres </TD>
<TD> The Recombination Line Maser MWC349 -
Velocity-resolved Spectroscopy and Molecular Transitions
</TD></TR>
<TR>
<TD>Timmermann R. </TD>
<TD>Univerisitaet zu Koeln </TD>
<TD> Low velocity shocks in the dense medium of outflows
</TD></TR>
<TR>
<TD>Trams N. </TD>
<TD>ISO-SOC, ESA, Vilspa </TD>
<TD> IR Spectro photometry and 60 micron photometry
of LMC and SMC AGB stars
</TD></TR>
<TR>
<TD>Trewhella M. </TD>
<TD>Department of Physics and Astronomy, Cardiff </TD>
<TD> Dust in Spiral Galaxies
Energy distribution and Temperature
</TD></TR>
<TR>
<TD>Tuffs R. </TD>
<TD>Max Planck Institut f. Kernphysik, Heidelberg </TD>
<TD> Heating and Metallicity in the Extended HI Disks around
NGC 891 and NGC 6946
</TD></TR>
<TR>
<TD>Tuffs R. </TD>
<TD>Max Planck Institut f. Kernphysik, Heidelberg </TD>
<TD> Observations of Gas and Dust in Supernova Remnants
</TD></TR>
<TR>
<TD>Unger S. </TD>
<TD>Space Science Dept, RAL </TD>
<TD> A time variable plerion: modelling the BE star disk in the unique
milli-second pulsar binary system PSR B1259-63
<BR>
</TD></TR>
<TR>
<TD>Van der Hulst J. </TD>
<TD>Kapteyn Astronomical Institute, Groningen </TD>
<TD> Far IR observations of Low Surface Brightness Galaxies - Search for
cool dust in Low Surface Brightness Galaxies
<BR>
</TD></TR>
<TR>
<TD>Van der Werf P. </TD>
<TD>Leiden Observatory </TD>
<TD> Deep ISOCAM imaging of faint blue galaxies and
microjansky radio sources in the deepest VLA field
</TD></TR>
<TR>
<TD>Van der Werf P. </TD>
<TD>Leiden Observatory </TD>
<TD> Shocked molecular gas in NGC6240 and Arp220 -
Measuring energy dissipation and gas flow to the centre
</TD></TR>
<TR>
<TD>Van Dishoeck E. </TD>
<TD>Leiden Observatory </TD>
<TD> The chemistry of H <IMG WIDTH=5 HEIGHT=10 ALIGN=MIDDLE ALT="tex2html_wrap_inline136" SRC="imgx.gif" > O and CO <IMG WIDTH=5 HEIGHT=10 ALIGN=MIDDLE ALT="tex2html_wrap_inline136" SRC="imgx.gif" > in star-forming regions
</TD></TR>
<TR>
<TD>Van Hoof P. </TD>
<TD>Kapteyn Astronomical Institute, Groningen </TD>
<TD> Accurate abundance determination of CNO in PN.
An investigation into the t <SUP>2</SUP> problem.
</TD></TR>
<TR>
<TD>Van Hoof P. </TD>
<TD>Kapteyn Astronomical Institute, Groningen </TD>
<TD> A search for PN with carbon and oxygen dust-features
</TD></TR>
<TR>
<TD>Verma R. </TD>
<TD>TATA Institute of Fundamental Research, Mumbai </TD>
<TD> Mid infrared imaging of ultra compact HII regions/ CO clumps
</TD></TR>
<TR>
<TD>Viallefond F. </TD>
<TD>Observatoire de Paris </TD>
<TD> CAM-CVF observations of NGC 604 in the nearby galaxy M 33
</TD></TR>
<TR>
<TD>Volk K. </TD>
<TD>University of Calgary </TD>
<TD> Observation of the 21 micron feature prototype IRAS07134+1005
</TD></TR>
<TR>
<TD>Volk K. </TD>
<TD>University of Calgary </TD>
<TD> Study of Low Temperature, featureless IRAS sources
</TD></TR>
<TR>
<TD>Voors R. </TD>
<TD>Astronomical Institute, University of Utrecht </TD>
<TD> Disks around B[e]-supergiants
</TD></TR>
<TR>
<TD>Waelkens C. </TD>
<TD>Instituut voor Sterrenkunde, Leuven </TD>
<TD> Accurate modelling of cool-star atmospheres
</TD></TR>
<TR>
<TD>Waelkens C. </TD>
<TD>Instituut voor Sterrenkunde, Leuven </TD>
<TD> Jupiters and circumstellar dust disks around southern G dwarfs
</TD></TR>
<TR>
<TD>Waelkens C. </TD>
<TD>Instituut voor Sterrenkunde, Leuven </TD>
<TD> Detailed mineralogy of the oxygen-rich dust around young stars
</TD></TR>
<TR>
<TD>Walker H. </TD>
<TD>Rutherford Appleton Laboratory </TD>
<TD> Mapping of R CRB dust shells
</TD></TR>
<TR>
<TD>Walker H. </TD>
<TD>Rutherford Appleton Laboratory </TD>
<TD> Mapping the environment of VEGA-like candidates
</TD></TR>
<TR>
<TD>Waller W. </TD>
<TD>Hughes STX, NASA/GSFC </TD>
<TD> Starburst anatomy
IR spectral imaging of giant HII regions in M33
</TD></TR>
<TR>
<TD>Ward M. </TD>
<TD>University of Leicester </TD>
<TD> Narrow-Line Seyfert 1s : the Infrared Connection
</TD></TR>
<TR>
<TD>Ward-Thompson D. </TD>
<TD>Royal Observatory, Edinburgh </TD>
<TD> Pre-stellar
Cores
</TD></TR>
<TR>
<TD>Waters R. </TD>
<TD>Astronomical Institute `Anton Pannekoek', Amsterdam </TD>
<TD> IR spectroscopy of OB dwarfs -
probing the outer layers of the atmosphere
</TD></TR>
<TR>
<TD>Waters R. </TD>
<TD>Astronomical Institute `Anton Pannekoek', Amsterdam </TD>
<TD> Mineralogy of crystalline dust -
oxygen rich dust shells in evolved stars
</TD></TR>
<TR>
<TD>Wehrle A. </TD>
<TD>IPAC </TD>
<TD> The Energy Emission Mechanism of Gamma-Ray Blazars
</TD></TR>
<TR>
<TD>Wehrse R. </TD>
<TD>Institut f. Theoretische Astrophysik, Heidelberg </TD>
<TD> ISOPHOT Backgound Observations for M Dwarfs
</TD></TR>
<TR>
<TD>Werner M. </TD>
<TD>JPL/CALTECH </TD>
<TD> Studies of Wolf-Rayet Galaxies
</TD></TR>
<TR>
<TD>Wesselius P. </TD>
<TD>SRON Space Laboratory Groningen </TD>
<TD> Solid <SUP>12</SUP>CO <IMG WIDTH=5 HEIGHT=10 ALIGN=MIDDLE ALT="tex2html_wrap_inline136" SRC="imgx.gif" > and <SUP>13</SUP>CO <IMG WIDTH=5 HEIGHT=10 ALIGN=MIDDLE ALT="tex2html_wrap_inline136" SRC="imgx.gif" > ice absorption features -
the galactic <SUP>12</SUP>C/ <SUP>13</SUP>C abundance ratio
</TD></TR>
<TR>
<TD>Wilking B. </TD>
<TD>University of Missouri-St. Louis </TD>
<TD> The Nature of Weak Radio Sources in the rho Oph Cloud Core
</TD></TR>
<TR>
<TD>Willis A. </TD>
<TD>University College London </TD>
<TD> IR Spectroscopy of Wolf-rayet Starburst Galaxies
</TD></TR>
<TR>
<TD>Willis A. </TD>
<TD>University College London </TD>
<TD> The Neon + Magnesium Abundances in WC Stars
</TD></TR>
<TR>
<TD>Wilson T. </TD>
<TD>Max-Planck-Institut f. Radioastronomie, Bonn </TD>
<TD> Molecular cloud cores in Orion -
star formation in Orion
</TD></TR>
<TR>
<TD>Wright C. </TD>
<TD>Max-Planck-Institut f. Extraterrestrische Physik, Garching </TD>
<TD> Absorption in the cold ISM toward the Galactic Center
Molecular hydrogen
</TD></TR>
<TR>
<TD>Xu C. </TD>
<TD>Max Planck Institut f. Kernphysik, Heidelberg </TD>
<TD> Ionizing flux and extinction
in closely interacting spiral-spiral pairs
</TD></TR>
<TR>
<TD>Yamamura I. </TD>
<TD>SRON Laboratory for Space Research, Groningen </TD>
<TD> High-Resolution Spectroscopy of IRTS Template Stars.
</TD></TR>
<TR>
<TD>Yui Y. </TD>
<TD>Communications Research Laboratory, Koganei </TD>
<TD> H <IMG WIDTH=5 HEIGHT=10 ALIGN=MIDDLE ALT="tex2html_wrap_inline136" SRC="imgx.gif" > Molecule Lines in rho-Oph Cloud -
UV Radiation Field in Dark Clouds
</TD></TR>
<TR>
<TD>Zijlstra A. </TD>
<TD>European Southern Observatory </TD>
<TD> Carbon stars and [WC]-planetary nebulae in the
Sagittarius dwarf spheroidal galaxy
</TD></TR>
</TABLE>
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