1. MOLECULES IN ASTROPHYSICS - WINNEWISSER, G.
Author Institution: Max-Planck-Institut f\""{U}r Radioastronomie.

2. VIBRATIONAL SATELLITES AS A MEANS TO STUDY DENSE AND HOT PARTS OF THE INTERSTELLAR MEDIUM. RESULTS OF A 3 mm LINE SURVEY OF SAGITTARIUS B2(N) AND (M) - Muller, Holger S. P.; Belloche, Arnaud; Menten, Karl M.; Comito, Claudia; Schilke, Peter
Author Institution: I.

3. INTERSTELLAR METHANOL - Menten, Karl M.
Author Institution: Max-Planck-Institut f\""{u}r Radioastronomie, Auf dem H\""{u}gel 69.

4. THE SEARCH FOR COMPLEX MOLECULES IN THE ISM: A 3mm LINE SURVEY OF SgrB2 - Comito, Claudia; Belloche, Arnaud; Hieret, Carolin; Menten, Karl M.; Schilke, Peter; Muller, Holger S.P.
Author Institution: Max-Planck-Institut fur Radioastronomie, Auf dem Hugel; 69, 53121 Bonn, Germany; Physikalisches Institut, Universitat zu Koln, Zulpicher; Strasse 77, 50937 Koln, Germany.

5. LABORATORY AND TENTATIVE ASTRONOMICAL DETECTION OF THIOCYANIC ACID, HSCN - Brunken, Sandra; Yu, Zhenhong; McCarthy, Michael C.; Gottlieb, Carl A.; Thaddeus, Patrick; Belloche, Arnaud; Menten, Karl M.
Author Institution: Harvard Smithsonian Center for Astrophysics and School of Engineering and Applied Sciences, Harvard University, Cambridge, MA 02138; Max-Planck-Institut fur Radioastronomie, 53121 Bonn, Germany.

6. THE MICROWAVE AND MILLIMETER WAVE SPECTRUM OF ISOTHIOCYANIC ACID, HNCS - SZALANSKI, L.B.; GERRY, M.C.L.; WINNEWISSER, G.; WINNEWISSER, M.
Author Institution: Department of Chemistry, The University of British Columbia; Department of Chemistry, Max-Planck-Institut f\""{U}r Radioastronomie Bonn; Department of Chemistry, Physikalisch-Chemisches-Institut der Justus-Liebig-Universit\""{a}t.

7. TESTING THE LIMITS OF INTEGRATION TIME (AND OBSERVER PATIENCE): DETECTION OF INTERSTELLAR KCN - Savage. C.; Ziurys, L. M.; Guelin, M.
Author Institution: Department of Chemistry, Department of Astronomy, and Steward Observatory, University of Arizona; Department of Chemistry, Department of Astronomy, and Steward Observatory, Institut de RadioAstronomie Millim\'{e}trique, 300 rue de la Piscine, Domaine Universitaire.

8. A SURVEY OF LARGE MOLECULES TOWARD THE PROTOPLANETARY NEBULA CRL 618 - Remijan, Anthony J.; Wyrowski, Friedrich; Friedel, D.N.; Meier, D.S.; Snyder, L.E.
Author Institution: NASA Goddard Space Flight Center, Computational and Information Sciences and Technology Office, Code 606, Greenbelt, MD 20771; Max-Planck-Institut fur Radioastronomie, Auf dem Hugel; 69, D-53121 Bonn, Germany; Department of Astronomy, University of Illinois, Urbana, IL 61801.

9. ROTATIONAL SPECTROSCOPY AND MOLECULAR PROPERTIES OF TITANIUM DIOXIDE, TiO$_2$ - Müller, Holger S.P.; Brünken, Sandra; McCarthy, Michael C.; Thaddeus, Patrick
Author Institution: I.

10. COMPLEX ORGANIC MOLECULES IN HOT CORINOS AND HOT CORES - Bottinelli, Sandrine; Ceccarelli, Cecilia; Williams, Jonathan P.; Neri, Roberto
Author Institution: Laboratoire d'Astrophysique de l'Observatoire de Grenoble,; BP 53, 38041 Grenoble Cedex 9, France, and; Institute for Astronomy, University of Hawai`i,; 2680 Woodlawn Drive, Honolulu, HI 96822; Laboratoire d'Astrophysique de l'Observatoire de Grenoble,; BP 53, 38041 Grenoble Cedex 9, France; Institute for Astronomy, University of Hawai`i,; 2680 Woodlawn Drive, Honolulu, HI 96822; Institut de Radioastronomie Millimetrique (IRAM),; 300 rue de la Piscine, 38406 Saint Martin d'Heres, France.

11. A NEW MODEL FOR COMPLEX CHEMISTRY IN HOT CORES - Widicus Weaver, Susanna L.; Garrod, Robin; Herbst, Eric
Author Institution: Departments of Chemistry and Astronomy, University of Illinois at Urbana-Champaign, Urbana, IL 61801; Max-Planck-Institut fur Radioastronomie, 53121 Bonn, Germany; Department of Physics, The Ohio State University, Columbus,; OH 43210, USA; Departments of Astronomy and Chemistry, The Ohio; State University, Columbus, OH 43210, USA.

12. A LABORATORY AND THEORETICAL INVESTIGATION OF THE SILICON SULFUR MOLECULES H$_2$SiS AND Si$_2$S - McCarthy, Michael C.; Thaddeus, Patrick; Gupta, Harshal; Thorwirth, Sven; Gauss, Jurgen
Author Institution: Harvard-Smithsonian Center for Astrophysics, 60 Garden St.; Cambridge, MA 02138, and School of Engineering \& Applied Sciences, Harvard University, 29 Oxford St., Cambridge, MA 02138; Institute for Theoretical Chemistry, Department of Chemistry and Biochemistry, University of Texas at Austin, Austin, Texas 78712; Max-Planck-Institut fur Radioastronomie, Auf dem Hugel 69, 53121 Bonn, Germany; Institut fur Physikalische Chemie, Johannes Gutenberg-Universitat Mainz, Jakob-Welder-Weg 11, D-55128 Mainz, Germany.

13. A high sensitivity HI survey of the sky at delta < -25 deg Final data release - Bajaja, E.; Arnal, E. M.; Larrarte, J. J.; Morras, R.; Poppel, W. G. L.; Kalberla, P. M. W.
A total of 50980positions lying on a galactic coordinate grid with points spaced by (Delta l,Delta b) = ((0.5 deg)/cos b, 0.5 deg) were observed with the 30-m dish of theInstituto Argentino de Radioastronomia (IAR).

14. BSSDATA - Protótipo de um sistema otimizado para tratamento e análise de dados do brasilian solar spectroscope - André Ricardo Fazanaro Martinon
Este trabalho propõe um sistema otimizado para tratamento e análise de dados em radioastronomia solar, específico para o Espectrógrafo Solar BSS Brazilian Solar Spectroscope, INPE.

15. The Leiden/Argentine/Bonn (LAB) Survey of Galactic HI: Final data release of the combined LDS and IAR surveys with improved stray-radiation corrections - Kalberla, P. M. W.; Burton, W. B.; Hartmann, Dap; Arnal, E. M.; Bajaja, E.; Morras, R.; Poppel, W. G. L.
We present the final data release of observations of lambda 21-cm emissionfrom Galactic neutral hydrogen over the entire sky, merging theLeiden/Dwingeloo Survey (LDS: Hartmann & Burton, 1997) of the sky north ofdelta = -30 deg with the Instituto Argentino de Radioastronomia Survey (IAR:Arnal et al., 2000, and Bajaja et al., 2005) of the sky south of delta = -25deg.

16. Orbital variability of the PSR J2051-0827 Binary System - Doroshenko, O.; Loehmer, O.; Kramer, M.; Jessner, A.; Wielebinski, R.; Lyne, A. G.; Lange, Ch.
The 6.5-yrs radio timing measurements have revealeda significant secular variation of the projected semi-major axis of the pulsarat a rate of $\dot x\equiv d(a_{\rm 1} \sin i)/dt = (-0.23\pm 0.03)\times10^{-12}$, which is probably caused by the Newtonian spin-orbit coupling inthis binary system leading to a precession of the orbital plane.

17. Calibration Validation and Polarimetry in 2D Aperture Synthesis. Application to MIRAS - Ribó Vedrilla, Serni
RESUMLa missió SMOS de l'Agència Europea de l'Espai (ESA) té com a objectiu mesurar la humitat del sòl i la salinitat dels oceans, paràmetres fonamentals per tal d'entendre el canvi climàtic global.