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A. Doressoundiram, F. Roques, and Y. Boissel, Probing the radial distribution of the Kuiper Belt, using the ESO-VLT

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Y. Shih*"è, &. Boissel, H. Chang'7, A. Doressoundiram, &. et al., Taiwan E-mail: stephen.shih@obspm.fr MIOSOTYS (Multi-object Instrument l'or Occultation in the SOlar System and TransitorY Sys tems) is a multiple-object, high-speed photometer primarily designed for the observation of serendipitous stellar occultations by small (less than or of the order of 1 km at 40 AU) transneptunian objects as well as other high lime resolution astronomical subjects. It is currently a visiting instrument to the 1.93m telescope at Observatoire de Haute-Provence (OHP), France, J. Guérin, 2010.

I. Shih, A. Doressoundiram, and Y. Boissel, Introduction to MIOSOTYS: a multiple-object, high-speedphotometer, 2010.

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I. Shih and &. Y. Boissel, MIOSOTYS data réduction and analysis

S. Conférence, Proceedings. Introduction to MIOSOTYS: a multiple-object, 2010.

C. Shiha, /\ Alain Doressoundiram6. Yannick Boissel6, Françoise Roques6, Frédéric Dauny6

P. Felenbok6, A. Fernandez6, J. Guérin6, K. Hsiang, and . Chang, Chih-Yuan Liua'6 "Institute of Astronomy

6. , O. De-paris, and . Meudon, France the performance, i.e., signal-to-noise ratio

, Each arm sweeps a triangular zone by 2 motions: translation by 130mm and rotation by ± 7 degree. The image fibre is fixed on the arm tip which is electrically insulated. The image fibre is a glass fibre bundle of 900mm long, the diameter of the elementary fibre is 18/im. Its transmission efficiency is about 40-45%. The viewing surface is 1.9x 1.9mm. The output end of the 29 image fibres are projected on to a CCD caméra through the optics of AGIS with a réduction factor. 2.2 EMCCD caméra We chose the ProEM? caméra manufactured by Princeton Instruments* as the imaging sensor for the instru ment. The sensor of e2v CCD201B is a back-illuminated, frame-transfer EMCCD with 1024x1024 image pixels (or active area 13.3x13.3 mm). The large image area can cover ail of 29 fibre images. The peak Q.E. at 530 nm is 95%. The air cooling System maintains the operating température at-55°C or lower, Time résolution, Imaging, Photometry 2.1 Arms and fibres There are 30 positioning arms

, The EMCCD lias dual readout amplifiers (or ports, see figure 1), one is a traditional sériés register for LN

&. If-tp and . Tr, however, one should be aware of that the exposed sensor has to wait for the

L. Mortara and A. Fowler, Evaluations of charge-coupled device / ccd / performance for astronomical use, Solid State Imagers For Astronomy: proc. SPIE, vol.290, p.28, 1981.

, Annexe 4 : Poster DPS 2008 Search for simili satellites and rings orbitting Pluto through stellar occultations N

F. Observatoire-de-paris and . Paris,

. Fédéral-do-rio-de-janeiro, . Observatorio-do-valongo, . Brésil, . De-vajongo, . Brésil et al., Abstract: Uaing data obtained during stellar occultation* by Pluto in 2006-2008, we hâve aearched foc faint materiel and sroall satellites around Pluto W« hâve selected the beat Hght curvea

, These light curves hâve been used to scan Pluto surroundings up to Six and Hydra's ortuts. The flux versus time data hâve been transformed into flux versus distance in Pluto'* équatorial plane. The équivalent width of putative material (ring* or email satellites) has been computed into slkimg Windows. No aeoondaiy evenU corresponding to rings with équivalent width of a fraction of km hâve been detected yet, and no individuel objecU vrith aize of 100 m or ao hâve been found, beat ESO Paranal, the 14 lune 2007 frora Pico dos Dias (Brazil) and the 24 June 2008 hum Mauna Kea/CFHT (Hawaii), 2006.

J. Conférences, occasion durant cette thèse de participer à quelques conférences et workshops. J'ai présenté un poster au colloque d'Octobre 2008 du DPS (voir annexe J), Division for Planetary Science, le rassemblement international annuel de la planétologie

, Search for Small Satellites and Rings Orbiting Pluto

J. Pu-rencontrer-georges-georgevits-À-sydney, l'ingénieur et étudiant en thèse à l'origine des observations d'occultations d'OTNs avec l'instrument 6df, en, 2008.

, sur les logiciels de MIOSOTYS, la recherche de champs stellaires, les observations à l'OHP, la réduction des données

, Frédéric Arenou sur une méthode de sélection d'étoiles pour MIOSOTYS (voir chapitre 5)

, Enseignement et diffusion de la culture scientifique En parallèle de ma thèse, j'ai été moniteur durant deux ans (j'ai commencé en deuxième année), composé d'amateurs, de chercheurs, de doctorants, Annexe, vol.6

, Durant ces deux années de monitorat, j'ai également participé aux nuits des planètes

N. Soleil and . Galiléennes, nuits des chercheurs, journées du patrimoine, nuits des étoiles, en donnant des conférences, en animant des observations publiques et en menant des animations pour les enfants

, J'ai également donné des conférences dans le cadre de la formation des maîtres

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