1. 26-29 March, 2007Arena Workshop, Tenerife1 SIAMOIS Sismomètre Interférentiel A Mesurer les Oscillations des Intérieurs Stellaires Seismic Interferometer to Measure Oscillations in the Interior of Stars Tristan Buey, Benoît Mosser, Claude Catala, Pernelle Bernardi, Jean-Christophe Leclech, Alain Piacentino, Thierry Appourchaux, Jean-Pierre Maillard, François-Xavier Schmider, Jean-Baptiste Daban, François Fressin, Frédéric Thévenin, Stéphane Charpinet, Michel Dupieux, Denis Fappani, Philippe Mathias et al. Observatoire de Paris/LESIA, IAS, UNSA/LUAN, OMP/LATT, IAP, OCA

2. 26-29 March, 2007Arena Workshop, Tenerife2 Asteroseismology Two methods : photometry = space-based observations spectrometry = ground-based observations Advantages of Doppler measurements:- complementary observations Bright stars Low mass stars reduced granulation noise, modes l=3 Scientific requirements: continuous observations & long duration

3. 26-29 March, 2007Arena Workshop, Tenerife3 SIAMOIS at Dome C Observing conditions Consequences SeeingFibre = 5" on the sky No big telescope available at Dome C Science with a 40-cm telescope Only circumpolar targetsEnough interesting bright targets for more than 6 winters Duty cycle ~ 90% !Scientific specification #1 : duty cycle > 85% Polar night = 3 monthsScientific specification #2 : 100-day long run on the same target Demanding site Project ~ spatial organization Quasi-automatic, simple setup Reduced mass, power, telemetry

4. 26-29 March, 2007Arena Workshop, Tenerife4 Instrument Thermo-mechanical structure. Optical bench. Interferometer Camera Dedicated Telescope Bonnette Calibration Optical fibers : signal and calibration Command/control system: Acquisition,image processing … Vacuum pump

5. 26-29 March, 2007Arena Workshop, Tenerife5 Overall description Divided in four sub-systems : –a dedicated Telescope with its Bonnette (telescope guiding and fiber coupling). –an Interferometer and a CCD Camera. –a structure for thermal and mechanical control. –a command/control software system (CCS). Divided among five laboratories : –GIGT / OMP (Observatoire Midi-Pyrénées): Bonnette –LUAN / OCA (Observatoire Côte d’Azur): Telescope –IAS (Institut d’Astrophysique Spatiale): Thermal structure –LESIA / OPM (Observatoire Paris-Meudon): Interferometer –CSIC from Institutode Astrofisica de Andalusia (in discussion).CCS One associated private contractor : –SESO (Société Européenne de Systèmes Optiques).Optics

6. 26-29 March, 2007Arena Workshop, Tenerife6 Instrument 40-cm telescope low cost, dedicated to the project Interferometer monolithic instrument no moving parts, reduced size fiber fed Post-dispersion efficiency, photon noise limited performances, wide spectral range from 400 to 560nm. Optical Fiber For more technical details have a look at the poster.

7. 26-29 March, 2007Arena Workshop, Tenerife7 Planning 2006 - design - Achievement of the feasibility phase. 2007 - thermo-mechanical analysis - Qualification tests. 2008 - PDR - FDR 2009 - integration 2010 - tests - summer campaign: Dome C 2011 - first winter at Dome C Cost : 860 k€ Including ANR : 460 k€ For phase A in 2006 (ACI + CSA + PNPS) : 116 k€

8. 26-29 March, 2007Arena Workshop, Tenerife8 The constraints Of development: Small budget and short planning… Observation requirements : 90% of duty cycle. Of the site: Very difficult to fix anything at Dome C Wintering assumes a minimum maintenance. Rather hard environmental conditions; large temperature range, long travel to the site; shocks and vibrations. Design: Highly reliable instrument with easy set up and maintenance. Qualification like a space instrument for the critical components Commercial approach for the delivery Minimal customization and technological developments. Fully automated instrument for the main (and very simple) mode of observation. Spares to replace the malfunctioning elements.

9. 26-29 March, 2007Arena Workshop, Tenerife9 Response to the Dome-C constraints Qualification : Telescope and bonnette outside --> Fully qualified (-100°C/+25°C). Mechanical bench, thermal control --> No need to be qualified. Optical components --> Light qualification(-30°C/+25°C), care during transportation, inside a heated shelter. Simplification : The instrument is completely tested and set up before arriving in Dome-C. Only standard mechanical integration and simple good health tests are needed. Apart from calibration modes at the beginning of the observation, only one observation mode, requiring no human intervention (or by remote control). Apart from the active tracking control loop, no complex control inside the instrument, no critical moving parts (simple shutter). Specific optical fiber connector to be qualified (soon) at -100°C.

10. 26-29 March, 2007Arena Workshop, Tenerife10 Response to the Dome-C constraints Automation: Pointing and tracking star: Telescope may point a region of the sky, the bonnette uses a guiding CCD to track the target (control loop). The telescope makes a U-turn every 24 hours to follow the movement of the Earth (specific mechanism allows the rolling-up of the cables). Frame Acquisition: the spectra are automatically acquired by the control/command system with all the house-keeping of the instrument. The thermal control is based on a simple heating system and passive filtering and is naturally automatic. The mechanical control is based on active autonomous suspension. The data during the main observation mode are processed via a constant pipeline for: visualization (remote control), data sending to Europe, storage.

11. 26-29 March, 2007Arena Workshop, Tenerife11 The Command/Control System First estimation around 200ko/day

12. 26-29 March, 2007Arena Workshop, Tenerife12 Dome C: a unique site for Asteroseismology 3-month of continuous observation with duty cycle ~ 90% A specific scientific program after High performances possible with a 40-cm collector –Pioneering project at Dome C –FT seismometer: suitable concept for installation and setup at Dome C –Multiplex advantage of FT spectrometry –Small instrument : < 300kg, < 2m 3, < 1kW, … –Fairly fast development with a demonstrated feasibility. –Fully automated for the main observational mode. Conclusion ‘‘Big science’’ at Dome C with a budget < 1 M€, with little maintenance and limited human intervention.