1. SETI By means of the Water MASER Radio-Emission at 22 GHz
C.B.Cosmovici, IAPS / INAF Roma

3. Water Maser emission during the Jupiter impact
of Comet Shoemaker-Levy 9

10. Comparative spectra of Epsilon Eridani: on the left hand the data acquired with the SPECTRA-2 backend show a clear detection with a SNR > 4; on the right hand, the same target was simultaneoulsy acquired with the old spectrometer MSPEC0 used for the Jupiter – Comet impact
Both spectra were obtained by means of a similar instrumental and antenna setup. Please note that MSPEC0 was not able to detect any visible feature.

11. Spectrum of the exoplanetary target Lalande observed at a frequency of 22 GHz, with the Noto INAF-IRA radiotelescope.

12. Gliese 581, Noto, 30-08-2012. Boxcar filter
Gliese 581, Noto, Boxcar filter. SNR = 5, FWHM=44kHz, vrad=0.4 km/s

13. Present and Future Extrasolar Planet Search
Optical Spectroscopy: gravitational wobbling
Optical Photometry I: occultation
Optical Photometry II: gravitational microlensing
Radio : MASER Emission
Space Interferometry: direct imaging