A first characterization of a 1100 g sapphire bolometer, performed at sea l
evel and at a working temperature of 40 mK, is presented. Despite perturbat
ions coming from the high-radioactive background and cosmic rays, calibrati
on spectra could be achieved with an internal alpha source and a Co-57 gamm
a-ray source: the experimental threshold is 25 keV, while the FWHM resoluti
on is 17.4 keV for the 122 keV peak. Possible heat release effects are disc
ussed, and a new limit of 9 x 10(-14) W/g is obtained for sapphire. (C) 199
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