The table contains all the sdB stars observed during the NOT survey that were not identified as pulsators. It provides coordinates, details of the photometric sequences, and on the variability for each object. (1 data file).

It is known the fusion cross section plays crucial role in the choice of the reaction to synthesize new superheavy elements. An estimation of the fusion cross section in the reactions with massive nuclei is difficult task when the mass (charge) and angular distributions of the quasifission and fusion-fission fragments strongly overlap. The measured

Not Available

Not Available

Not Available

We present preliminary results of line identification and equivalent width measurements in spectra of late M Dwarfs. We obtained 3.5 nights on Keck NASA time to collect high resolution (R 20,000) near-infrared (J-band) spectra using the NIRSPEC instrument on the Keck II telescope. Our sample consists of 40 nearby (distance 20 pc) late M dwarfs