Ana Laura O'Mill, Fernanda Duplancic, Diego García Lambas, Carlos Valotto, Laerte Sodré Jr
We present a new catalogue of galaxy triplets derived from the Sloan Digital
Sky Survey Data Release 7. The identification of systems was performed
considering galaxies brighter than M_r=-20.5 and imposing constraints over the
projected distances, radial velocity differences of neighbouring galaxies and
isolation. To improve the identification of triplets we employed a data
pixelization scheme, which allows to handle large amounts of data as in the
SDSS photometric survey. Using spectroscopic and photometric data in the
redshift range 0.01View original: http://arxiv.org/abs/1111.6971
No comments:
Post a Comment